Jun 4 – 8, 2018
Case Western Reserve University
US/Eastern timezone

Contribution List

141 out of 141 displayed
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  1. Prof. Pavel Fileviez Perez (Case Western Reserve University)
    6/4/18, 4:00 PM
  2. C. Taylor
    6/4/18, 4:05 PM
  3. K. Kash
    6/4/18, 4:15 PM
  4. Glenn David Starkman (Case Western Reserve University (US))
    6/4/18, 4:25 PM
  5. Gerardus 't Hooft (Utrecht University)
    6/4/18, 4:30 PM
  6. Mark Trodden
    6/4/18, 5:00 PM
  7. Marcela Carena (Fermilab)
    6/4/18, 6:00 PM
  8. Marc Kamionkowski
    6/4/18, 6:30 PM
  9. Gregory Gabadadze (N)
    6/5/18, 8:30 AM
  10. Andrew Tolley
    6/5/18, 9:00 AM
  11. Claudia de Rham
    6/5/18, 9:30 AM
  12. Daniel Akerib
    6/5/18, 10:30 AM
  13. Kerstin Perez (MIT)
    6/5/18, 11:00 AM
  14. Rouven Essig
    6/5/18, 11:30 AM
  15. Terrance Figy (Wichita State University)
    6/5/18, 2:00 PM
  16. Mustafa Amin (Rice University)
    6/5/18, 2:00 PM
  17. Eric Chabert (Centre National de la Recherche Scientifique (FR))
    6/5/18, 2:00 PM
  18. Federico Galli (Perimeter Institute)
    6/5/18, 2:00 PM
  19. Tim Linden
    6/5/18, 2:00 PM
  20. Matti Jarvinen (Utrecht University)
    6/5/18, 2:20 PM
  21. Dr Francisco Ponce (Stanford University)
    6/5/18, 2:20 PM
  22. Sonia Paban
    6/5/18, 2:20 PM
  23. Zhenbin Wu (University of Illinois at Chicago (US))
    6/5/18, 2:20 PM
  24. Tobias Neumann (Illinois Tech / Fermi National Accelerator Laboratory)
    6/5/18, 2:20 PM
  25. Hongwan Liu (Massachusetts Institute of Technology)
    6/5/18, 2:40 PM
  26. Javier Tarrío
    6/5/18, 2:40 PM

    I will discuss a mechanism that describes the spontaneous breaking of the gauge (color) group in strongly coupled N=4SYM coupled to charged fundamental matter. The system is holographically described by an intersection of D3 and D7 branes, with a global (baryonic) U(1) charge on the worldvolume of the latter. Backreaction of the D7 branes and the baryonic charge on the geometry is crucial in...

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  27. Claudius Krause (Fermilab)
    6/5/18, 2:40 PM

    We perform a Bayesian statistical analysis of the constraints on the Higgs couplings given by the Higgs electroweak chiral Lagrangian. We obtain bounds on the effective coefficients entering in Higgs observables at the leading order, using all available Higgs-boson signal strengths from the LHC runs 1 and 2 including data reported at Moriond 2018. Using a prior dependence study of the...

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  28. Matthew Johnson, Matthew Johnson (York University/Perimeter Institute)
    6/5/18, 2:40 PM
  29. Adam Davis (Tsinghua University (CN))
    6/5/18, 2:40 PM
  30. Ethan Brown
    6/5/18, 3:00 PM
  31. Márcio O'Dwyer (Case Western Reserve University)
    6/5/18, 3:00 PM
  32. Falko Dulat (SLAC)
    6/5/18, 3:00 PM
  33. Thomas Bachlechner (Columbia University)
    6/5/18, 3:00 PM
  34. Nisar Nellikunnummel (University of Pittsburgh)
    6/5/18, 3:00 PM
  35. Sebastian Ellis
    6/5/18, 3:40 PM

    A light bosonic field mediates a long-range "fifth" force between objects. If the field has self-interactions, experimental constraints on such forces are weakened due to a screening effect. We study how technically natural values for self-interaction terms in the field's potential lead to modification of existing constraints. We show that under this assumption of natural self-interactions,...

