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International conference PUMA22 Probing the Universe with Multimessenger Astrophysics

26–30 Sept 2022
Sestri Levante
Europe/Rome timezone

Session

Session 7

29 Sept 2022, 09:00
Sestri Levante

Sestri Levante

Grand Hotel dei Castelli, Via Penisola Levante, 26, 16039 Sestri Levante (GE), Italy

Conveners

Session 7

  • ALESSIO Caminata (Istituto Nazionale di Fisica Nucleare)
  • Anna Marini (Istituto Nazionale di Fisica Nucleare)

Presentation materials

There are no materials yet.

  1. 22. The LISA orbiting observatory for low frequency gravitational waves
    William Weber (TIFP)
    29/09/2022, 09:00
    Oral contribution

    The Laser Interferometer Space Antenna, LISA, is the ESA "L3" large mission, destined to be an orbiting observatory for gravitational waves in the 0.1 mHz to 1 Hz band. This will open a scientifically rich and deep window for astronomy, cosmology, and fundamental physics in a gravitational wave band that can only be reached from space. We present here the observatory science potential --...

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  2. 33. Physics prospects of the Einstein Telescope
    Michele Maggiore (Geneva University)
    29/09/2022, 09:30
    Oral contribution
  3. 28. Supernova remnants
    Manami Sasaki (Friedrich-Alexander-Universitaet)
    29/09/2022, 10:00
    Oral contribution
  4. 34. Supernovae explosions: an observational perspective
    Jozsef Vinko (University of Szeged )
    29/09/2022, 11:00
    Oral contribution
  5. 11. GWSkySim: a fast simulator of gravitational wave sources with multimessenger applications
    Mr Nunziato Sorrentino (University of Pisa and INFN Pisa)
    29/09/2022, 11:30
    Oral contribution

    The observation of the GW170817 event has shown how multimessenger astronomy is a powerful tool to investigate the most energetic phenomena in the Universe. Simulations are an important tool to study multimessenger emission and understand the constraints that can be put using joined electromagnetic and gravitational-wave observations. For that purpose, we developed the Gravitational Wave Sky...

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  6. 76. Status of the Cryogenic AntiCoincidence detector for ATHENA X-IFU: DM and SM models
    Giovanni Gallucci (Istituto Nazionale di Fisica Nucleare)
    29/09/2022, 11:50
    Oral contribution

    The study of the X-ray sky, in particular transient sources, is an important part of the multimessenger astrophysics concurrent to Gravitational Waves and Neutrino Observations. It helps to understand different phenomena, e.g. the central engine and jet physics in compact binary mergers, the equation of state of neutron stars, cosmic accelerators, and the origin of Cosmic Rays (CRs), the...

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  7. 97. Cosmology from the weak lensing of gravitational waves
    Charlie Mpetha
    29/09/2022, 12:10
    Oral contribution

    Planned and proposed future gravitational wave detectors will observe huge numbers of binary mergers. It is timely to explore cosmological tests that can be performed with this forthcoming plethora of data, in combination with present and future galaxy surveys. We forecast a combined standard siren + weak lensing analysis, where perturbations in the propagation of gravitational waves by...

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