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Andrew White (University of Texas at Arlington (US))22/10/2018, 09:30
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22/10/2018, 09:35
Dr. Duane Dimos (UTA VP Research)
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Dr. Morteza Khaledi (Dean, College of Science)
Dr. Alex Weiss (Chair, UTA Physics) -
Satoru Yamashita (U. Tokyo)22/10/2018, 09:50
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Karsten Buesser (DESY)22/10/2018, 10:20
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Andrew White (University of Texas at Arlington (US))22/10/2018, 10:35
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Lyn Evans (Imperial College Sci., Tech. & Med. (GB))22/10/2018, 11:30
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Shinichiro Michizono (KEK)22/10/2018, 11:50
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Philip Burrows22/10/2018, 12:15
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Junping Tian (University of Tokyo)22/10/2018, 13:45
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Jessie Shelton (Yale U.)22/10/2018, 14:10
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Michael Peskin22/10/2018, 14:35
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Marcel Vos (IFIC (UVEG/CSIC) Valencia)22/10/2018, 15:00
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Jan Strube (PNNL)22/10/2018, 16:00
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Jenny List (Deutsches Elektronen-Synchrotron (DE))22/10/2018, 16:25
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Aidan Robson (University of Glasgow (GB))22/10/2018, 16:50
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Marcel Stanitzki22/10/2018, 17:15
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Daniel Jeans22/10/2018, 17:40
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Haleh Hadavand (UTA)23/10/2018, 08:30
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Mr Hisayasu Nagoshi (Hiroshima University)23/10/2018, 08:30
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Dr Mitsuru Kakizaki (University of Toyama)23/10/2018, 08:30
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Andrea Latina (CERN)23/10/2018, 08:30
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Pierre Korysko (University of Oxford (GB))23/10/2018, 08:45
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Sven Dildick23/10/2018, 08:55
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tsunehiko omori (KEK)23/10/2018, 09:00
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Felix Sefkow (Deutsches Elektronen-Synchrotron (DE))23/10/2018, 09:00
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Pierre Korysko (University of Oxford (GB))23/10/2018, 09:15
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ATLAS, Andrew Bell23/10/2018, 09:20
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Angel Christian Abusleme Hoffman (Pontifical Catholic University of Chile (CL))23/10/2018, 09:30
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Tohru Takahashi23/10/2018, 09:30
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Sean Jiun Wang23/10/2018, 09:45
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Toshiyuki Okugi (KEK)23/10/2018, 09:45
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23/10/2018, 10:00
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Alexei Safonov23/10/2018, 10:00
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Allison Delana23/10/2018, 10:10
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Andrea Latina (CERN)23/10/2018, 10:15
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tsunehiko omori (KEK)23/10/2018, 11:00
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Sami Tantawi (SLAC)23/10/2018, 11:00
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Sven Heinemeyer23/10/2018, 11:00
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Auguste Guillaume Besson (Centre National de la Recherche Scientifique (FR))23/10/2018, 11:00
CMOS Pixel Sensors (CPS) are currently developed for the CBM Micro-Vertex Detector at FAIR/GSI, extrapolating from the ALPIDE
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chip fabricated for the ALICE-ITS. The MIMOSIS sensor for CBM will provide resolutions of 5 mum and 5 mus to comply with the CBM requirements and a 50 times higher data flow capacity compared to ALPIDE. Sensors adapted to the ILC requirements are... -
Samantha Pitman (CERN)23/10/2018, 11:20
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Masafumi Fukuda (KEK: High energy accelerator research organization)23/10/2018, 11:30
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Marcel Vos (Univ. of Valencia and CSIC (ES)), Marcel Vos (IFIC (UVEG/CSIC) Valencia)23/10/2018, 11:30
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Shufang Su (University of Arizona)23/10/2018, 11:35
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Frank Krawczyk23/10/2018, 11:40
Future accelerator facilities such as the proposed MaRIE X‐ray Free Electron Laser (XFEL) and compact accelerators for medical applications and National Security would greatly benefit from ultra‐high gradient (UHG) radio‐frequency (RF) accelerating structures. High gradient structures will reduce the construction and operational cost of large facilities and deliver engineering solutions for...
