Strong and Electroweak Matter 2016
University of Stavanger
Update 29.07.2016: Check out some photos of the conference and of the region around Stavanger! Feel free to send us your photos  either directly or a link to an online album  and we will create a page to link to them.
The focus of the conference was the theory of the Standard Model and beyond at finite temperature and density and out of equilibrium, including applications to cosmology, astrophysics and relativistic heavyion collision experiments. Among the topics to be discussed are:
 QCD in extreme conditions and dense nuclear matter
 Baryogenesis and leptogenesis
 Heavyion collisions and the QuarkGluon Plasma
 Quantum fields out of equilibrium and thermalization
 Electroweak phase transition beyond the Standard Model
 Early Universe physics and sources for gravitational waves
 Quantum field dynamics and inflation
With the following invited speakers:
 Frank Wilczek [MIT]
 Dietrich Bödeker [Bielefeld]
 Paolo Creminelli [ICTP]
 Gergely Endrődi [Frankfurt]
 Mark Hindmarsh [Sussex]
 Aleksi Kurkela [CERN]
 Jose M. No [Sussex]
 Sami Nurmi [Jyväskylä]
 Troels C. Petersen [Copenhagen/ATLAS]
 Claudia Ratti [Houston]
 Dieter Röhrich [Bergen/ALICE]
 Andreas Schmitt [Southampton]
 Geraldine Servant [DESY]
 Mikhail Shaposhnikov [Lausanne]
 Jaroslav Trnka [UC Davis]
 Raju Venugopalan [BNL/Heidelberg]
 Bin Wu [Ohio State]
 Naoki Yamamoto [Keio]
The conference will be held on campus at University of Stavanger.
The organisers can be contacted by email at contact@sewm2016.org.
You can download our poster or the timetable as PDFs.
 Akihiko Monnai
 Aleksi Kurkela
 Aleksi Vuorinen
 Alexander Rothkopf
 Anders Haarr
 Anders Tranberg
 Andreas Helset
 Andreas Hohenegger
 Andreas Ipp
 Andreas Schmitt
 Andreas Windisch
 Angel Gomez Nicola
 Angelo Ricciardone
 Anton Rebhan
 Antonio Dobado
 Asgeir Osland
 Attila Pasztor
 Ayan Mukhopadhyay
 Bin Wu
 Björn Garbrecht
 BumHoon Lee
 Caglar Dogan
 Christoph Groß
 Christopher Harman
 Claudia Ratti
 Cristina Manuel
 Daniil Gelfand
 David Weir
 Dieter Röhrich
 Dietrich Bödeker
 Edmond Iancu
 Florian Divotgey
 Florian Preis
 Frank Wilczek
 Geraldine Servant
 Gergely Endrődi
 Gergely Marko
 Germano Nardini
 Gert Aarts
 Guy Moore
 Jacopo Ghiglieri
 Jamie McDonald
 Jaroslav Trnka
 Jason Tsz Shing Yue
 jeanloic kneur
 Jens Oluf Andersen
 JonIvar Skullerud
 Jose Miguel No
 Julien Serreau
 Juraj Klaric
 Jürgen Eser
 Kirill Boguslavski
 Kohtaroh Miura
 Konrad Tywoniuk
 Krzysztof Kutak
 Laurence Yaffe
 Mandy M. Wygas
 Manuel Meyer
 Margaret Carrington
 Mark Bogers
 Mark Hindmarsh
 Martin Jakobsen
 Masahiro Takimoto
 Matias Säppi
 Maxime Guilleux
 maximilian attems
 Mikhail Shaposhnikov
 Mikko Laine
 Naoki Yamamoto
 Niklas Mueller
 Olli Koskivaara
 Paolo Creminelli
 Patrick Kneschke
 Per Amund Amundsen
 Peter Arnold
 Raju Venugopalan
 Rasmus Larsen
 Sami Nurmi
 Savvas Zafeiropoulos
 Shi Pu
 Shu Lin
 Stanislaw Mrowczynski
 Stefan Stricker
 Stephen Stopyra
 Thomas Degrand
 Thomas Garratt
 Tobias Rindlisbacher
 Tomas Brauner
 Tomoya Hayata
 Troels Petersen
 Tuomas Tenkanen


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Lunch 55m Aula
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Welcome G001
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Plenary G001
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University of Stavanger
Arne Rettedal buildingConvener: Tomas Brauner (University of Stavanger)
13:30
Overview of ATLAS & CMS: Experiments, Techniques, and Results 1hSpeaker: Troels Petersen (NBI)

14:30
Recent results from the LHC heavy ion programme 1h
A brief overview of the ultrarelativistic heavy ion physics programme at the Large Hadron Collider at CERN will be given. Collisions of lead ions have been studied at a centerofmass energy per nucleon of 2.76 TeV (run I), and, more recently, at 5.02 TeV (run II). The ultimate goal of heavyion collisions is the study of the properties of the deconfined and chirally restored state of matter known as the QuarkGluon Plasma. Various probes are used to characterize the properties of the QGP  from collective effects and direct photons to heavy quarks and jets. Main highlights from run I and recent results from run II will be presented.
Speaker: Dieter Rohrich (Department of Physics & TechnologyUniversity of Bergen)

13:30

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Coffee 30m Aula
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Plenary G001
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University of Stavanger
Arne Rettedal buildingConvener: Tomas Brauner (University of Stavanger)
16:00
Recent results on lattice QCD thermodynamics 1h
I review recent results on QCD thermodynamics from lattice simulations. In particular, I will focus on the QCD equation of state at zero and finite chemical potential, the curvature of the phase diagram and fluctuations of conserved charges. The latter will be compared to experimental data, to the purpose of extracting the chemical freezeout temperature and chemical potential from first principles.
Speaker: Claudia Ratti (University of Houston) 
17:00
Probes of the Electroweak Phase Transition and Baryogenesis at the LHC 45m
Uncovering the nature of the electroweak (EW) phase transition in the early Universe would be key to shed light on the possible origin of the cosmic matterantimatter asymmetry. We discuss various ways in which searches for new physics beyond the Standard model at the LHC can be used to probe the nature of the EW phase transition, and their implications for the generation of the baryon asymmetry of the Universe at the EW scale.
Speaker: Jose Miguel No (University of Sussex)

16:00

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Plenary G001
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University of Stavanger
Arne Rettedal buildingConvener: Mikhail Shaposhnikov (EPFL)
09:00
Geometric picture for scattering amplitudes 45m
There has been a growing evidence that the standard formulation of Quantum Field Theory using path integrals and Feynman diagrams fails to explain unexpected simplicity and hidden symmetries of the scattering amplitudes. I show that in a certain gauge theory there exists a radically different picture for amplitudes as volumes of "Amplituhedron" which is a higherdimensional generalization of convex polygons. I will also comment on the extension of this approach to other theories.
Speaker: Jaroslav Trnka (UC Davis) 
09:45
Electroweak baryogenesis from dynamical CKM matrix 45m
There are good motivations to consider that the flavour structure could emerge during electroweak symmetry breaking, for example if the FroggattNielsen field dynamics were linked to the Higgs field. Remarkably, the the nature of the electroweak phase transition is completely changed when the Standard Model Yukawas vary at the same time as the Higgs is acquiring its vacuum expectation value, starting from order one values in the symmetric phase to reach their present values at the end of the phase transition. The thermal contribution of the fermions creates a barrier between the symmetric and broken phase minima of the effective potential, leading to a firstorder electroweak phase transition. Besides, in this framework, the CKM matrix is the unique and sufficient CPviolating source for baryogenesis. This offers new routes for generating the baryon asymmetry at the electroweak scale, strongly tied to flavour models.
Speaker: Geraldine Servant (Deutsches ElektronenSynchrotron (DE))

