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AstroParticle Symposium 2022

October 31, 2022 to November 25, 2022
Institut Pascal
Europe/Paris timezone

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Session

Conference day

Nov 2, 2022, 9:30 AM
Institut Pascal

Institut Pascal

530 Rue André Rivière 91400 Orsay

Conveners

Conference day: Welcome

  • There are no conveners in this block

Conference day: Week 1

  • Lucien Heurtier

Conference day

  • Mathias Pierre

Conference day: Week 1

  • Simon Clery

Conference day

  • Alejandro Ibarra

Conference day

  • There are no conveners in this block

Conference day

  • There are no conveners in this block

Conference day: Conference day

  • There are no conveners in this block

Conference day

  • There are no conveners in this block

Conference day

  • There are no conveners in this block

Presentation materials

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  1. 49. Welcoming address
    Mrs Tiina Suomijärvi (P2I - Graduate School of Physics)
    11/2/22, 9:30 AM
  2. 50. The Pascal Institute
    Mr Yves Balkanski
    11/2/22, 9:45 AM
  3. 1. Gravitational portal at the end of inflation
    Simon Clery
    11/2/22, 10:00 AM
  4. 13. Dark matter production during preheating
    Jong Hyun Yoon
    11/2/22, 10:20 AM
  5. 14. Searching for supersymmetric LLPs
    Donald Kpatcha
    11/2/22, 10:40 AM
  6. 15. Primordial Black Holes from Dissipation During Inflation
    Marcos Garcia
    11/2/22, 11:00 AM
  7. 16. Non-perturbative gravitational production of vector Dark Matter
    Ms Anna Socha
    11/2/22, 11:40 AM
  8. 17. Dark matter from the primordial plasma: from freeze-in to pandemic production
    Mr Torsten Bringmann
    11/2/22, 12:00 PM
  9. 18. Observational signatures of compact dark stars
    Mr Alejandro Ibara
    11/2/22, 12:20 PM
  10. 28. Boltzmann or Bogoliubov? A Case of Gravitational Particle Production
    Mr Kunio Kaneta
    11/2/22, 12:40 PM
  11. 20. Scalar production in the Early Universe
    Mr Oleg Lebedev
    11/2/22, 2:10 PM
  12. 21. Unitarity in Higgs inflation and UV complete models
    Mr Hyun Min Lee
    11/2/22, 2:30 PM
  13. 25. Dark Matter beyond freeze-in
    Sabir Ramanazov
    11/2/22, 2:50 PM
  14. 26. Imprints of Mini Primordial Black Holes In Cosmological Data
    Lucien Heurtier
    11/2/22, 3:10 PM
  15. 22. Reheating and dark matter freeze-in in the Higgs-R^2 inflation model
    Ms Adriana Menkara
    11/2/22, 4:00 PM
  16. 23. Long-lived particles and co-scattering
    Mrs Genevieve Belanger
    11/2/22, 4:20 PM
  17. 24. Dark matter and baryogenesis from freeze-in
    Andreas Goudelis
    11/2/22, 4:40 PM
  18. 27. Dark Matter Production from Preheating and Structure Formation Constraints
    Mr Mathias Pierre
    11/2/22, 5:00 PM
  19. 66. Cosmology with Fast Radio Bursts
    Robert Reischke, Steffen Hagstotz
    11/15/22, 10:30 AM
  20. 59. Lessons learned from multi-messenger models of active galaxies
    Xavier Rodriguez
    11/15/22, 11:00 AM

    Evidence is pointing more and more clearly to blazars and other active galaxies as significant multi-messenger sources.
    In this talk I summarize some of the latest developments in the modeling of cosmic-ray interactions in blazars and how these models can explain recent associations between IceCube events and individual sources. I also discuss the predicted flare signatures across the...

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  21. 60. Teieresias Radiative Transfer: Consistently modelling the Kilonova Afterglow with Relativistic Hydrodynamics.
    Ethan van Woerkom
    11/15/22, 11:30 AM

    The kilonova afterglow is the final phase of the electromagnetic counterpart to a BNS/NSBH merger, and it is the only predicted counterpart of GW170817, which has not been observed yet. The kilonova afterglow lightcurve is dependent on the mass, velocity and angular distributions of the ejecta, and thus represents an opportunity to independently constrain these properties. We present Teiresias...