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23/10/2018, 12:00
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Lee Millar (CERN/U. Lancaster)23/10/2018, 12:00
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Marcel Vos (Univ. of Valencia and CSIC (ES)), Marcel Vos (IFIC (UVEG/CSIC) Valencia)23/10/2018, 12:00
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B.F.L. Ward, Bennie Ward (Baylor University (US))23/10/2018, 12:00
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Joel Sauza (CERN)23/10/2018, 12:20
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Uwe Kraemer (DESY)23/10/2018, 14:00
The DESY II Test Beam Facility is one of few facilities around the world capable of providing multi
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GeV particle beams. It is, as such, a key component in current particle detector development including
development of detectors for the International Linear Collider (ILC) .
As part of the AIDA2020 project, a new large area silicon hodoscope has been designed for installa-
tion at the DESY II... -
Jinchi Cai (CERN)23/10/2018, 14:00
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Keith Ulmer23/10/2018, 14:00
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Adrian Irles (LAL)23/10/2018, 14:00
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Andriy Ushakov (University of Hamburg)23/10/2018, 14:00
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Matt Franzi (SLAC)23/10/2018, 14:20
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Howard Baer (University of Oklahoma)23/10/2018, 14:22
How LHC tells us that there is excellent potential for ILC to discover new particles
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Data from LHC confirm the existence of a very SM-like Higgs boson
at 125 GeV.
However, it is hard to understand the existence of such a particle
state when its mass is unstable under quantum corrections.
Supersymmetry tames the quantum divergences and the h(125) mass falls
squarely within the narrow SUSY... -
Vincent Boudry (LLR)23/10/2018, 14:30
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Sabine Riemann (Deutsches Elektronen-Synchrotron (DE))23/10/2018, 14:30
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Mr Matthew Kilpatrick23/10/2018, 14:30
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Akira Yamamoto (High Energy Accelerator Research Organization (JP))23/10/2018, 14:40
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Sven Heinemeyer23/10/2018, 14:54
-> based on fits in various SUSY frameworks we predict where to find
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SUSY at ILC/CLIC. -
Mr Khaled Alharbi (University of Hamburg)23/10/2018, 15:00
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Emilio Nanni (SLAC National Accelerator Laboratory)23/10/2018, 15:00
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Taikan Suehara (Kyushu University)23/10/2018, 15:00
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Oscar Alonso (University of Barcelona)23/10/2018, 15:00
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Yongcheng Wu23/10/2018, 15:16
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Jeffrey Neilson (SLAC)23/10/2018, 15:20
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Roman Poeschl (Centre National de la Recherche Scientifique (FR))23/10/2018, 15:30
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Mr Manuel Formela (DESY)23/10/2018, 15:30
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Swathi Sasikumar (DESY)23/10/2018, 15:38
In supersymmetric extensions of the Standard Model,higgsino-like charginos and neutralinos are preferred to have masses of the order of the elecktroweak scale by naturalness arguments. Light higgsinos are also well motivated from a top-down perspective. Such light χ ̃±1 ,χ ̃01 and χ ̃02 states can be almost mass degenerate. In this talk the analysis of two benchmark points which exhibits mass...