09:00

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Coffee 30m Aula
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Plenary G001
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University of Stavanger
Arne Rettedal buildingConvener: Mikhail Shaposhnikov (EPFL)
11:00
The first Fermi of a HeavyIon Collision: results, puzzles, and opportunities 45mSpeaker: Raju Venugopalan (Brookhaven National Laboratory)

11:45
Vacuum stability and early universe physics 45m
Stability of the electroweak vacuum in the very early universe is a novel probe of high energy physics. A key question
is whether new physics beyond SM is required to maintain stability against inflationary fluctuations of the Higgs field.
Here curvature couplings induced by radiative corrections in curved space play a crucial role. I review the topic and show
that curvature effects can keep the electroweak vacuum stable in the early universe without any new physics. I also comment
on the use of vacuum stability as a new test for SM extensions and discuss the observational imprints of inflationary
Higgs fluctuations.Speaker: Sami Nurmi (University of Jyväskylä)

11:00

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Lunch 1h Aula
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Parallel Track 1 Ø110
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University of Stavanger
Arne Rettedal buildingConvener: Dietrich Bödeker (Bielefeld University)
13:30
Dijet production as a probe of dense partonic system 30m
In order to investigate structure of Pb nuclei at high energies we study forward dijet production in pPb hadronic collisions.
We propose a framework for evaluating cross section for production of forward dijets that encompasses Color Glass Condensate and high energy factorization effects and is therefore applicable regardless of the magnitude of transversal momenta of produced jets.
The framework is based on the generalization of the Transversal Momentum Dependent Factorization formula for dijet production.
Furthermore we provide fenomenological results for nuclear modification ratios using the developed framework.Speaker: Krzysztof Kutak (Instytut Fizyki Jadrowej Polskiej Akademii Nauk) 
14:00
Eventbyevent picture for the mediuminduced jet evolution 30m
We discuss the evolution of an energetic jet which propagates through a dense quarkgluon plasma
and radiates gluons due to its interactions with the medium. Within perturbative QCD,
this evolution can be described as a stochastic branching process, that we have managed to solve exactly.
We present exact, analytic, results for the gluon spectrum (the average gluon distribution)
and for the higher npoint functions, which describe correlations and fluctuations.
Using these results, we construct the eventbyevent picture of the gluon distribution produced via mediuminduced gluon branching.In contrast to what happens in a usual QCD cascade
in vacuum, the mediuminduced branchings are quasidemocratic, with offspring gluons carrying sizable fractions of the energy of their parent parton. This results in wave turbulence 
an efficient mechanism for the transport of energy from the jet towards the medium.
This mechanism is characterized by a powerlaw (Kolmogorov) spectrum
and by large fluctuations in the energy loss and the multiplicity
of soft gluons. The multiplicity distribution is predicted to
exhibit KNO (KobaNielsenOlesen) scaling. These predictions can be tested
in Pb+Pb collisions at the LHC, via eventbyevent measurements of the dijet asymmetry.Based on ePrint: arXiv:1601.03629 [hepph] published in JHEP 1605 (2016) 008
Speaker: Dr. Edmond Iancu (IPhT Saclay) 
14:30
Energy Loss in Unstable QuarkGluon Plasma 30m
The momentum distribution of quarkgluon plasma at the early stage of a relativistic heavyion collision is anisotropic and consequently the system, which is assumed to be weakly coupled, is unstable due to chromomagnetic plasma modes. We consider a highenergy parton which flies across such an unstable plasma, and the energy transfer between the parton and the medium is studied as an initial value problem. In the case of equilibrium plasmas, the wellknown formula of collisional energy loss is reproduced. The unstable plasma case is much more complex, and the parton can lose or gain energy depending on the initial conditions. The extremely prolate and extremely oblate systems are considered as examples of unstable plasmas, and two classes of initial conditions are discussed. When the initial chromodynamic field is uncorrelated with the color state of the parton, it typically looses energy, and the magnitude of the energy loss is comparable to that in an equilibrium plasma of the same density. When the initial chromodynamic field is induced by the parton, it can be either accelerated or decelerated depending on the relative phase factor. With a correlated initial condition, the energy transfer grows exponentially in time and its magnitude can much exceed the absolute value of energy loss in an equilibrium plasma. The energy transfer is also strongly directionally dependent. Consequences of our findings for the phenomenology of jet quenching in relativistic heavyion collisions are briefly discussed.
Speaker: Stanislaw Mrowczynski (Jan Kochanowski University) 
15:00
Thermal contributions to the soft dijet function 30m
We present the first analysis of event shape distributions in e+e annihilation into a dijet pair in a hightemperature quarkgluon plasma in thermal equilibrium. We focus on temperatures much smaller than the jet mass, such that the jet function remains unresolved by medium fluctuations. In this limit, the medium influences the crosssection of the process only through the dijet soft function that describes the interjet activity and is a central ingredient for several event shape observables, such as thrust and jet mass distributions. Concretely, we calculate moments of the soft function by extracting the expectation values of energy flow operators, that are in turn closely related to energyenergy correlations. We demonstrate that, at nexttoleading (g^2) order, the thermal contribution to the moments of the hemisphere mass distribution factorise, which allows us to resum all moments and thus reconstruct the full soft function. Finally, we comment on higherorder (g^4) corrections and the relevance of event shape observables in the context of the ongoing ultrarelativistic heavyion experiments.
Speaker: Konrad Tywoniuk (CERN)

