Session

Electromagnetic detectors and future prospects for multimessenger science and contributed talks

7 Oct 2022, 15:00

Conveners

Electromagnetic detectors and future prospects for multimessenger science and contributed talks

  • Giancarlo Cella (Istituto Nazionale di Fisica Nucleare)

Presentation materials

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  1. Andrea Melandri (INAF - OAB)
    07/10/2022, 15:00
    Invited talk

    The discovery of gravitational waves (GWs) from the coalescence of compact objects is one of the most exciting scientific discoveries of the last decade, and started a “golden age” for the multi-messenger astronomy. Merging of either black hole-neutron star or two neutron stars are among the most promising GW sources able to generate electromagnetic counterparts, but also core-collapsing...

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  2. Stefano Germani (Istituto Nazionale di Fisica Nucleare)
    07/10/2022, 15:30
    Invited talk

    The recent detection Gamma Ray Burts (GRB) by Imaging Atmospheric Cherenkov Telescopes opened up the possibility of Multi Messenger (MM) detection of neutron star merger events and the assiciated GRBs with Gravitational Waves (GW) and Very High Energy (VHE) gamma rays.
    New facilities with enhanced sensitivities which are under construction or will start construction in the near future...

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  3. Stefano Ciprini (INFN)
    Contributed talk

    In this contribution I just report some artistic and graphical ideas and products created, in particular,
    for astro-particle physics experiments and space observatories.
    With so much information, data analysis and science results being collected through high-energy
    physics and multimessenger particle astrophysics experiments and observatories, we must have
    a way to produce data...

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  4. Federica Giacchino (INFN)
    Contributed talk

    Axion-like particles (ALPs) and other feebly interacting particles (FIPs) at sub-GeV scales has gen-
    erated a lot of interest in the recent years.
    Stars are good FIPs factories and consequently can be detected through their interaction with the
    interstellar matter or decay in standard particles. Many sources are taken as target, such as the
    sun and SNe.
    I will illustrate how high-energy...

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