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James Rosenzweig23/10/2018, 15:40
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Masafumi Fukuda (KEK: High energy accelerator research organization)23/10/2018, 16:30
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Andrei Lunin (Fermilab)23/10/2018, 16:30
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Akiya Miyamoto23/10/2018, 16:30
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Georgios Gerasimos Voutsinas (DESY)23/10/2018, 16:30
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Toshiyuki Okugi (KEK)23/10/2018, 16:30
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Jan Strube (PNNL)23/10/2018, 16:50
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Nikolay Solyak (FNAL)23/10/2018, 16:55
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Joseph Grames (JLab)23/10/2018, 17:00
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Aurelien Martens (Laboratoire de l'Accélérateur Linéaire Université Paris-Sud 11)23/10/2018, 17:00
A global review of the design of the laser-beam systems for the ILC polarimeters is made in view of modern and commercially available systems. This review is done in view of robustness of operations and ease of implementation while preserving or improving the required performances of the laser system at the Compton Interaction Point. The challenges related to precise demonstration of per-mille...
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Takanori Hara (KEK)23/10/2018, 17:10
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Mr Yosuke Kobayashi (Tohoku University)23/10/2018, 17:10
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Kiyoshi Kubo (KEK)23/10/2018, 17:20
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23/10/2018, 17:30
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Glen White (SLAC)23/10/2018, 17:30
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Edu Marin Lacoma (CERN)24/10/2018, 08:30
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Tetsuo Shindou (Kogakuin University)24/10/2018, 08:30
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Hugh Montgomery (Jefferson Lab)24/10/2018, 08:30
This short talk introduces the session and includes the complete Agenda for the day.
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Mr Reima Terada (Shinshu University)24/10/2018, 08:30
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Uwe Kraemer (DESY)24/10/2018, 08:30
For the International Large Detector (ILD) at the planned International Linear Collider (ILC) a time projection chamber (TPC) is foreseen as the main tracking detector. To achieve the required point resolution, micro pattern gaseous detectors (MPGD) will be used in the amplification stage. A readout module using a stack of three gas electron multipliers (GEM) for gas amplification...
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Marc Ross24/10/2018, 08:45
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Jim Orgen (CERN)24/10/2018, 08:50
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Yuya Yoshimura24/10/2018, 08:54
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Toshinori Matsui (University of Toyama)24/10/2018, 08:55
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Aiko Shoji, Aiko Shoji (Iwate University)24/10/2018, 09:00
Micro Pattern Gaseous Detectors (MPGD)-based TPC is proposed as centraltracker in the ILD for the ILC experiment. As the advantages of MPGD,ExB effect is small and a few millimeter 2-track separation is possiblecompared with MWPC readout. Electron Multipliers (GEM) or Micro-MEshGAseous Structure (Micro MEGAS) are candidate as MPGD-readout technology.Gas detector such as the MPGD has a issue of...
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Mr Andrii Pastushenko (Université Paris-Saclay (FR))24/10/2018, 09:10
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Olivier Napoly24/10/2018, 09:15
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Felix Sefkow (Deutsches Elektronen-Synchrotron (DE))24/10/2018, 09:18
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LianTao Wang (University of Chicago)24/10/2018, 09:20
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Vera Cilento (Universita del Sannio (IT))24/10/2018, 09:30
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Mr Kees Ligtenberg (Nikhef)24/10/2018, 09:30
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Katja Krueger (DESY)24/10/2018, 09:42
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Jie Gao (IHEP)24/10/2018, 09:45
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Stephen Jacob Sekula (Southern Methodist University (US))24/10/2018, 10:05
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Mr Naoki Tsuji (The University of Tokyo)24/10/2018, 10:06
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Masanori Matsuoka24/10/2018, 11:00
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Yuichi Okugawa24/10/2018, 11:00
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Sven Heinemeyer24/10/2018, 11:00
-> full one loop calculations of EW SUSY production
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incl. parameter dependence analysis -
Paul Conrad Vaagen Thrane (Norwegian University of Science and Technology (NO))24/10/2018, 11:00
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Adrian Irles (LAL)24/10/2018, 11:20
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Masakazu Yoshioka (KEK)24/10/2018, 11:20
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Vera Cilento (Universita del Sannio (IT))24/10/2018, 11:20
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Xing Wang (Department of Physics and Astronomy, University of Pittsburgh)24/10/2018, 11:22
Once any new particle indicating new physics beyond the SM is discovered at colliders, one of the first crucial steps is to experimentally determine its spin as well as its mass. The future $e^+e^-$ colliders provide perfect tools for studying such properties as long as kinematically accessible, because of the well-constrained event topology and the very clean experimental environment. In this...