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Parallel Track 2 Ø120
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University of Stavanger
Arne Rettedal buildingConvener: Prof. Anton Rebhan (Technische Universität Wien)
13:30
Semiholography for heavy ion collisions 30m
I will present the recent developments [JHEP05(2016)141] of the semiholographic model first proposed in [JHEP06(2015)003]. The semiholographic approach makes it possible to combine Color Glass Condensate initial conditions and weakcoupling glasma field equations with a simultaneous evolution of a strongly coupled infrared sector describing the soft gluons radiated by hard partons. The new developments presented here include selfconsistent couplings between the CGC framework and an infrared AdS/CFT sector, such as to guarantee the existence of a conserved energymomentum tensor for the combined system that is local in space and time. Moreover, we include a coupling of the topological charge density in the glasma to the same of the soft sector. As a first numerical test of a of the iterative numerical procedure suggested earlier we study the dynamics of fluctuating homogeneous colorspinlocked YangMills fields when coupled to a homogeneous and isotropic energymomentum tensor of the soft sector.
Speaker: Mr. Florian Preis (Technische Universität Wien) 
14:00
Monitoring shock wave collisions with non local observables 30m
Understanding the complicated field dynamics taking place in a heavy ion collision is a difficult task. Holography provides us with a framework that enables us to study the strongly coupled sector of certain gauge theories.
We mimic the heavy ion collision by two gravitational shock waves and monitor the time evolution of the dual strongly coupled super YangMills plasma via nonlocal observables such as twopoint functions and entaglement entropy.
Different initial conditions exhibit different phenomenology with respect to nonlocal observables. We show that entanglement entropy can be used as an order parameter to distinguish between the two phases of the crossover from the transparency to the fullstopping scenario in dynamical YangMills formation.Speaker: Stefan Stricker (TU Wien) 
14:30
Collisions in Nonconformal Theories: Hydrodynamization without Equilibration 30m
Ever since fast hydrodynamization has been observed in heavy ion collisions the understanding of the very early nonequilbrium stage of such collisions has been a topic of intense research. We use the gauge/string duality to model the creation of a strongly coupled QuarkGluon plasma in a nonconformal gauge theory. We focus on new physics (as compared to the conformal case) such as the nontrivial equation of state and the presence of a sizeable bulk viscosity. Nonconformality gives rise to an increase of the relaxation times of the resulting plasma. Furthermore, if the bulk viscosity is large enough then the plasma becomes well described by hydrodynamics before the equilibrium equation of state becomes applicable.
Speaker: maximilian attems (University of Barcelona) 
15:00
Thermalization of SchwingerKeldysh correlation functions in hologrpahy 30m
Holography provides a powerful tool for studying outofequilibrium strongly interacting quantum fields. Most works on this subject have focused on the dynamics of local operators, as for instance on how quickly they approach hydrodynamic behavior. We have developed the first general method for studying timedependence of the causal response function in holography for arbitrary nonequilibrium states and external quench protocols by vastly improving preexisting methods. This method has been further extended for obtaining all nonequilibrium SchwingerKeldysh correlation functions (to appear soon). We will present results on the timedependence of the spectral function in AdSVaidya geometries dual to nonequilibrium states driven by a homogeneous quench of an arbitrary duration. Unlike the onepoint functions, the spectral function exhibits four distinct patterns of timedependence (initial time dynamics and thermalization) characterized by very welldefined features going to be described. It can be readily argued that holography can help us to classify patterns of thermalization of correlation functions in strongly coupled largeN theories based on a few simple combinations of extrinsic and intrinsic parameters, in a manner analogous to how we use the Reynolds number to classify hydrodynamic flows. We will discuss connections with solidstate experiments and heavyion physics.
Speaker: Ayan Mukhopadhyay (Vienna University of Technology)

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Parallel Track 3 Ø130
Ø130
University of Stavanger
Arne Rettedal buildingConvener: Julien Serreau (Université Paris Diderot)
13:30
The effects of higher order truncations in the 2PI description of phase transitions 30m
We thoroughly investigated the applicability of the twoparticle irreducible
(2PI) formalism in the description of phase transitions occurring at finite temperature in scalar field theories. We studied the importance of truncation effects on the order of the phase transition and indeed found that the long known problem of the HartreeFock truncation is cured by improving the approximation to the next level. during the investigation of BoseEinstein condensation at finite density we found infrared problems one might face in the selfconsistent treatment of the propagators. We studied this problem in more detail developing various semianalytical localized approximations. We have shown within a truncation at twoloop level that the socalled symmetry improved 2PI, recently proposed in the literature to enforce the Goldstone theorem on the variational propagator, results in a loss of solution to the selfconsistent propagator equations because the resummation cannot cope with the deep IR modes. We think that the most likely way out for this rather general problem is to employ vertex resummations e.g. using 1/N expansion to next to leading order in the 2PI effective action.Speaker: Gergely Marko (MTAELTE Statistical and Biological Physics Research Group) 
14:00
Nonequilibrium dynamics of inhomogeneous quantum fields 30m
The dynamics of inhomogeneous quantum fields out of equilibrium are especially relevant for the study of firstorder phase transitions. It is our aim to calculate how critical bubbles of the new phase that form in such a process propagate for different quantum field theories. The Electroweak phase transition in the early universe is of particular interest, since Baryogenesis can potentially explain the matterantimatter asymmetry in the universe for fitting dynamical properties of the phase transition and the bubble collisions result in gravitational waves.
To simulate the bubble dynamics we have developed a program that solves the nonequilibrium equations of motion in the so called 2PIFormalism. As a starting point we have simulated the dynamics of bubbles in a scalar $\lambda_{4} \phi^{4} + \lambda_{6} \phi^{6}$ toy model in (1+1)dimensions.Speaker: Thomas Garratt (JuliusMaximilians Universitaet Wuerzburg) 
14:30
Renormalization of $\phi^4$theory in the 2PI Hartree approximation scheme for nonvanishing background field 30m
In the study of phase transitions in the early universe, methods based on $N$ particle irreducible effective actions have become very important for describing the out of equilibrium dynamics of these phenomena. Equations of motion for classical 1, up to $N$point functions can be obtained from stationarity conditions. However, in order to extract physical information, the action must first be renormalized. Selfconsistent schemes for doing so have been presented in the literature. Typically, when performing the renormalization, it is assumed that the classical field vanishes. We have adopted the renormalization procedure presented by Berges et al. [arXiv:hepph/0503240], applying it to a $\phi^4$ toy model and explicitely perform the renormalization in the Hartree approximation, assuming a nonvanishing classical field.
Speaker: Christoph Groß (JuliusMaximilians Universität Würzburg) 
15:00
Nexttoleading order nPI calculations in scalar theories 30m
Previous calculations have shown that the 2 particle irreducible (2pi) effective theory is a promising method to study strongly coupled systems, for which nonperturbative techniques are needed. Calculations at the 3 loop level show improved convergence, relative to perturbative results. We present results in \phi^4 theory at the 4 loop level which show that convergence breaks down at large coupling. This indicates the need for higher order effective theories.
4pi calculations in 4 dimensions have never been attempted, because no method is known to deal with the overlapping subdivergences that appear in these theories. We present a new technique to renormalize the 4pi effective theory, based on a renormalization group approach.Speaker: Margaret Carrington (Brandon University)

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Coffee 30m Aula
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IAC Meeting (IAC members only) 1h

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Public talk: Public talk  Frank Wilczek  "Some Intersections of Art and Science" G001
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Plenary G001
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University of Stavanger
Arne Rettedal buildingConvener: Alexander Rothkopf (Heidelberg University)
09:00
Effective field theory techniques applied to the hard scales of the plasmas 45m
We show that effective field theory techniques can be applied
in the high temperature T plasmas to
improve the accuracy of the physics of the hard scales ( or scales of order T).
At leading order in the
coupling constant the hard scales of the plasma can be viewed as
onshell classical particles. Based on this observation, and without any
reference
to the state of the system, we derive an effective field
theory describing the quantum fluctuations around an onshell fermion with
energy p, described as a set of high dimension operators over the onshell energy
p. When applied to systems close to equilibrium, when for most onshell particles p ~ T,
we show that the
onshell effective field theory (OSEFT) properly describes the HTL photon
polarization tensor of QED, and its 1/T corrections. We also show how with
the OSEFT one can derive quantum corrections
to classical transport equations.Speaker: Cristina Manuel (CSICIEEC) 
09:45
Axions: The Unfinished Business of QCD 1hSpeaker: Frank Wilczek (MIT)

