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    PASCOS 2018, Case Western Reserve University, Cleveland, USA

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

    Session

    Parallel 5

    7 Jun 2018, 15:40
    Thwing Center, Thwing Excelsior Ballroom (Case Western Reserve University)

    Thwing Center, Thwing Excelsior Ballroom

    Case Western Reserve University

    Case Western Reserve University, Thwing Center, Thwing Excelsior Ballroom (Second Floor), 11111 Euclid Ave, Cleveland, OH 44106 Parallel Talks take place at the Rockefeller Building, Physics Department, 2076 Adelbert Rd. Cleveland, OH 44106.

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    1. 104. Aspects of Axion Dark Matter Clumps
      Mark Hertzberg (Tufts University)
      07/06/2018, 15:40
    2. 128. Astrophysical implications of GW observations
      Reed Essik
      07/06/2018, 15:40
    3. 112. Classical Hawking radiation
      George Zahariade (Laboratoire APC)
      07/06/2018, 15:40
    4. 136. LHC searches for dark sector showers
      Siddharth Mishra-Sharma
      07/06/2018, 15:40
    5. 120. The Dark Energy Spectroscopic Instrument
      Robert Kehoe (Southern Methodist University (US))
      07/06/2018, 15:40
    6. 121. Cosmological simulations for precision cosmology with large galaxy surveys
      Linda Blot (Institute of Space Sciences (CSIC), IEEC)
      07/06/2018, 16:00

      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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    7. 105. Intermediate Scale Non-resonant Leptogenesis
      Jessica Turner (Durham University)
      07/06/2018, 16:00
    8. 129. Measuring the neutron star equation of state with gravita- tional waves
      Leslie Wade
      07/06/2018, 16:00
    9. 137. One loop corrections to the spin-independent blind spot
      Hongkai Liu (University of Pittsburgh (US))
      07/06/2018, 16:00
    10. 113. Testing Modified Gravity with Merging Neutron Stars
      Laura Sagunski
      07/06/2018, 16:00
    11. 138. Electroweak DM at Future Hadron Collider
      Xing Wang (University of Pittsburgh)
      07/06/2018, 16:20
    12. 106. Enhancement of the dark matter abundance before reheating: thermal and non-thermal production
      Marcos A. Garcia Garcia (Rice University)
      07/06/2018, 16:20
    13. 130. Folding-in astrophysical priors in searches for continuous gravitational waves
      Jing Ming
      07/06/2018, 16:20
    14. 122. The Status of Constraints on Dark Energy from Baryon Acoustic Oscillation Scale Measurements
      Ashley Ross (Ohio State University)
      07/06/2018, 16:20

      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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    15. 114. Transverse phonons in holographic massive gravity
      Lasma Alberte
      07/06/2018, 16:20
    16. 107. Constraining Axion-like-Particles with Hard X-Ray Emission from Magnetars
      Kuver Sinha
      07/06/2018, 16:40
    17. 123. Exploring neutrino masses with Large Scale Structure
      Elena Giusarma
      07/06/2018, 16:40
    18. 139. Low temperature EW phase transition in the SM with hidden scale invariance
      Suntharan Arunasalam (University of Sydney)
      07/06/2018, 16:40

      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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    19. 131. Searching for scalar and tensor polarizations with the stochas- tic gravitational wave background
      Tom Callister
      07/06/2018, 16:40
    20. 115. Superfluids and the cosmological constant problem
      Jeremy Sakstein (University of Pennsylvania)
      07/06/2018, 16:40
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