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Dr Douglas Bett (University of Oxford)24/10/2018, 11:40
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Masakazu Kurata (KEK)24/10/2018, 11:40
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Camille Ginsburg24/10/2018, 11:40
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Zhuoni Qian (University of Pittsburgh)24/10/2018, 11:44
By assuming a dynamical source of CP violation, the tension between sufficient CP violation for successful electroweak baryogenesis and strong constraints from current electric dipole moment measurements could be alleviated. We study how to explore such scenarios through gravitational wave detection, collider experiments, and their possible synergies with a well-studied example.
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Andre Sailer (CERN), Esteban Fullana Torregrosa (Univ. of Valencia and CSIC (ES))24/10/2018, 12:00
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Renjun YANG (LAL)24/10/2018, 12:00
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Roberto Franceschini (Universita e INFN Roma Tre (IT))24/10/2018, 12:06
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Qinyan Pan24/10/2018, 13:10
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Mattieu Cavellier24/10/2018, 13:40
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Yasuhiro Fuwa (Kyoto University)24/10/2018, 14:00
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Javier Caceres24/10/2018, 14:00
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Andy White, Marcel Stanitzki24/10/2018, 14:00
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Uwe Kraemer (DESY)24/10/2018, 14:15
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Hiroyuki Adachi24/10/2018, 14:20
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yoshihisa iwashita (Kyoto Univ.)24/10/2018, 14:20
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Martin Breidenbach (SLAC)24/10/2018, 14:35
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Kazuyuki Meguro24/10/2018, 14:40
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James Koga (QST)24/10/2018, 14:40
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Gerald Eigen (University of Bergen (NO)), Gerald Eigen (University of Bergen)24/10/2018, 14:55
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Masakazu Yoshioka (KEK)24/10/2018, 15:00
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Steve Greuel24/10/2018, 15:00
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Jan Strube (PNNL)24/10/2018, 15:10
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24/10/2018, 15:25
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Paul Gearing24/10/2018, 15:50
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Mr Yu Morikawa (KEK)24/10/2018, 16:00
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Joel Meissner24/10/2018, 16:10
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Yu Morikawa (KEK)24/10/2018, 16:20
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Joachim Mnich (Deutsches Elektronen Synchrotron (DESY))24/10/2018, 16:30
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Hitoshi Hayano24/10/2018, 16:40
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Takeshi Dohmae25/10/2018, 08:30
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Kiyoshi Kubo (KEK)25/10/2018, 08:30
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73. Radiative corrections to triple Higgs coupling and electroweak phase transition: 2-loop analysisEibun Senaha (KIAS)25/10/2018, 08:30
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Vitaly Yakimenko (BNL)25/10/2018, 08:30
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Hiroshi Sakai (KEK)25/10/2018, 08:50
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Chetan Gohil (University of Oxford (GB))25/10/2018, 08:55
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Kodai Sakurai (University of Toyama)25/10/2018, 08:55
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Dr Victor Smaluk (Brookhaven National Laboratory)25/10/2018, 09:00
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Kazu Terao (SLAC)25/10/2018, 09:00
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Vijay Chouhan (Marui Galvanizing Co., Ltd Japan)25/10/2018, 09:10
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Dr Masakazu Kurata (KEK)25/10/2018, 09:20
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Dr Neven Blaskovic Kraljevic (CERN)25/10/2018, 09:20
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Yuto Deguchi25/10/2018, 09:20
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Yannis Papaphilippou (CERN)25/10/2018, 09:30
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Hitoshi Hayano25/10/2018, 09:30
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Mr Keita Yumino (SOKENDAI)25/10/2018, 09:40
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Takayuki Ueno (Tohoku University)25/10/2018, 09:45
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Andrei Lunin (Fermilab)25/10/2018, 09:45