09:00

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Coffee 30m Aula
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Plenary G001
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University of Stavanger
Arne Rettedal buildingConvener: Alexander Rothkopf (Heidelberg University)
11:15
EFT and its applications in cosmology 45mSpeaker: Paolo Creminelli (ICTP)

12:00
Topological transport phenomena in strong and electroweak matter 45m
Chirality of fermions has a topological nature. This microscopic property modifies the macroscopic hydrodynamic behavior and leads to unusual transport phenomena protected by topology in relativistic systems. We show how conventional kinetic theory should be modified to take into account such effects. We also discuss their potential importance in strong and electroweak matter, and, in particular, in the evolution of supernovae.
Speaker: Naoki Yamamoto (Keio University)

11:15

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Lunch 1h Aula
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Parallel Track 1 Ø110
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University of Stavanger
Arne Rettedal buildingConvener: Jens Oluf Andersen
13:45
Baryons across the deconfinement transition 30m
Surprisingly, unlike mesonic correlators, baryonic correlators at nonzero temperature have only been studied in a handful of studies. Here we present a lattice study of baryonic correlators and spectral functions across the deconfinement transition, using FASTSUM's 2+1 Wilson ensembles. We present results for inmedium effects below Tc and parity doubling above Tc.
Speaker: Gert Aarts (Swansea University) 
14:15
Dense 2colour QCD towards the continuum limit 30m
We report on simulations of 2colour QCD with Nf=2 Wilson fermions at nonzero chemical potential and temperature. We present results for the diquark condensate, Polyakov loop and quark number density on finer lattices than those previously reported, as well as ongoing simulations with smaller quark masses. Our results confirm the existence of a "quarkyonic" phase at high density, while the putative lowtemperature, highdensity deconfinement transition appears to recede as the continuum limit is approached. There are indications of a BEC region opening up at intermediate chemical potentials as the quark mass is lowered.
Speaker: JonIvar Skullerud (National University of Ireland Maynooth) 
14:45
QCD critical point and thermal photons 30m
The beam energy scan programs at BNL Relativistic Heavy Ion Collider open up a new opportunity to explore the quarkgluon plasma (QGP) at finite densities. The quantitative success of hydrodynamic modeling motivates one to extend the model to lower energies to verify its applicability, to study the transport properties at finite densities, and ultimately to understand the phase structure of QCD, including the longsought critical point.
One of the problems in the search for the critical point is that its signal in hadronic observables would be washed away if its location is far from freezeout even if it exists. In this work, we propose to study thermal photon spectra and elliptic flow at finite baryon density using a (2+1)dimensional hydrodynamic model. We investigate a possible signal of the QCD critical point in those observables because it would be visible regardless of its location on the $T$$\mu$ plane owing to the fact that the QGP medium is electromagnetically transparent.
Speaker: Akihiko Monnai (Institut de Physique Théorique, CNRS/CEA) 
15:15
Equation of state of QCD from analytical continuation 30m
We determine the 2+1 flavour equation of state of QCD at finite chemical potential to order $(\mu_B/T)^6$ from lattice simulations. The simulations are performed at
the physical mass for the light and strange quarks on several lattice spacings;
the results are continuum extrapolated. The coefficients of the expansion in
$(\mu_B/T)$ are determined through the analytic continuation from imaginary chemical potentials of the baryonic density. Strangeness neutrality and charge conservation are imposed, to match the experimental conditions at heavy ion colliders. The pressure and interaction measure are calculated along the isentropic trajectories in the $(T, \mu_B)$
plane corresponding to the RHIC Beam Energy Scan collision energies.Speaker: Attila Pasztor (Wuppertal University)

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Parallel Track 2 Ø120
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University of Stavanger
Arne Rettedal buildingConvener: Aleksi Vuorinen
13:45
Quantum inferference in showering: LPM effect for sequential bremsstrahlung 30m
Highenergy particles passing through matter lose energy by showering via hard bremsstrahlung and pair production. At very high energy, the quantum duration of each splitting process, known as the formation time, exceeds the mean free time for collisions with the medium, leading to a significant reduction in the splitting rate, known as the LandauPomeranchukMigdal (LPM) effect. In the QCD case, there are important and potentially important corrections to the usual treatment of the LPM effect, arising from cases where the coherence lengths of two consecutive splitting processes overlap. I will discuss the computation of such corrections beyond leadinglog approximation.
Speaker: Peter Arnold (University of Virginia) 
14:15
Perturbative study of the QCD phase diagram for heavy quarks at nonzero chemical potential 30m
We investigate the phase diagram of QCD with heavy quarks at finite temperature and chemical potential in the context of background field methods. In particular, we use a massive extension of the LandauDeWitt gauge which is motivated by previous studies of the deconfinement phase transition in pure YangMills theories. We show that a simple oneloop calculation is able to capture the richness of the phase diagram in the heavy quark region, both at real and imaginary chemical potential. Moreover, dimensionless ratios of quantities directly measurable in numerical simulations are in good agreement with lattice results.
Speaker: Julien Serreau (Université Paris Diderot) 
14:45
scale invariant resummed perturbation at finite temperature 30m
We will illustrate how a nonperturbative variational technique combined with renormalization group (RG) properties efficiently resums perturbative expansions in thermal field theories. The resulting convergence and scale dependence of optimized thermodynamical quantities are drastically improved as compared to standard perturbative expansions, as well as to other related methods such as the screened perturbation or (resummed) hardthermalloop perturbation. Our general method will be illustrated for the scalar phi^4 model, and we will discuss also how it can be generalized to QCD.
Speaker: JeanLoic Kneur (Univ Montpellier) 
15:15
Towards a high statistics analysis of quarkonium at T>0 using NRQCD on realistic Nf=2+1 HISQ lattices 30m
Lattice QCD has has the potential to provide urgently needed first principles insight into the binding properties of heavy quarkonium inmedium, which form a central pillar of the experimental investigations of the quarkgluon plasma at the RHIC and LHC collider facilities.
Here we report on progress in our ongoing work to deploy the effective field theory NRQCD on current generation dynamical QCD lattices with Nf=2+1 light HISQ flavors at T>0, in order to ultimately extract the inmedium spectral properties of bbar and ccbar bound states around the phase transition and in the QGP regime.
In addition to previously published results on Bottomonium [1], we have investigated both correlator and spectral properties of Charmonium states [2] which showed a clear ordering of their inmedium modification, also among different flavors, according to the vacuum binding energy. Both computations are currently being extended [3] to higher temperatures, preliminary results of which are presented on this poster.
[1] S.Kim, P.Petreczky, A.R. Phys.Rev. D91 (2015) 054511
[2] S.Kim, P.Petreczky, A.R. arXiv:1511.04151, arXiv:1512.05289
[3] S.Kim, P.Petreczky, A.R. in preparationSpeaker: Dr. Alexander Rothkopf (Institute for Theoretical Physics, Heidelberg University)

