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Spyros Argyropoulos (Albert Ludwigs Universitaet Freiburg (DE))13/05/2024, 14:00
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David Curtin (University of Toronto)13/05/2024, 14:20
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Jackson Carl Burzynski (Simon Fraser University (CA))13/05/2024, 14:55
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Joseph Reichert (Rutgers State Univ. of New Jersey (US))13/05/2024, 15:20
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Audrey Katherine Kvam (University of Massachusetts (US))13/05/2024, 15:45
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Christina Wenlu Wang (California Institute of Technology (US))13/05/2024, 16:45
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Prof. Andre Lessa (CCNH - Univ. Federal do ABC), Andre Lessa (IFGW - UNICAMP)13/05/2024, 17:05
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Louis Henry (EPFL - Ecole Polytechnique Federale Lausanne (CH))13/05/2024, 17:30LLP signatures
The High Luminosity LHC will be a tremendous opportunity to search for long lived particles (LLPs) from an extended hidden/dark sector, feebly connected to the known SM sector. Such LLP searches will require special detectors, placed far away from the proton-proton collision point and shielded against SM backgrounds. The CODEX-b detector, to be placed behind a thick shielding wall inside the...
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Dr Louie Dartmoor Corpe (Laboratoire de Physique Clermont Auvergne (LPCA))13/05/2024, 17:50
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Dr Atri Dey (Dublin Institute for Advanced Studies)14/05/2024, 09:00
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Prof. Alexander Belyaev (University of Southampton & Rutherford Appleton Laboratory)14/05/2024, 09:30
We suggest a new class of models - Fermionic Portal Vector Dark Matter (FPVDM) which extends the Standard Model (SM) with SU(2)_D dark gauge sector. While FPVDM does not require kinetic mixing and Higgs portal. It is based on the Vector-Like (VL) fermionic doublet which couples the dark sector with the SM sector through the Yukawa interaction. The FPVDM framework provides a vector Dark Matter...
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Max Fieg (University of California Irvine (US))14/05/2024, 10:00
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Thea Aarrestad (ETH Zurich (CH))14/05/2024, 10:30
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Jnanadeva Maharana (National Institute of Science Education and Research (IN))14/05/2024, 11:30Unexplored signatures & wildcard ideas
t has been proposed that, in the large radius compactification (LRC) scenario, the Kaluza-Klein states might be considered as dark matter (DM) candidates. The universal extra dimension (UED) hypothesis, together with the LRC paradigm, holds the prospect of observing KK states at LHC if masses lie in the accessible LHC energy scale. If observed, they might be possible DM candidates, provided...
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Konstantin Zioutas (University of Patras (GR))14/05/2024, 11:45Unexplored signatures & wildcard ideas
Anti-quark nuggets, AQNs, (ZHITNITSKY, 2003), have been suggested to solve the dark matter (DM) and the missing antimatter problem in the universe, and have been proposed as an explanation of various observations.
Their size is in the μm range and their density equal to the nuclear density with an expected flux of about 1 / km2 / year. For the typical velocity of DM constituents (~250...
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James Pinfold (University of Alberta (CA))14/05/2024, 12:00
The MoEDAL-MAPP experiment at Run-3 incorporates the MoEDAL and MAPP-1 (MoEDAL Apparatus for Penetrating Particles) detectors deployed at IP8 and in the UA83 tunnel on the LHC Ring, respectively. The passive, triggerless, MoEDAL detector has been taking data at Run-1 and Run-2 and is a world leader in the direct search for Highly Ionizing Particles (HIPs) at a Collider. HIP avatars of new...
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Spyros Argyropoulos (Albert Ludwigs Universitaet Freiburg (DE))14/05/2024, 12:15
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Diallo Boye (Brookhaven National Laboratory)14/05/2024, 14:00
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Andrea Malara (Universite Libre de Bruxelles (BE))14/05/2024, 14:30
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Matteo Bauce (Sapienza Universita e INFN, Roma I (IT))14/05/2024, 15:00
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David Yu (University of Nebraska Lincoln (US))14/05/2024, 15:30
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Prof. Pyungwon Ko (KIAS (Korea Institute for Advanced Study))14/05/2024, 16:30
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Prof. Myeonghun Park (Seoultech)14/05/2024, 17:00s-channel & Higgs to invisible
In this talk, I will review the importance of "Gauge invariance" in the search for Dark matter at the High Energy Collider including LHC.
The major topics I will include will be
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1) The limit of effective field theory / simplified model approach at the High Energy collider
2) Dark matter showering at the High Energy collider -
Rhitaja Sengupta (BCTP and Physikalisches Institut der Universität Bonn, Germany)14/05/2024, 17:25s-channel & Higgs to invisible
We explore the parameter space of the phenomenological Minimal Supersymmetric Standard Model (pMSSM) with a light neutralino thermal dark matter (M ̃χ01 ≤ Mh/2) that is consistent with current collider and astrophysical constraints. We identify that a narrow region with light Higgsinos having masses between 125-160 GeV survives the present constraints for the μ < 0 scenario, including the...