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Anna Grassellino Grassellino (Fermilab)25/10/2018, 09:50
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Ewen H. Maclean (CERN)25/10/2018, 10:00
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Yuto Uesugi (Kyushu university)25/10/2018, 10:00
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Shin-ichi Kawada (DESY)25/10/2018, 10:10
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Kensei Umemori (KEK)25/10/2018, 10:10
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Victor Smaluk (Brookhaven National Laboratory)25/10/2018, 11:00
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Toshihiro MATSUMOTO25/10/2018, 11:00
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ari palczewski (Jefferson National Laboratory)25/10/2018, 11:00
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Remi Ete (DESY)25/10/2018, 11:00
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Michael Robert Trott25/10/2018, 11:00
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Frank Simon25/10/2018, 11:20
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Matthew James Stuart (CERN)25/10/2018, 11:20
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Marc Wenskat (DESY)25/10/2018, 11:20
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Yipeng Sun (ANL)25/10/2018, 11:30
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Yumi Aoki (SOKENDAI,KEK)25/10/2018, 11:35
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Zuhawn Sung (Fermilab)25/10/2018, 11:40
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Reima Terada (Shinshu University)25/10/2018, 11:40
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Jim Brau (University of Oregon (US))25/10/2018, 12:00
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Silvia Zorzetti (zorzetti@fnal.gov)25/10/2018, 12:00
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Junping Tian (University of Tokyo), Kazuki Fujii (University of Tokyo)25/10/2018, 12:00
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Dr Mathieu Omet (Deutsches Elektronen-Synchrotron)25/10/2018, 12:00
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25/10/2018, 12:20
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Mila Pandurovic (University of Belgrade (RS))25/10/2018, 12:25
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Da Liu, Da Liu (Argonne National Laboratory)25/10/2018, 13:55
In this talk, I will discuss about my recent work on universal relations for the Higgs couplings in composite Higgs models and their phenomenological application for the future lepton colliders. These relations are among one Higgs couplings with two electroweak gauge bosons (HVV), two Higgses couplings with two electroweak gauge bosons (HHVV), one Higgs couplings with three electroweak guage...
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Liang Li (Shanghai Jiao Tong University)25/10/2018, 14:00
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Rongli Geng (Jefferson Lab)25/10/2018, 14:00
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Rohin Thampilali Narayan (University of Texas at Austin (US))25/10/2018, 14:00
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Zhewei Yin (Northwestern University)25/10/2018, 14:19
Recently a method of constructing the non-linear sigma model using only the infrared information is developed. The infrared construction utilizes the unbroken symmetry and the Adler’s zero condition as the only input, resulting in a universal Lagrangian for different symmetry breaking patterns. This implies that the interaction of Higgs bosons in composite Higgs models is universal, where the...
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Bianca Giaccone (Fermilab)25/10/2018, 14:20
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Frank Simon25/10/2018, 14:25
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Adrian Thomson25/10/2018, 14:30
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25/10/2018, 14:40
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Daniel Jeans25/10/2018, 14:43
We present a measurement of the CP state of tau lepton pairs produced in Higgs decay using their spin correlations. A precision of 75mrad on the system's CP phase can be obtained using the 2/ab integrated luminosity envisaged for the ILC250 program.
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Jürgen Reuter (DESY Hamburg, Germany)25/10/2018, 14:45
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Sam Posen (Fermilab)25/10/2018, 15:00
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Todd Adams (Florida State University (US))25/10/2018, 15:00
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yan wang (desy)25/10/2018, 15:07
In many models with extended Higgs sectors, e.g. Two Higgs Doublet Model, Next-to-Minimal Supersymmetric Standard Model and Randall Sundrum model, there exists an extra scalar $S$, and the coupling of $SZZ$ can be very small, as expected from the likeness of the 125 GeV Higgs boson measured at the LHC to the SM Higgs boson. Searches for additional scalars at LEP and LHC are usually dependent...