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Parallel Track 3 Ø130
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University of Stavanger
Arne Rettedal buildingConvener: Mikko Sakari Laine (Universitaet Bern (CH))
13:45
Active and sterile neutrino dynamics below the electroweak crossover 30m
I will summarize a recent estimation (arXiv:1605.07720) of the thermal masses and damping rates of active (m < eV) and sterile (M ∼ GeV)
neutrinos with thermal momenta k ∼ 3T at temperatures below the electroweak crossover
(5 GeV < T < 160 GeV). These quantities in turn fix the washout rates of Standard
Model lepton number densities and the thermal production rate of sterile neutrinos. These interact via direct scatterings mediated
by Yukawa couplings, and via their overlap with active neutrinos. I will review the calculation, which includes all leading order reactions. I will show that the resulting washout rate generally exceeds the Hubble rate for 5 GeV
< T < 30 GeV. Therefore it is challenging to generate a large lepton asymmetry facilitating dark matter computations operating at T < 5 GeV, whereas the generation of a baryon asymmetry at T > 130 GeV remains an option.Speaker: Jacopo Ghiglieri (Universitaet Bern (CH)) 
14:15
Decay Rate of RightHanded Neutrinos in Light of Collective Excitations at Electroweak Scale 30m
The origin of the baryon asymmetry in the Universe (BAU) is a big mystery in particle physics and cosmology. One interesting scenario to explain BAU is the resonant leptogenesis which admits lepton number creation in the electroweakscale, and therefore, receives lots of phenomenological interests in the LHC era. Then, the decay of righthanded neutrinos which causes the lepton number must be evaluated in the electroweakscale plasma, where nontrivial collective excitations emerge due to coexistence of a mass scale induced by the Higgs mechanism and temperature. We investigate the decay rate of righthanded neutrinos with respect to such collective modes providing novel decay channels for the righthanded neutrinos. The collective excitation has been well investigated in the physics of the quarkgluon plasma (QGP), and the subject in this presentation would provide a bridge between the leptogenesis and the QGP community.
Speaker: Dr. Kohtaroh Miura (CPT, AixMarseille Universite) 
14:45
Leptogenesis and gravity: baryon asymmetry without decays 30m
Explaining the matterantimatter asymmetry of the Universe remains one of the most intriguing problems in particle physics and cosmology. A popular class of theories attributes this asymmetry to CPviolating decays of superheavy particles in the Early Universe. We present a new source of baryogenesis within these models, and show how the same Yukawa phases which provide the CPviolation for decays, combined with curvedspacetime loop effects, allow matter and antimatter to fall differently in the presence of gravity. This splits the energy spectrum for matter and antimatter, driving the system towards an asymmetric state. By analysing the full Boltzmann equation, we demonstrate regions of parameter space where the observed asymmetry is produced solely by gravitational effects, with decays playing no part at all.
Speaker: Mr. Jamie McDonald (Swansea University) 
15:15
Leptogenesis in GeV seesaw models with large mixing angles 30m
We consider the dynamics of the standard model extended by two or more right
handed neutrinos, which simultaneously explains the origin of neutrino masses
through the seesaw mechanism and the baryon asymmetry of the universe
through leptogenesis.
Specifically, we focus on right handed neutrinos with GeV scale mass which can
be found in collider or fixed target experiments.
We use quantum kinetic equations to calculate the baryon asymmetry produced
through righthanded neutrino oscillations in the early universe, and predict
their properties from the requirement to explain the observed baryon asymmetry
of the universe.
By identifying the time scales of oscillations and equilibration, and
comparing them we find two regimes of production.
The oscillatory regime, where the oscillations happen much earlier than the equilibration of the right handed neutrinos, which is suitable for calculating
the baryon asymmetry for regions of parameter space where the mixing between
the left and righthanded neutrinos is small.
For large mixing angles we find the overdamped regime,
where one of the right handed neutrinos typically reaches equilibrium before
the oscillations among the right handed neutrinos begin.
We develop analytic approximations for each of the two regimes, and use them
to derive predictions of the right handed neutrino properties if they are
responsible for the origin of matter.Speaker: Mr. Juraj Klaric (Technische Universität München)

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Coffee 30m Aula
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Excursion and dinner 5h
NB: the boat departs from the quay (Skagenkaien) at 18.00. No alternative transportation!

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Plenary G001
G001
University of Stavanger
Arne Rettedal buildingConvener: Jacopo Ghiglieri (Universitaet Bern (CH))
09:00
Gravitational waves and eLISA 45mSpeaker: Mark Hindmarsh (University of Sussex)

09:45
Jet evolution in dense QCD matter 45m
I discuss the physical picture for the evolution of a highenergy jet in a hot quarkgluon plasma, with emphasis on our latest results on this topic. A complete picture of jet evolution includes both coherent gluon emissions and incoherent emissions. We find a double logarithmic contribution from coherent gluon emissions. The resummation of such leading double logs can be absorbed into a renormalized transport coefficient \hat{q} (the celebrated jet quenching coefficient). Such a radiative correction significantly enhances the value of \hat{q}, with important consequences for the studies of jet quenching in ultrarelativistic heavyion collisions. In the second part of my talk, I discuss the jet evolution via incoherent multiple branching and thermalization of the soft branching products. I argue that the following scenario should hold: the leading particle emits a significant number of minijets which promptly evolve via multiple branchings and thus degrade into a myriad of soft gluons, with energies of the order of the medium temperature T. Via elastic collisions with the medium constituents, these soft gluons relax to local thermal equilibrium with the plasma over a time scale which is considerably shorter than the typical lifetime of the minijet. The thermalized gluons form a tail which lags behind the hard components of the jet.
Speaker: Bin Wu (Ohio State)

09:00

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Coffee 30m Aula
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Plenary G001
G001
University of Stavanger
Arne Rettedal buildingConvener: Jacopo Ghiglieri (Universitaet Bern (CH))
11:00
Leptogenesis 45mSpeaker: Dietrich Bödeker (Bielefeld University)

11:45
Background magnetic fields and the QCD phase diagram 45m
Strongly interacting quarks and gluons exposed to a background magnetic field reveal a rich physical structure. This topic has recently become of interest, both because it challenges our understanding of the underlying theory (QCD) as well as due to a wide range of phenomenological applications, from neutron star physics to heavyion collisions.
A particularly interesting aspect of this theory is the response of the order parameter (the quark condensate) to the magnetic field and the structure of the corresponding phase diagram. In this talk, I summarize our current knowledge about the mechanisms that are relevant for this response within a variety of settings: effective theories, lowenergy models of QCD and lattice QCD simulations.
Speaker: Gergely Endrődi (University of Frankfurt)