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  36. Clara Murgui Galvez
    6/5/18, 3:40 PM
  37. David Miller (University of Chicago (US))
    6/5/18, 3:40 PM
  38. Michael Miloradovic
    6/5/18, 3:40 PM
  39. Mr Oliver Janssen (New York University)
    6/5/18, 3:40 PM
  40. Da Liu
    6/5/18, 4:00 PM
  41. Raymond Co (University of California, Berkeley)
    6/5/18, 4:00 PM
  42. Ian Lewis (The University of Kansas)
    6/5/18, 4:00 PM
  43. Alice Di Tucci (Max Planck Institute)
    6/5/18, 4:00 PM
  44. Paul-Konstantin Oehlmann
    6/5/18, 4:00 PM
  45. Saurabh Kumar
    6/5/18, 4:20 PM
  46. Juan C. Vasquez Carmona
    6/5/18, 4:20 PM
  47. Sebastian Bramberger (Max Planck Institute for Gravitational Physics (Albert Einstein Institute))
    6/5/18, 4:20 PM
  48. Oleksii Matsedonskyi (INFN Padua/Padua University)
    6/5/18, 4:20 PM
  49. Nikhil Raghuram (Massachusetts Institute of Technology)
    6/5/18, 4:20 PM
  50. De-Chang Dai
    6/5/18, 4:40 PM
  51. Jia Liu (University of Chicago)
    6/5/18, 4:40 PM
  52. Daniel Wiegand (University of Pittsburgh)
    6/5/18, 4:40 PM
  53. Cristian Armendariz-Picon
    6/5/18, 4:40 PM
  54. Michal Malinsky (Charles University (CZ))
    6/5/18, 4:40 PM
  55. John Ruhl
    6/5/18, 6:00 PM
  56. Justin Khoury
    6/5/18, 6:30 PM
  57. Alexander Vilenkin
    6/5/18, 7:00 PM
  58. Tao Han (University of Pittsburgh)
    6/6/18, 8:30 AM

    The experiments at the LHC have been improving the measurements of the Higgs boson properties, and searches for new physics are being actively conducted. In the absence of deviations from the Standard Model thus far, it would be prudent to seek for other complementary strategies in the experiments at the energy frontier. For this purpose, we propose to study the Higgs couplings at high energy...

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  59. German Rodrigo (IFIC CSIC-UV)
    6/6/18, 9:00 AM
  60. Corbin Covault
    6/6/18, 9:30 AM
  61. Belen Gavela Legazpi (Universidad Autonoma de Madrid (ES))
    6/6/18, 10:30 AM
  62. Elizabeth Simmons (University of California, San Diego)
    6/6/18, 11:00 AM
  63. Stanley J. Brodsky (SLAC National Accelerator Laboratory, Stanford University)
    6/6/18, 11:30 AM
  64. Ashley Perko (Dartmouth College)
    6/6/18, 2:00 PM
  65. Zhen Liu (Fermilab)
    6/6/18, 2:00 PM
  66. Rebecca Leane (Massachusetts Institute of Technology)
    6/6/18, 2:00 PM
  67. Mr Caner Unal (University of Minnesota)
    6/6/18, 2:00 PM
  68. James Mertens (York University)
    6/6/18, 2:00 PM
  69. Xiaoping Wang (Johannes Gutenberg University Mainz)
    6/6/18, 2:20 PM
  70. Gilly Elor
    6/6/18, 2:20 PM
  71. Igal Jaegle
    6/6/18, 2:20 PM
  72. Ely Kovetz
    6/6/18, 2:20 PM
  73. Mariana Carrillo Gonzalez
    6/6/18, 2:20 PM
  74. Madeline Wade
    6/6/18, 2:40 PM
  75. Rachael Beaton (Princeton University)
    6/6/18, 2:40 PM
  76. Michael Geller (Technion)
    6/6/18, 2:40 PM
  77. Timothy Classen (Lawrence Livermore National Laboratory)
    6/6/18, 2:40 PM
  78. Scott Melville (Imperial College, London)
    6/6/18, 2:40 PM
  79. Sarah Vigeland (University of Wisconsin-Milwaukee)
    6/6/18, 3:00 PM
  80. Jia Liu (Princeton University)
    6/6/18, 3:00 PM
  81. Jeff Dror (Cornell University)
    6/6/18, 3:00 PM
  82. Yoshihisa OBAYASHI (ICRR, Univ. of Tokyo)
    6/6/18, 3:00 PM
  83. Tom Giblin (Kenyon College)
    6/6/18, 3:00 PM
  84. Brandom Eberly
    6/6/18, 3:20 PM

    The MicroBooNE detector is a 170 ton liquid argon time projection chamber (LArTPC) operating in the Booster and NuMI neutrino beams at Fermilab since October 2015. The MicroBooNE physics program includes neutrino oscillation searches that aim to resolve the anomalous excess of low-energy electromagnetic shower events observed by MiniBooNE, as well as neutrino cross-section measurements on...