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sonny mantry mantry (University of Wisconsin at Madison)25/10/2018, 15:10
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Ryan Porter (Cornell University)25/10/2018, 15:20
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Zhen Liu (University of Maryland)25/10/2018, 15:31
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Marcel Vos (IFIC (UVEG/CSIC) Valencia), Martín Perelló Roselló (Instituto de Física Corpuscular (IFIC) - Valencia)25/10/2018, 15:35
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25/10/2018, 15:40
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Nobuhiro Terunuma (KEK)25/10/2018, 16:30
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Yongchao Zhang25/10/2018, 16:30
Lepton flavour violation in seesaew models at future lepton colliders ||| The type-II seesaw and its left-right extensions are well-motivated frameworks to understand the tiny neutrino masses. Both the neutral and doubly-charged scalars from these models could couple to the charged leptons in a flavor-changing way, which is intimately related to the neutrino mass generation. A large parameter...
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Andrew Burrill25/10/2018, 16:35
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Yasuhiro Sugimoto (KEK)25/10/2018, 16:50
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Nobuchika Okada25/10/2018, 16:52
We consider the minimal U(1)$_X$ extension of the Standard Model (SM), where three right-handed neutrinos (RHNs) and one SM singlet $U(1)_X$ Higgs field are introduced. The model is anomaly free in the presence of the three RHNs. Associated with the U(1)$_X$ symmetry breaking by the $U(1)_X$ Higgs VEV, the RHNs acquire Majorana masses, and the seesaw mechanism for generating light SM...
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Yasuchika Yamamoto (KEK)25/10/2018, 16:55
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Matthew James Stuart (CERN)25/10/2018, 17:10
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Cédric Weiland25/10/2018, 17:14
Heavy neutral leptons are part of many extensions of the Standard Model, in particular seesaw models that can explain the light neutrino masses and mixing. Many search strategy have been proposed, either via the direct production of the new heavy neutral leptons or via their indirect effects in processes like lepton flavour violation. We propose here a new search strategy based on WWH...
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Nikolay Solyak (FNAL)25/10/2018, 17:15
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Tomoyuki Sanuki (Tohoku University)25/10/2018, 17:30
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25/10/2018, 17:35
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Marcin Kucharczyk25/10/2018, 17:36
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Taikan Suehara (Kyushu University)26/10/2018, 08:30
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Shintaro Ito (Japanese DIET)26/10/2018, 09:00
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Sam Posen (Fermilab)26/10/2018, 09:20
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Patrick Meade (Stony Brook University)26/10/2018, 09:45
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T. Nakada (EPFL, Lausanne)26/10/2018, 10:40
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Dr Masanori Yamauchi26/10/2018, 10:55
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Juan Fuster Verdu (Univ. of Valencia and CSIC (ES))26/10/2018, 11:15
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Aidan Robson (University of Glasgow (GB))26/10/2018, 11:35
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Dr Chris Fall (US Department of Energy)26/10/2018, 11:55
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Geoffrey Norman Taylor (University of Melbourne (AU))26/10/2018, 12:15
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Steve Greuel
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Victor Smalyuk (BNL)
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Yunlong Zhang
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Jim Brau (University of Oregon (US))
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Kazuyuki Meguro
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Remi Ete (DESY)
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Frank Simon
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Ruben Grewe (TU Darmstadt)
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Steve Greuel
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TBD
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Dr Shin-ichi Kawada (DESY)
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Hitoshi Hayano
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Frank Simon
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Yoshio Fujitani (Tohoku University)
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Reima Terada (Shinshu University)
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Michael Robert Trott
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Ms Yumi Aoki (SOKENDAI,KEK)
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