11:00

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Lunch 1h Aula
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Parallel Track 1 Ø110
Ø110
University of Stavanger
Arne Rettedal buildingConvener: Peter Arnold (University of Virginia)
13:30
Rapid thermal coannihilation through bound states 30m
The coannihilation rate of kinetically equilibrated nonrelativistic
particles plays an essential role in the classic WIMP dark matter
scenario. If the dark matter particles interact attractively, for
instance through Z0 exchange, the coannihilation rate could be
substantially increased with respect to a treelevel estimate, a
phenomenon known as the Sommerfeld effect. We study this physics in an
analogous QCD situation, replacing WIMPs by charm or bottom quarks at
a temperature of a few hundred MeV. Through resummed perturbative
estimates and lattice simulations, we demonstrate that the
coannihilation rate can increase much more than predicted by the
standard Sommerfeld enhancement, by up to two orders of magnitude.
The boost originates from the formation of (thermally broadened)
bound states, which subsequently decay.Speaker: Mikko Laine (U. Bern) 
14:00
Standard Model thermodynamics across the electroweak crossover 30m
Within the Standard Model there is no electroweak phase transition which could
account for the nonequilibrium physics needed for Baryogenesis. Nevertheless, at temperatures around 160 GeV some interesting features in the equation of state and other thermodynamical functions, e.g. the heat capacity, can be observed. These features of the Standard Model background could have an impact on nonequilibrium BSM physics, e.g. leptogenesis scenarios or dark matter particle production, taking place at this crossover temperature. In a perturbative threeloop computation and by using already existing lattice simulation data in a dimensionally reduced effective field theory we estimate the relevant thermodynamical functions across the crossover.Speaker: Manuel Meyer (Universität Bern) 
14:30
Thermal Gravitino Production due to Bremsstrahlung and Annihilation Processes 30m
In a theory in which (local) supersymmetry is spontaneously broken for temperatures T \ll M_{pl}, where M_{pl} is the Planck mass, gravitinos couple to MSSM particles via the supercurrent. Thermal gravitino production rate per unit volume due to the strongly interacting sector of the theory can be calculated perturbatively, and to leading order in the QCD coupling \alpha_s(T), is of order \alpha_s(T) (\frac{T}{M_{pl}})^2 T^4. The contribution from 2>2 scatterings of plasma particles with each other has already been calculated. There are, however, additional processes that contribute at the same order which have been overlooked in the literature: bremsstrahlung of gravitinos by quarks, squarks, gluons and gluinos in the thermal bath, and annihilation of these particles to gravitinos. A consistent treatment of these N+1 \rightarrow N+2 processes requires that LandauPomeranchukMigdal effect be incorporated in the calculation.
Speaker: Prof. Çağlar Doğan (Istanbul University) 
15:00
Confinement and Chiral Symmetry Breaking from an ensemble of interacting Instantondyons(monopoles) in SU(2) QCD 30m
We show how the increase in the Instantondyon density can explain both Confinement and Chiral symmetry breaking. We simulate an ensemble of 64 interacting Instantondyons for 2 colors and 0 or 2 quark flavors. We find that at low temperatures, the high density of dyons prefer a symmetric density, which leads to the confining value of the Polyakov Loop. At the same time the Chiral condensate is highly sensitive to the Polyakov Loop. As the Polyakov Loop gets close to the confining value, the Chiral condensate develops a nonzero expectation value, thus breaking Chiral symmetry.
Speaker: Rasmus Larsen (Stony Brook University)

13:30

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Parallel Track 2 Ø120
Ø120
University of Stavanger
Arne Rettedal buildingConvener: Edmond Iancu (CEA/IRFU,Centre d'etude de Saclay GifsurYvette (FR))
13:30
Standard Model vacuum decay and nonminimal coupling. 30m
I will discuss the effect of including a nonminimal coupling between the Higgs field and gravity on vacuum decay in the Standard Model. High precision numerical results indicate that this suppresses vacuum decay relative to flat space calculations, with the minimal suppression near the conformal value of the coupling, $\xi = 1/6$, due to the nearconformal symmetry of the large field 3loop effective potential. The effect with backreaction alone, and no nonminimal coupling ($\xi = 0$), produces an almost negligible shift in the stability bounds for the Standard Model.
Speaker: Stephen Stopyra (Imperial College London) 
14:00
Non Perturbative Renormalization Group for scalar fields in de Sitter space 30m
We address the issue of light scalar fields in de Sitter space using the non perturbative renormalization group. The derivative expansion used in flat space is adapted to this context. At lowest order, the Local Potential Approximation reproduces results of the stochastic approach. We discuss mass and coupling generation as well as radiative symmetry restoration. A simplified first order expansion shows that the flow is slowed down but yields the same IR physics, suggesting that a higher order computation is necessary to capture corrections to the stochastic approach.
Speaker: Maxime Guilleux (Université Paris Diderot) 
14:30
Selfconsistent solitons for tunneling transitions 30m
In many models of electroweak symmetry breaking, the vacuum
structure depends crucially on radiative effects. In order to compute
the decay rate of metastable states, the loop corrections must therefore
be accounted for in the tunneling solitons. In turn, the loops depend on
the solitonic background, such that selfconsistent solutions must be
found. We will discuss the relevance of this problem for the finding
lifetime of the Standard Model vacuum as well as the development of
methods of resolving this problem. (based on 1509.08480, 1509.07847,
1501.07466)Speaker: Prof. Björn Garbrecht (TU München) 
15:00
High temperature nonAbelian chiral instabilities in a lattice effective field theory 30m
The question of whether anomalous, i.e. CPodd effects, in QCD have been observed in relativistic heavyion collisions is a topic of current theoretical and experimental interest. Its solution requires a deeper understanding of how CPodd domains with chiral imbalance n5, if formed in the collision center, evolve in realtime.
Here we present recent results [1] on a new class of plasma instabilities so called chiral instabilities that may play a key role in the presence of finite n5. We investigate their existence and dynamics in nonAbelian SU(2) gauge theory implemented via a Langevinlike anomalous effective field theory [2] on the lattice. n5 enters as a dynamical degree of freedom, driven by changes in topology.
We find that fluctuations in the gauge fields indeed initiate a rapid energy transfer into the magnetic degrees of freedom, while depleting the chiral imbalance. At the same time the topological charge, as helicity is conserved, shows a clear drift among vacuum sectors proportional to the initial n5, as well as a significantly enhanced diffusion constant, i.e. sphaleron rate.
[1] Y.Akamatsu, A.R., N.Yamamoto, JHEP 1603 (2016) 210
[2] Y.Akamatsu, N.Yamamoto, Phys.Rev. D90 (2014) 125031Speaker: Dr. Alexander Rothkopf (Institute for Theoretical Physics, Heidelberg University)

