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TACOS Workshop at Rice

America/Chicago
Duncan Hall, Room 1070 (Rice University)

Duncan Hall, Room 1070

Rice University

Rice University Duncan Hall, Room 1070 6100 Main Street Houston, TX 77005
Andrew Long (Rice University), Fred Olness (Southern Methodist University (US)), James Dent, Joel Meyers (Southern Methodist University), Kimberly Boddy (University of Texas at Austin), Louis Strigari (Texas A&M)
Description

Theoretical Astroparticle and Cosmology Symposium in Texas

 

Building research ties across Texas:  This meeting brings together researchers interested in topics at the intersection of theoretical particle physics, astrophysics, and cosmology. Participants from various institutions in Texas present and discuss the latest developments in their subfields, with the aim of fostering ideas and collaborations among faculty, postdocs, and graduate students. The host institution rotates from year to year to enable interactions with local experts in neighboring subfields.

 

Meeting Website:

https://sites.google.com/view/texas-tacos/upcoming-meeting

 

Scientific Organizing Committee:

Kimberly Boddy (UT Austin)
James Dent (Sam Houston)
Andrew Long (Rice)
Joel Meyers (SMU)
Louis Strigari (TAMU)

  • Monday 9 October
    • 08:30 21:10
      Monday Session
      • 08:30
        Breakfast 30m
      • 09:00
        Opening 10m

        Welcome remarks by Chris Johns-Krull, chair of the Physics and Astronomy Department.

        Speaker: Andrew Long (Rice University)
      • 09:10
        New Opportunities and New Challenges with Upcoming CMB Surveys 30m
        Speaker: Joel Meyers (Southern Methodist University)
      • 09:40
        The Dark Energy Spectroscopic Instrument (DESI): HOD-dependent systematics in modelling Baryon Acoustic Oscillations for Emission Line Galaxy 20m
        Speaker: Cristhian Garcia Quintero (UT Dallas)
      • 10:00
        Taquitos I 30m
        Speakers: Andrew Long (Rice University), Dorian Amaral (Rice University), Joel Meyers (Southern Methodist University)
      • 10:30
        Coffee Break 40m
      • 11:10
        Has JWST Discovered Dark Stars? 30m
        Speaker: Katherine Freese
      • 11:40
        The viability of ultralight bosonic dark matter in dwarf galaxies 20m
        Speaker: Isabelle Goldstein (Brown University)
      • 12:00
        Neutron star cooling with lepton-flavor-violating axions 20m
        Speaker: Hong-Yi Zhang
      • 12:20
        Group Photo 10m
      • 12:30
        Lunch 1h 20m
      • 13:50
        GRMHD Positron Applications from the Present and Primordial Universe 30m

        With the 2019 Event Horizon Telescope (EHT) sub-mm observation of M87*, the first horizon-scale image in history, we are now in position to infer the physical properties of jet/accretion flow/black hole (JAB) systems through direct comparison of phenomenological models with the regions surrounding supermassive black holes. Using general relativistic magnetohydrodynamic (GRMHD) simulations of M87, we compare parametric models in which plasma imparts energy to synchrotron emitters via turbulent heating to those in which the emitters derive their energy directly from magnetic fields. Positrons are incorporated into the general relativistic ray tracer IPOLE to postprocess the GRMHD simulations-- showing stark differences in polarization signatures between standard and normal evolution (SANE) and magnetically arrested disk (MAD) accretion modes due to positron-mediated Faraday effects. MAD simulations with both types of emission model considered are concordant with EHT M87 linear and circular polarization constraints. The inclusion of electrons, positrons and protons in our radiative transfer pipeline thus provides a powerful probe of the composition and phenomenology of JAB systems. We then consider the role of positrons in the primordial plasma of the early Universe. From approximately 10ms to 10s after the Big Bang, relativistic positronium (electron-positron) plasma was a billion times more abundant than protons and neutrons. We consider GRMHD simulations in this unique environment, in which we model the accretion of positronium by primordial black holes. With the addition of rotation and the magnetorotational instability, we show how accreting primordial black holes could account for at least a percent-level contribution to the dark matter budget today, as well as the gamma ray background.

        Speaker: Richard Anantua (UT San Antonio)
      • 14:20
        Maximizing Direct Detection with HYPER Dark Matter 20m
        Speaker: Gilly Elor
      • 14:40
        Taquitos II 30m
        Speakers: Andrew Long (Rice University), Dorian Amaral (Rice University), Joel Meyers (Southern Methodist University)
      • 15:10
        Coffee 40m
      • 15:50
        Dark Matter in Extreme Astrophysical Environments 30m
        Speaker: Kuver Sinha (University of Oklahoma)
      • 16:20
        Supermassive Black Hole Binaries in Ultralight Dark Matter 20m
        Speaker: Barmak Shams Es Haghi (University of Texas at Austin)
      • 16:40
        Cosmological gravitational particle production of massive spin-2 particles 20m
        Speaker: Siyang Ling
      • 17:00
        Coffee 30m
      • 17:30
        The THESAN Project: Radiation-Hydrodynamic Simulations of the Epoch of Reionization 30m
        Speaker: Aaron Smith (UT Dallas)
      • 18:00
        Gravitational waves from Nnaturalness 20m
        Speaker: Mudit Rai (University of Pittsburgh)
      • 18:20
        PROBING SOLAR NEUTRINOS WITH CE𝞶NS AND FLAVOR-DEPENDENT RADIATIVE CORRECTIONS AT DARK MATTER DETECTORS 20m
        Speaker: Nityasa Mishra
      • 18:40
        Reception 2h 30m
  • Tuesday 10 October
    • 08:30 15:00
      Tuesday Session
      • 08:30
        Breakfast 40m
      • 09:10
        The Magnetic Mysteries of Magnetars 30m
        Speaker: Matthew Baring (Rice University)
      • 09:40
        On the gamma-ray emission from the core of the Sagittarius dwarf galaxy 20m
        Speaker: Addy Evans
      • 10:00
        Surfing Dark Matter Waves at the Windchime Experiment 20m
        Speaker: Dorian Amaral (Rice University)
      • 10:20
        Coffee 50m
      • 11:10
        Cosmology with Gravitational-Wave Multi-Messenger Observations 30m
        Speaker: Hsin-Yu Chen (UT Austin)
      • 11:40
        Harmonic Analysis Method to Search for Gravitational Waves with Pulsar Timing Arrays 20m
        Speaker: Jonathan Nay (UT Austin)
      • 12:00
        New Windows Into High Redshift Galaxies with Line Intensity Mapping 30m
        Speaker: Patrick Breysse (NYU)
      • 12:30
        Closing 10m
        Speakers: Andrew Long (Rice University), James Dent, Joel Meyers (Southern Methodist University), Prof. Kimberly Boddy (University of Texas at Austin), Louis Strigari (Texas A&M)