from 28 November 2022 to 2 December 2022 (Europe/Warsaw)
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Astrophysics and GW Detectors

Place

Location: ONLINE
Address: ONLINE
Room: ONLINE
Date: 2 Dec 14:30 - 19:00

Description

Gravitational Waves from Astrophysical Sources and GW Detectors

Conveners

    • Dr. de Muia, Francesco

Timetable | Contribution List

Displaying 7 contributions out of 7
Presented by Prof. John ELLIS on 02/12/2022 at 17:30
Presented by Volodymyr TAKHISTOV on 02/12/2022 at 13:30
Gravitational waves have offered us a whole new way of looking at our Universe. So far, we have seen them in the ~10-100 Hz range, and there are hints that we might soon see them in the nanohertz regime. However, there are parts of the frequency space that are currently not covered by any future or planned observations. I will explain how we can use upcoming photometric surveys to bridge the gaps ... More
Presented by Kris PARDO on 02/12/2022 at 15:30
Presented by Prof. Laura SAGUNSKI on 02/12/2022 at 16:30
The Peters formula, which tells how the coalescence time of a binary system emitting gravitational radiation is determined by the initial size and shape of the elliptic orbit, is often used in estimating the merger rate of primordial black holes and the gravitational wave background from the mergers. Valid as it is in some interesting scenarios, such as the analysis of the LIGO-Virgo events, the P ... More
Presented by Heling DENG on 02/12/2022 at 16:00
I will discuss how specially designed SRF cavities can have enhanced sensitivity to axions and gravitational waves for frequencies below GHz. The projected sensitivity of a futuristic apparatus covers the QCD line over two decades of axion dark matter mass and new parameter space all the way down to the fuzzy dark matter limit. Additionally, the same concept with a different geometry has the poten ... More
Presented by Raffaele-Tito D'AGNOLO on 02/12/2022 at 14:00
The first seven years of direct gravitational wave detection have had a huge impact not only on astrophysics, but also on cosmology and fundamental physics. We’ll start by reviewing some ways cosmologically-motivated departures from GR can affect gravitational wave propagation. Then I’ll present some constraints from current data and forecasts for future detectors using these methods. In parti ... More
Presented by Tessa BAKER on 02/12/2022 at 14:30
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