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  85. Carlos E.M. Wagner (University of Chicago)
    6/7/18, 8:30 AM
  86. Howard Baer (University of Oklahoma)
    6/7/18, 9:00 AM
  87. Neil Cornish
    6/7/18, 9:30 AM
  88. Philip Argyres
    6/7/18, 10:30 AM
  89. John Duncan
    6/7/18, 11:00 AM
  90. Dejan Stojkovic (SUNY at Buffalo)
    6/7/18, 11:30 AM
  91. James Bonifacio
    6/7/18, 2:00 PM
  92. Lilli Sun
    6/7/18, 2:00 PM
  93. Yuhsin Tsai (University of Maryland)
    6/7/18, 2:00 PM
  94. Matthew Hasselfield (Penn State University)
    6/7/18, 2:00 PM
  95. Luke Kippenbrock
    6/7/18, 2:00 PM
  96. Vivek Singh
    6/7/18, 2:20 PM
  97. Marcin Badziak
    6/7/18, 2:20 PM
  98. Rachel Rosen
    6/7/18, 2:20 PM
  99. Mathew Madhavacheril (Princeton)
    6/7/18, 2:20 PM
  100. Joey Shapiro Key (University of Washington Bothell)
    6/7/18, 2:20 PM
  101. Adrian Liu (UC Berkeley)
    6/7/18, 2:40 PM
  102. Dr Jax Sanders (Syracuse University)
    6/7/18, 2:40 PM
  103. Zhengkang Zhang (University of Michigan)
    6/7/18, 2:40 PM
  104. Keisuke Harigaya (UC Berkeley, LBNL)
    6/7/18, 2:40 PM
  105. Austin Joyce
    6/7/18, 2:40 PM
  106. Matthew Low (Institute for Advanced Study)
    6/7/18, 3:00 PM
  107. Dr Yongchao Zhang
    6/7/18, 3:00 PM
  108. Laura Johnson
    6/7/18, 3:00 PM
  109. Andrew Matas
    6/7/18, 3:00 PM
  110. Francisco Villaescusa Navarro
    6/7/18, 3:00 PM

    The 21cm radiation from cosmic neutral hydrogen can be used to survey large cosmological volumes of the Universe through intensity mapping. I will discuss the impact of neutrino masses on the abundance and clustering of neutral hydrogen, that we have investigated through hydrodynamic simulations with massive neutrinos. I will show that it can be understood by accounting for the effects...

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  111. Mark Hertzberg (Tufts University)
    6/7/18, 3:40 PM
  112. Reed Essik
    6/7/18, 3:40 PM
  113. George Zahariade (Laboratoire APC)
    6/7/18, 3:40 PM
  114. Siddharth Mishra-Sharma
    6/7/18, 3:40 PM
  115. Robert Kehoe (Southern Methodist University (US))
    6/7/18, 3:40 PM
  116. Linda Blot (Institute of Space Sciences (CSIC), IEEC)
    6/7/18, 4:00 PM

    Large scale structure simulations are a fundamental tool to interpret data from large volume galaxy surveys. In fact, modelling the observables and their covariance is affected by the non-linear regime of gravitational collapse, a phenomenon that is best captured through simulations. In this talk I will present some applications of simulations that are relevant to present and upcoming galaxy...

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  117. Jessica Turner (Durham University)
    6/7/18, 4:00 PM
  118. Leslie Wade
    6/7/18, 4:00 PM
  119. Hongkai Liu (University of Pittsburgh (US))
    6/7/18, 4:00 PM
  120. Laura Sagunski
    6/7/18, 4:00 PM
  121. Xing Wang (University of Pittsburgh)
    6/7/18, 4:20 PM
  122. Marcos A. Garcia Garcia (Rice University)
    6/7/18, 4:20 PM
  123. Jing Ming
    6/7/18, 4:20 PM
  124. Ashley Ross (Ohio State University)
    6/7/18, 4:20 PM

    I will describe how the baryon acoustic oscillation (BAO) scale observed in the distribution of galaxies can be treated as a standard ruler that enables distance measurements as a function of redshift. These measurement allow precise tests on the nature of Dark Energy. I will describe the current status of BAO measurements and the constraints they afford, focusing on recent measurements from...

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  125. Lasma Alberte
    6/7/18, 4:20 PM
  126. Kuver Sinha
    6/7/18, 4:40 PM
  127. Elena Giusarma
    6/7/18, 4:40 PM
  128. Suntharan Arunasalam (University of Sydney)
    6/7/18, 4:40 PM

    We discuss a cosmological phase transition within the Standard Model which incorporates spontaneously broken scale invariance as a low-energy theory. In addition to the Standard Model fields, the minimal model involves a light dilaton, which acquires a large vacuum expectation value (VEV) through the mechanism of dimensional transmutation. Under the assumption of the cancellation of the vacuum...

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  129. Tom Callister
    6/7/18, 4:40 PM
  130. Jeremy Sakstein (University of Pennsylvania)
    6/7/18, 4:40 PM
  131. Francis Halzen (IceCube/WIPAC)
    6/7/18, 6:00 PM
  132. Tanmay Vachaspati
    6/7/18, 6:30 PM
  133. Ravi Sheth (ICTP/UPenn)
    6/7/18, 7:00 PM
  134. Albert de Roeck
    6/8/18, 9:00 AM
  135. Robert Bernstein
    6/8/18, 9:30 AM
  136. Pran Nath (Department of Physics)
    6/8/18, 10:00 AM
  137. Rabindra Mohapatra (University of Maryland)
    6/8/18, 11:00 AM
  138. Goran Senjanovic
    6/8/18, 11:30 AM
  139. Juan Maldacena (Unknown)
    6/8/18, 12:00 PM
  140. Madeline Wade
  141. Da Liu