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Parallel Track 3 Ø130
Ø130
University of Stavanger
Arne Rettedal buildingConvener: Gert Aarts (Swansea University)
13:30
Study of the chiral phase transition with vector and axialvector mesons in an extended linear sigma model within the functional renormalization group approach 30m
We use the functional renormalization group (FRG) technique to explore the characteristics of the chiral phase transition between the hadronic phase of quantum chromodynamics and the quarkgluon plasma. The restoration of chiral symmetry at high temperatures and/or netbaryon densities leads to changes in the inmedium spectral properties of light vector mesons, directly affecting the dilepton spectrum measurable in heavyion collisions. Therefore a study of vector and axialvector mesons is indispensable for understanding the underlying mechanism of chiral symmetry restoration.
The theoretical framework for our investigation is the socalled extended linear sigma
model (eLSM). This model is an effective description of the strong interaction which
features besides scalars and pseudoscalars also vector and axialvector mesons. Here,
all degrees of freedom in the eLSM are exclusively treated beyond meanfield, i.e. they
are involved in the FRG flow and, consequently, are subject to quantum and statistical
fluctuations.Recent results on the order of the chiral phase transition and on the mass degeneracy
of chiral partners occurring beyond the phase boundary are presented. The chiral limit as well as the effect of the axial anomaly are examined. Finally, the inclusion of quark fields will be discussed. This study may serve as the starting point for computing the vector meson spectral functions in the near future.Speaker: Jürgen Eser (GoetheUniversity Frankfurt) 
14:00
Chiral symmetry restoration from the hadronic regime 30m
We will present recent results regarding chiral symmetry restoration and other hadronic properties at finite temperature. In particular, we will discuss the interpretation of the temperature dependence of lattice screening masses through Ward identities relating pseudoscalar susceptibilities and quark condensates. Such identities are derived for two and three flavours and studied within the $SU(2)$, $SU(3)$ and $U(3)$ frameworks of Chiral Perturbation Theory, including axial anomaly and $\eta'$ corrections. We will also examine chiral degeneration patterns and the role of the $f_0(500)$ or $\sigma$ state in the saturation of the scalar susceptibility, where our results are consistent with lattice data. The $f_0(500)$ thermal state is generated dynamically from pion scattering and thermal unitarity, both within unitarized ChPT and in other schemes such as that with large number of Goldstone Bosons. Aspects regarding external magnetic fields could also be discussed. Recent references: JHEP 1603 (2016) 186, Phys.Rev. D93 (2016) no.3, 036001.
Speaker: Angel Gomez Nicola (Universidad Complutense Madrid) 
14:30
Complex Langevin Dynamics for a Random Matrix Model of QCD at finite density 30m
We study a Random Matrix Model for QCD at finite density via Complex Langevin dynamics. This model has a phase transition to a phase with nonzero baryon density. We study the convergence of the algorithm as a function of the quark mass and the chemical potential and focus on two main observables: the baryon density and the chiral condensate. As expected, for simulations close to the chiral limit, the algorithm has wrong convergence properties when the quark mass is in the spectral domain of the quenched Dirac operator. Possible solutions of this problem are discussed.
Speaker: Dr. Savvas Zafeiropoulos (Goethe University of Frankfurt) 
15:00
Symmetry breaking restoration by acceleration 30m
In this work we consider the ontological status of the Unruh effect. Is it just a formal mathematical result? Or the temperature detected by an accelerating observer can lead to real physical effects such as phase transitions? In order to clarify this issue we use the Thermalization Theorem to explore the possibility of having a restoration of the symmetry in a system with spontaneous symmetry breaking of an internal continuous symmetry as seen by an accelerating observer. We conclude that the Unruh effect is real physical effect rather than a formal result, giving rise, in the particular example considered here, to a phase transition (symmetry restoration) in the region close to the accelerating observer horizon. We apply our results also to the region close to BH horizons.
Speaker: ANTONIO DOBADO GONZALEZ

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Coffee 30m Aula
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Parallel Track 1 Ø110
Ø110
University of Stavanger
Arne Rettedal buildingConvener: jose Miguel No
16:00
Gravitational waves as a probe of the electroweak phase transition 30m
A firstorder phase transition produces gravitational waves and such a transition only occurs if there is physics beyond the standard model. In this sense gravitational wave experiments can be considered as detectors of new physics. In this talk we review the status of the eLISA experiment and we analyze its capabilities for probing a firstorder phase transition. We demonstrate that in some cases eLISA is able to discover new physics arising at the electroweak scale or even much above. Moreover, by considering some illustrative beyondthestandardmodel scenarios with a firstorder electroweak phase transition, we highlight the existence of parameter regions that are hard to probe at the LHC but are testable at eLISA.
Speaker: Germano Nardini (DESY) 
16:30
Gravitational waves from the phase transition of a nonlinearly realised electroweak symmetry 30m
The 125 GeV Higgs may be a singlet under a nonlinearly realised electroweak symmetry. Differing from the SM, anomalous Higgs cubic couplings are then permitted in the potential, which may lead to a first order electroweak phase transition. We find a range of cubic coupling that may lead to observable gravitational waves signatures at interferometer such as eLISA.
Speaker: Jason Tsz Shing Yue (University of Sydney) 
17:00
Analytic gravitational wave spectrum from bubble collisions 30m
We consider gravitational wave production by bubble collisions during a cosmological firstorder phase transition. Based on socalled thinwall and envelope approximations, we estimate gravitational wave spectrum by an analytic way. Our estimation is based on the observation that the twopoint correlator of the energymomentum tensor can be expressed analytically under these assumptions.
Speaker: Masahiro Takimoto (KEK) 
17:30
Simulating a firstorder electroweak phase transition 30m
In various extensions of the Standard Model it is possible that the electroweak phase transition was first order. This would have been a violent process, involving the formation of bubbles and associated shock waves. The collision of these bubbles and shock waves could be a detectable source of gravitational waves. I will summarise the current status of efforts to model the such a phase transition based on largescale hydrodynamical simulations. From the nucleation of bubbles through to the onset of turbulence, I will discuss the processes involved, the dependence upon particular models, and the implications for detectability of the resulting gravitational wave power spectrum.
Speaker: David Weir (University of Stavanger)

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Parallel Track 2 Ø120
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University of Stavanger
Arne Rettedal buildingConvener: Raju Venugopalan (Brookhaven National Laboratory)
16:00
Realtime dynamics of the Chiral Magnetic Effect 30m
We present a firstprinciples study of the dynamics of the
Chiral Magnetic Effect based on realtime lattice gauge theory
simulations with dynamical fermions. We demonstrate how topological
densities and transitions during the early stages of highenergy
collision lead to the production of axial charge imbalances via the
the axial anomaly and investigate in detail the interplay between
axial and vector currents in the presence of strong magnetic fields.
We also discuss how such simulations can be utilized to provide
initial conditions for the evolution in anomalous hydrodynamics, to
improve the understanding of experimental signatures of the effects in
highenergy heavyion collisions.Speaker: Niklas Mueller (Heidelberg University) 
16:30
Farfromequilibrium universality classes: From heavyion collisions to superfluid scalar systems 30m
Quantum manybody systems far from equilibrium can approach a nonthermal fixed point during their realtime evolution. One example is scalar field theory, which occurs in models of cosmological inflation, and similar examples are found for ultracold Bose gases and for nonAbelian plasmas relevant for heavyion collisions. We present two novel farfromequilibrium universality classes that provide links between these field theories.
One of them involves nonrelativistic, relativistic and expanding scalar systems. It occurs in the deep infrared regime of very high occupancies and leads to the formation of a BoseEinstein condensate. The other novel universality class encompasses scalar field theories and nonAbelian plasmas in a longitudinally expanding background and corresponds to an early dynamical stage of heavyion collisions in the highenergy limit.
The observed universality connects different physics disciplines from heavyion collisions to ultracold atoms, making a remarkable link between the world's hottest and coldest matter.Speaker: Kirill Boguslavski (University of Heidelberg) 
17:00
Simulating thick pancake collisions 30m
A common simplification for describing the early stages of heavy ion collisions is the assumption that incoming nuclei are Lorentzcontracted to infinitely thin "pancakes". This leads to boostinvariance of the produced glasmastate and reduces the system to effectively 2+1 dimensions. This assumption is less justified at lower collision energies. In a recent work [1] we showed how to allow for a finite pancake thickness in the simulation of the production of a glasma state within the McLerranVenugopalan model. This is achieved by using the colored particleincell (CPIC) method in the laboratory frame. We verify that this method agrees with boostinvariant approaches for thin nuclei and find deviations in observables like the pressure anisotropy for thicker nuclei.
[1] D. Gelfand, AI, D. Müller, arXiv:1605.07184
Speaker: Andreas Ipp (TU Wien) 
17:30
Early quark production and approach to chemical equilibrium 30m
We present results from realtime lattice simulations of outofequilibrium quark production in nonAbelian gauge theory in 3+1dimensions. Our simulations include the backreaction of quarks onto the dynamical gluon sector, which is particularly relevant for strongly correlated quarks. We observe fast isotropization and universal behavior of quarks and gluons at weak coupling and establish a quantitative connection to previous pure glue results. In order to understand the strongly correlated regime, we perform simulations for a large number of flavors and compare them to those obtained with two light quark flavors. By doing this we are able to provide estimates of the chemical equilibration time. The presentation is based on our recent publication in Phys. Rev. D93 no. 8, (2016) 085001, arXiv:1601.03576.
Speaker: Dr. Daniil Gelfand (Vienna University of Technology)