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Yang Bai14/05/2024, 17:50s-channel & Higgs to invisible
Dark matter bound states may exist within the dark sector, characterized by a substantial dark force. Depending on the spins and parity properties of the force carriers, Standard Model particles may primarily couple with either the lowest or excited bound states. We discuss the associated collider signatures at the LHC for various simplified models.
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Janna Katharina Behr (Deutsches Elektronen-Synchrotron (DE))15/05/2024, 09:00
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Danyer Perez Adan (RWTH Aachen University (DE))15/05/2024, 09:30
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Jose Miguel No Redondo (Conseil Europeen Recherche Nucl. (CERN)-Unknown-Unknown), Jose Miguel No Redondo15/05/2024, 10:00
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Giorgio Busoni (The University of Melbourne), Giorgio Busoni (The Australian National University)15/05/2024, 10:30
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Dr Manimala Mitra (Institute of Physics (IOP))15/05/2024, 11:30
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Dr Jayita Lahiri (II. Theoretical Institute for Physics, University of Hamburg)15/05/2024, 11:45
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Ilia Kalaitzidou (Albert Ludwigs Universitaet Freiburg (DE))15/05/2024, 12:00Extended Higgs sectors
The 2HDMa model is one of the main models used in the Dark Matter searches at the LHC. So far, all the 2HDMa benchmarks used by the LHC experiments feature a Type-II Yukawa sector with degenerate Higgses ($m_A=m_H=m_{H^{\pm}}$). The latter implies, together with the fact that flavour observables put lower bounds on the mass of the charged Higgses, that the $A/H/H^{\pm}$ bosons are all...
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Spyros Argyropoulos (Albert Ludwigs Universitaet Freiburg (DE))15/05/2024, 12:15
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Adrian Casais Vidal (Massachusetts Institute of Technology (MIT))15/05/2024, 14:00
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Elisa Fontanesi (Boston University (US))15/05/2024, 14:30
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Hassnae El Jarrari (CERN)15/05/2024, 15:00
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Yotam Soreq (Technion- Israel Institute of Technology (IL))15/05/2024, 15:30
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Kai Ma (Shaanxi University of Technology)15/05/2024, 16:30
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Stefania Gori (UC Santa Cruz)15/05/2024, 16:50
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Bertrand Echenard (California Institute of Technology (US))15/05/2024, 17:25
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Chiara Arina (CP3 UCLouvain)16/05/2024, 09:00
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Luca Panizzi (Uppsala University)16/05/2024, 09:30
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Monika Blanke (Karlsruhe Institute of Technology)16/05/2024, 10:10
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Deborah Pinna (University of Wisconsin Madison (US))16/05/2024, 11:15
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Dr Jan Heisig (Université catholique de Louvain (UCL)), Jan Heisig16/05/2024, 11:35
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Dr Adil Jueid (Institute for Basic Science)16/05/2024, 12:05
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Benjamin Fuks16/05/2024, 12:20
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Dr Giorgio Arcadi (University of Messina (Italy))16/05/2024, 14:00
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Mr Changqiao Li (Max Planck Society (DE))16/05/2024, 14:30
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Alicia Calderon Tazon (Universidad de Cantabria and CSIC (ES)), Alicia Calderon tazon16/05/2024, 14:50
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Even Simonsen Haaland (University of Oslo (NO))16/05/2024, 15:10Dark Higgs
We present a review of the models used for the search for a new leptonically decaying neutral vector boson in association with missing transverse energy by ATLAS, which was published as a conference note (ATLAS-CONF-2023-045) in August 2023. Three signal regions were defined as bins in the $\text{E}_\text{T}^{\text{miss}}$ significance, and the search was performed by scanning across the...
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Thomas Biekötter16/05/2024, 16:00
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Pallabi Das (Princeton University (US))16/05/2024, 16:30
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Patrick Ecker16/05/2024, 16:50Dark Higgs
Belle II has a unique reach for a broad class of models that postulate the existence of dark matter particles in the MeV-GeV mass range. One scenario is a model which involves inelastic dark matter, consisting of two dark matter states with a mass splitting between them and the presence of a dark Higgs boson. This model has a signature of up to two displaced vertices, one from the resonant...
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Felix Kahlhoefer (Karlsruhe Institute of Technology)16/05/2024, 17:10
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Annapaola De Cosa (ETH Zurich (CH)), Suchita Kulkarni (University of Graz), Sukanya Sinha (University of Manchester (GB))17/05/2024, 09:00
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Felix Kahlhoefer (Karlsruhe Institute of Technology)17/05/2024, 09:05Dark showers
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Dilia Maria Portillo Quintero (TRIUMF (CA))17/05/2024, 09:35
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Long Wang (University of Maryland (US))17/05/2024, 09:55
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Dr José Francisco Zurita (IFIC - Univ. of Valencia and CSIC (ES))17/05/2024, 10:15Dark showers
In this talk we will present the reinterpretation of the CMS emerging jets (that is, long-lived dark pions belonging to a strongly interacting dark sector), published in JHEP 01 (2024) 034 (arXiv:207.04847) and will show that particularly this search can set meaningful bounds on scenarios where the SM Higgs boson mediates between the visible and dark sectors. In particular we find that for...
