CERN LHC seminar: Precision Tests of the Electroweak Sector with the ATLAS detector

• Daniel Froidevaux (CERN)

Room: 222/R-001 See https://indico.cern.ch/event/719637/

TH Colloquium: NNLO Precision for the LHC's Next Stage

• Radja Boughezal (Argonne National Laboratory)

Room: 4/3-006 - TH Conference Room

New Ideas for Light Dark Matter

• Yonit Hochberg (Hebrew University)

Room: 4/3-006 - TH Conference Room

TH Colloquium: The generalized double copy and its applications to UV properties of supergravity theories

• Zvi Bern (Univ. of California Los Angeles (US))

Room: 4/3-006 - TH Conference Room

EFT at colliders: What next?

• Fabio Maltoni (Universite Catholique de Louvain (UCL) (BE))

Room: 4/3-006 - TH Conference Room

Supersymmetry at colliders.

• Carlos E.M. Wagner (University of Chicago)

Room: 4/3-006 - TH Conference Room

The Higgs as a Tool for Exploration

• Marcela Carena (Fermilab)

Room: 4/3-006 - TH Conference Room

Exotic Higgs Decays

• Zhen Liu (Fermilab)

Room: 4/3-006 - TH Conference Room

Bound states of Dark Matter

• Michele Redi (Universita e INFN, Firenze (IT))

Room: 4/3-006 - TH Conference Room

Neutral Naturalness

• Ennio Salvioni (Technische Universität Muenchen (DE))

Room: 4/3-006 - TH Conference Room

Axion and Dark Photon Direct Detection

• Masha Baryakhtar (PI - Perimeter Institute for Theoretical Physics (CA))

Room: 4/3-006 - TH Conference Room

Precision Electroweak Physics at the LHC

• Christoph Englert (Heidelberg University)
• Michael Spannowsky (University of Durham (GB))
• Giuliano Panico (The Barcelona Institute of Science and Technology (BIST) (ES))

Room: 4/3-006 - TH Conference Room

BSM/EFT

• Dave Sutherland

Room: 4/3-006 - TH Conference Room

TH Colloquium: Dark Matter in Disequilibrium

• Mariangela Lisanti (Stanford University)

Room: 503/1-001 - Council Chamber The Gaia mission is in the process of mapping nearly 1% of the Milky Way’s stars. This data set is unprecedented and provides a unique view into the formation history of our Galaxy and its associated dark matter halo. I will review results based on the most recent Gaia data release, which demonstrate that the inner Galaxy is dominated by the stellar remnants of a single massive satellite galaxy that merged with the Milky Way early on. These results suggest that the component of dark matter that is sourced from luminous satellites may not be in equilibrium, with a non-trivial fraction in substructure. I will explain the ramifications of these findings for direct detection experiments.

LLPs

• David Curtin (University of Toronto)

Room: 4/3-006 - TH Conference Room

Black Hole Dark Matter

• Oriol Pujolas Boix (Universitat Autònoma de Barcelona (ES))

Room: 4/3-006 - TH Conference Room

Cosmological Probes of Fine Tuning

• JiJi Fan (Brown University)

Room: 4/3-006 - TH Conference Room

Machine Learning and BSM

• Tim Cohen (University of Oregon)
• Andrea Wulzer (CERN)

Room: 4/3-006 - TH Conference Room

Axionic Electroweak Baryogenesis

• Chang Sub Shin (Institute for Basic Science )

Room: 4/3-006 - TH Conference Room

TH Colloquium: Is Nature Natural?

• Nathaniel Craig (UC Santa Barbara)

Room: 503/1-001 - Council Chamber The discovery of the Higgs boson at the Large Hadron Collider marks the culmination of a decades-long quest for the final piece of the Standard Model. But the discovery of the Higgs also adds new urgency to the hierarchy problem, namely the question of why the Higgs boson is so light despite its unique quantum sensitivity to much higher energy scales. This puzzle is made all the more challenging by the lack of evidence thus far for conventional approaches to the hierarchy problem at the LHC and other experiments. I'll discuss the essential features of the hierarchy problem and its possible solutions, with a particular focus on new approaches to the problem that have emerged in the years following the Higgs discovery. These new approaches feature novel experimental signatures, add urgency to the measurement of Higgs properties, and may shed light on dark matter and other mysteries of the Standard Model.

Solving the Hierarchy Problem Discretely - A light Higgs without top partners

• Anson Hook (Maryland)

Room: 4/3-006 - TH Conference Room

Higgs, Relaxion, and Dark Matter

• Nayara Fonseca (DESY)

Room: 4/3-006 - TH Conference Room

TBA

• Gilad Perez (CERN & Weizmann)

Room: 4/3-006 - TH Conference Room

Relaxion phenomenology

• Diego Redigolo (Weizmann Inst. & Tel Aviv University)

Room: 4/3-006 - TH Conference Room