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Parallel Track 3 Ø130
Ø130
University of Stavanger
Arne Rettedal buildingConvener: Andreas Schmitt (University of Southampton)
16:00
Chiral magnetic effect and chiral kinetic theory 30m
A power expansion scheme is set up to determine the Wigner function that satisfies the quantum kinetic equation for spin1/2 charged fermions in a background electromagnetic field. Vector and axialvector current induced by magnetic field and vorticity are obtained simultaneously from the Wigner function. The chiral magnetic and vortical effect and chiral anomaly are shown as natural consequences of the quantum kinetic equation. The axialvector current induced by vorticity is argued to lead to a local polarization effect along the vorticity direction in heavyion collisions.
Speaker: Dr. Shi Pu (Institute for Theoretical Physics, Goethe University, Frankfurt am Main) 
16:30
Chiral magnetic effect by synthetic gauge fields 30m
The chiral magnetic effect has attracted much interest in various areas of physics from condensed matter physics to nuclear and particle physics.
In condensed matter physics it has actively investigated in the so called Weyl (semi)metals in which Weyl fermions are realized as points of band touching with definite topological character.
The chiral magnetic effect arises only in nonequilibrium.
It needs finite chiral chemical potential, which equals the mismatch of the Fermi surfaces of right and lefthanded Weyl fermions.
The mismatch (chiral chemical potential) does not appear in equilibrium and is only dynamically generated.
However the dynamics of the chiral chemical potential has not been fully understood yet, which is important to understand the physics of anomaly induced transports in the chiral systems.We study the dynamical generation of the chiral chemical potential in a Weyl metal in a threedimensional optical lattice system, which will be realized by using ultracold atom gases.
Even though atoms are neutral and do not interact with electromagnetic fields, we can simulate the chiral magnetic effect by using ultracold atoms thanks to the so called synthetic gauge fields.
By numerically solving the Boltzmann equation with the Berry curvature in the presence of parallel synthetic electric and magnetic fields,
we analyze the time evolution of the chiral chemical potential and the chiral magnetic current.Speaker: Dr. Tomoya Hayata (Chuo University) 
17:00
Quark matter and neutron stars 30m
We will describe recent progress in perturbative and holographic calculations of the bulk thermodynamic properties of dense quark matter, both at zero and finite temperatures. Particular attention will be placed on the Equation of State and the question, how information about the behavior of this quantity at high densities can be combined with lowdensity results to constrain the observable properties of neutron stars.
Speaker: Aleksi Vuorinen 
17:30
Superfluid vortices in dense quark matter 30m
Superfluid vortices in the colorflavorlocked (CFL) phase of dense quark
matter are known to be energetically disfavored relative to wellseparated
triplets of socalled semisuperfluid color flux tubes. In this talk we will
present results from our numerical stability analysis of superfluid vortices
in dense quark matter. After identifying (physical) regions of
metastability/instability in the parameter space of the couplings of our
effective theory, we will discuss the structure of the unstable mode
responsible for the decay in the case of vanishing gauge coupling. If a
neutron star features a superfluid quark matter core, our analysis indicates
that it is very likely that it would contain semisuperfluid vortices rather
than superfluid vortices. We will point out possible implications of our
results to neutron stars.Speaker: Andreas Windisch (Washington University in St Louis)

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Plenary G001
G001
University of Stavanger
Arne Rettedal buildingConvener: Guy Moore
09:00
Vacuum (meta?)stability, Higgs inflation and physics beyond the Standard Model 45m
The measurements of the Higgs mass and top quark Yukawa coupling indicate that we live in a very special Universe, at the edge of the absolute stability of the electroweak vacuum. The most precise theoretical computations combined with the most recent LHC experiments do not allow us to decide with certainty whether our vacuum is absolutely stable or metastable. In any event, the Standard Model (SM) can be extended all the way up to the Planck scale $M_P$ in a selfconsistent manner. Still, the SM cannot be a complete theory below $M_P$ as it cannot explain the flatness and homogeneity of the Universe at large scales, existence of structures such as clusters or galaxies, its matterantimatter asymmetry, the presence of dark matter and neutrino masses. The first set of problems can be solved within the SM if the Higgs field has a nonminimal coupling to gravity. I will discuss the Higgs inflation for both stable and metastable vacuum and show that it can take place even if the scalar Higgs selfcoupling crosses zero at the energy scale much below the inflationary one. The second set of problems can be solved by extending the SM by three relatively light righthanded neutrinos. I will overview shortly the predictions of the model and discuss accelerator and astrophysical experiments which can be capable to test it.
Speaker: Mikhail Shaposhnikov (EPFL) 
09:45
Dense nuclear and quark matter in compact stars 45m
I will review how compact stars can serve as a laboratory for
fundamental physics, and how the latest astrophysical data can be used to put constraints on the properties of dense QCD matter, for example on its equation of state and on hydrodynamical properties of nuclear and quark superfluids. In the second, more specific, part of the talk, I will present latest results on employing holographic methods to obtain a strongcoupling equation of state for both nuclear and quark matter
within a single model.Speaker: Andreas Schmitt (University of Southampton)

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Coffee 30m Aula
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Plenary G001
G001
University of Stavanger
Arne Rettedal buildingConvener: Guy Moore
11:00
Hydrodynamization in weaklycoupled heavyion collisions 45m
I will discuss how hydrodynamical flow is reached in heavyion collisions
in the limit of weak coupling using an effective kinetic theory description
during the prethermal evolution. I present a Green function that can be
used to provide an initial condition for a hydrodynamical simulation given
the initial geometry.Speaker: Eero Aleksi Kurkela (CERN) 
11:45
Lessons from Numerical Holography 45m
Gauge/gravity duality (or "holography") allows one to calculate
highly nontrivial far from equilibrium dynamics in strongly coupled
gauge theory  provided one can solve asymptotically antide
Sitter initial value problems in higher dimensional gravity. Recent
results and work in progress in this area will be discussed,
focusing on calculations motivated by the physics of heavy ion
collisions and thermal gauge theories.Speaker: Laurence Yaffe (University of Washington)

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Lunch 1h Aula
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