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Deepak Kar (University of the Witwatersrand (ZA))17/05/2024, 10:30Dark showers
After the first round of SVJ experimental results, the focus has shifted to exploring more specific topologies, as well as attempts to design more sensitive observables. In this presentation, we will cover an exploratory study of SVJs produced preferentially with bottom quarks, including looking at the sensitivity from current public results. The advantage of using variable radius jets will be...
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Caleb Gemmell (University of Toronto)17/05/2024, 11:15
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Cesare Tiziano Cazzaniga (ETH Zurich (CH))17/05/2024, 11:40Dark showers
The Hidden Valley scenario consists of a set of models where the Standard Model is accompanied by a Hidden Sector and connected with it via a heavy mediator or a weak coupling. If realised in nature, the Hidden Valley scenario may result in unusual and little-studied phenomena at the LHC. Under the assumption of a QCD-like confining dark sector, novel experimental signatures emerge,...
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Joschka Birk (Hamburg University (DE))17/05/2024, 11:55
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William Shepherd17/05/2024, 12:15
I present ongoing work seeking to identify the presence of dark shower phenomena in otherwise ordinary-seeming jets using jet substructure techniques with a particular focus on the recently-proposed SIFT algorithm. The aim is to explicitly identify the mass scale signature of the dark shower products which then promptly decay back into SM quarks, giving effectively normal-looking SM jets. This...
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Annapaola De Cosa (ETH Zurich (CH)), Suchita Kulkarni (University of Graz), Sukanya Sinha (University of Manchester (GB))17/05/2024, 12:30
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James Frost (University of Oxford (GB))17/05/2024, 13:00
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Prof. Manimala Mitra (Institute of Physics (IOP))
Singlet-Triplet Fermionic Model ($\nu$STFM) with an extended fermion and Higgs sector is a well motivated model which explains both neutrino masses and dark matter (DM). Two of the triplet $\rho_{1,2}$ and singlet fermionic fields $N_{1,2}$ contribute to neutrino mass generation via seesaw mechanism, while, the remaining triplet $\rho_3$ and singlet $N_3$ fields are the constituents of the...
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Kai Ma (Shaanxi University of Technology), Prof. Shao-Feng Ge (Tsung-Dao Lee Institute (TDLI) & School of Physics and Astronomy (SPA) & SJTU)Low mass signatures, ALPs, dark photons
Searching for absorbed fermionic dark matter by nuclei is being taken more and more
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attention. In stead of the energy recoil signal at direct detection experiments, dark matter
appears always as missing energy at high energy colliders. For such a fermionic
dark matter, its production is always accompanied by an invisible neutrino.
Mono-X (photon, jet and $Z$ boson) productions are... -
Alvaro Lopez Solis (Deutsches Elektronen-Synchrotron (DE)), Marawan Barakat (Deutsches Elektronen-Synchrotron (DE)), Priscilla Pani (Deutsches Elektronen-Synchrotron (DE))Unexplored signatures & wildcard ideas
The existence of a new type of non-baryonic matter in the Universe, also called Dark Matter (DM), is supported by compelling astrophysical and cosmological evidence. Considerations on its measured relic density favour the hypothesis that Dark Matter is composed primarily of Weakly Interacting Massive Particles (WIMPs). Unfortunately, numerous experiments targeting the detection of these DM...
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Dr Jayita Lahiri (II. Theoretical Institute for Physics, University of Hamburg)Extended Higgs sectors
Recasting is an extremely powerful tool to derive limits on new physics
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models. With so many NP models at our disposal, recasting makes it easy to use the limits derived on certain models by experimental searches, to
constrain any model of our choice. However, this method can fail, if
the model of our interest not only differs from the one it is being
recasted from, in terms of event... -
William Shepherd
I present ongoing work seeking to identify the presence of dark shower phenomena in otherwise ordinary-seeming jets using jet substructure techniques with a particular focus on the recently-proposed SIFT algorithm. The aim is to explicitly identify the mass scale signature of the dark shower products which then promptly decay back into SM quarks, giving effectively normal-looking SM jets. This...
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James Pinfold (University of Alberta (CA))Unexplored signatures & wildcard ideas
The MoEDAL-MAPP experiment at Run-3 incorporates the MoEDAL and MAPP-1 (MoEDAL Apparatus for Penetrating Particles) detectors deployed at IP8 and in the UA83 tunnel on the LHC Ring, respectively. The passive, triggerless, MoEDAL detector has been taking data at Run-1 and Run-2 and is a world leader in the direct search for Highly Ionizing Particles (HIPs) at a Collider. HIP avatars of new...
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