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  22. 62. Multi-Messenger studies: From ideas to realization
    Jakob Nordin
    11/15/22, 12:00 PM

    I will use the recently observed association between extragalactic neutrinos and tidal disruption events as a starting point for an exploration of the tools needed to go from a scientific hypothesis to an active, high throughput time-domain program. I will introduce some of the concepts built into the AMPEL platform which were designed to make this possible.

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  23. 58. Fast astrophysical multi-messenger astrophysics with DWF
    Anais Möller (Swinburne University)
    11/15/22, 2:00 PM

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    The Deeper Wider Fast Programme (DWF) aims to discover and rapidly follow up the fastest bursts in the Universe (those lasting only milliseconds to hours). For this, we execute a main strategy comprised of coordinated international multi-facility, all-wavelength, and multi-messenger telescope observing runs to detect and follow up fast...

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  24. 56. 20 years of INTEGRAL
    Philippe Laurent
    11/15/22, 2:30 PM
  25. 57. The GRINTA mission for the next decade exploitation of the multimessenger sky
    Lorenzo Natalucci
    11/15/22, 3:00 PM

    The Gamma-Ray International Transient Array observatory (GRINTA) is a fast class mission designed to be a major breakthrough in the next decade (>2030) time domain astronomy, in particular for the multi-messenger domain. Transient signals from sources of gamma-ray bursts, gravitational waves and high energy neutrinos are known to produce hard X-rays that can be detected by an instrument with...

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  26. 61. General Coordinates Network (GCN): NASA’s Next Generation Time-Domain and Multimessenger Astronomy Alert System
    Leo Singer
    11/15/22, 4:00 PM

    The Gamma-ray Coordinates Network (GCN) is a public collaboration platform run by NASA for the astronomy research community to share alerts and rapid communications about high-energy, multimessenger, and transient phenomena. Over the past 30 years, GCN has helped enable many seminal advances by disseminating observations, quantitative near-term predictions, requests for follow-up observations,...

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  27. 63. The H.E.S.S transients follow-up system
    Halim ASHKAR (CNRS - Ecole Polytechnique - LLR)
    11/15/22, 4:30 PM
  28. 64. GRB observations with IACTs
    Sylvia Zhu (DESY)
    11/15/22, 5:00 PM

    In the last few years, very-high-energy (>100 GeV) emission from gamma-ray bursts (GRBs) has been detected for the first time, allowing us to build a multiwavelength picture of GRBs that extends all the way up to TeV energies. Now that we’ve detected a few GRBs, the question becomes: What’s next? In this talk, I will describe the GRB programs of the current generation of air Cherenkov...

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  29. 65. Astro-COLIBRI in practice
    Patrick Reichherzer (Ruhr-Universität Bochum (RUB))
    11/15/22, 5:30 PM

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    The study of flaring astrophysical events in the multi-messenger approach requires instantaneous follow-up observations to better understand the nature of these events through complementary observational data. We present Astro-COLIBRI as a meta platform for the patchwork of different specific tools in the real-time multi-messenger...

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  30. 78. Numerical local source modeling of active galactic nuclei
    Leander Schlegel (Ruhr-Universität Bochum)
    11/24/22, 10:30 AM
  31. 79. Constraining cosmic-ray sources with efficient propagation models
    Mr Xavier Rodrigues
    11/24/22, 10:45 AM
  32. 80. Horizon of UHECRs in galaxy clusters
    Antonio Condorelli (IJCLAB)
    11/24/22, 11:00 AM
  33. 81. Constraining transient sources of UHECRs with arrival directions
    Sullivan MARAFICO
    11/24/22, 11:15 AM
  34. 82. Indications of the Gerasimova-Zatsepin effect in the Auger scalers data
    Mr Martin Schimassek (IJCLab)
    11/24/22, 11:30 AM
  35. 83. 450 years of de nova stella - Tycho's supernova
    Dr Fabio ACERO (AIM, CEA, CNRS, Universite Paris-Saclay, Universite Paris)
    11/24/22, 11:45 AM
  36. 84. Flares associated with the synchrotron emission from the Crab pulsar wind nebula
    Michelle Tsirou (DESY)
    11/24/22, 12:00 PM
  37. 86. STeVeCAT
    Lucas Greaux
    11/24/22, 12:15 PM
  38. 87. Placehoder
    Sara Buson (Univ. of Wuerzburg)
    11/24/22, 12:30 PM
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    Mr .. ..
  40. 88. Placeholder
  41. 77. The EOSC multi-wavelength analysis prototype (MAP) for black hole models
    Mr Sheridan Lloyd
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