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GWADW2021 Gravitational Wave Advanced Detector Workshop

17–21 May 2021
remote
Europe/Rome timezone

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Session

Recorded talks: GW Physics

RTPh
17 May 2021, 06:00
remote

remote

Conveners

Recorded talks: GW Physics: GW Physics Talks Index

  • Edward Porter (APC-Paris)

Presentation materials

There are no materials yet.

  1. 138. The Science Case for the Einstein Telescope
    Michele Maggiore (Geneva University)
    17/05/2021, 06:00
    Gravitational wave perspective
    talk

    I will give a broad overview of the scientific targets of the Einstein Telescope in astrophysics, cosmology, and fundamental physics.

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  2. 164. On the nature of the remnants in mergers of compact binaries
    Walter Del Pozzo (P)
    17/05/2021, 06:20
    Gravitational wave perspective
    talk

    Observations of binary black holes mergers from the LIGO-Virgo interferometers provide a window to investigate the highly dynamical regime of gravity as well as the nature of astrophysical black holes. The black hole born from the merger of its progenitors emits gravitational waves with a characteristic spectrum, the so-called ringdown, whose direct detection provide informations about the...

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  3. 168. Searching for Primordial Black Holes: The Role of 3rd Generation Gravitational Wave Detectors
    Gabriele Franciolini (University of Geneva)
    17/05/2021, 06:40
    Gravitational wave perspective
    talk

    Primordial black holes form in the early universe and can give rise to mergers at high redshift. This distinctive feature can be exploited by 3G detectors to distinguish primordial binaries from the ones generated by other astrophysical formation channels. By considering a primordial black hole population compatible with current gravitational wave data, we show that 3G detectors such as the...

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  4. 140. Ranking the Love for the neutron star equation of state with third-generation detectors
    Andrea Maselli (Sapienza University of Rome)
    17/05/2021, 06:55
    Gravitational wave perspective
    talk

    Gravitational wave measurements of the tidal deformability
    in neutron-star binary coalescences are golden sources to infer properties of the still unknown equation of state (EoS) of dense matter above
    the nuclear saturation density. In this talk I will show how, using a
    Bayesian-ranking test we can quantify the ability of current and future gravitational-wave observations to discriminate...

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  5. 71. Challenges and Opportunities of Ultra-High-Frequency Gravitational Wave Detection
    Francesco Muia (University of Cambridge)
    17/05/2021, 07:10
    Gravitational wave perspective
    talk

    The first direct detection of gravitational waves by the LIGO and VIRGO collaborations has opened up new avenues to explore the Universe. Currently operating and planned gravitational wave detectors mostly focus on the range below 10 kHz, where signatures from known astrophysical sources are expected to be discovered. However, based on what happens with the electromagnetic spectrum, there...

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