Repozitorij Univerze v Novi Gorici

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Naslov:Chasing Gravitational Waves with the Cherenkov Telescope Array
Avtorji:ID Green, J. G. (Avtor)
ID BHATTACHARYYA, Saptashwa (Avtor)
ID Pérez-Romero, Judit (Avtor)
ID Stanič, Samo (Avtor)
ID VODEB, Veronika (Avtor)
ID Vorobiov, Serguei (Avtor)
ID Zavrtanik, Danilo (Avtor)
ID Zavrtanik, Marko (Avtor)
ID Živec, Miha (Avtor), et al.
Datoteke:.pdf ICRC2023_1534.pdf (1,66 MB)
MD5: 995961E9C226B65EFC902FF1C4659FF6
 
URL https://pos.sissa.it/444/
 
URL https://pos.sissa.it/444/1534/pdf
 
Jezik:Angleški jezik
Vrsta gradiva:Delo ni kategorizirano
Tipologija:1.08 - Objavljeni znanstveni prispevek na konferenci
Organizacija:UNG - Univerza v Novi Gorici
Opis:The detection of gravitational waves (GWs) from a binary neutron star (BNS) merger by Advanced LIGO and Advanced Virgo (GW170817), along with the discovery of the electromagnetic counterparts of this GW event, ushered in a new era of multimessenger astronomy, providing the first direct evidence that BNS mergers are progenitors of short gamma-ray bursts (GRBs). Such events may also produce very-high-energy (VHE, > 100 GeV) photons which have yet to be detected in coincidence with a GW signal. The Cherenkov Telescope Array (CTA) is a next-generation VHE observatory which aims to be indispensable in this search, with an unparalleled sensitivity and ability to slew anywhere on the sky within a few tens of seconds. Achieving such a feat will require a comprehensive real-time strategy capable of coordinating searches over potentially very large regions of the sky. This work will evaluate and provide estimations on the number of GW-CTA events determined from simulated BNS systems and short GRBs, considering both on and off-axis emission. In addition, we will present and discuss the prospects of potential follow-up strategies with CTA.
Ključne besede:gravitational waves (GWs), binary neutron star (BNS) merger, short gamma-ray bursts (GRBs), Advanced LIGO and Advanced Virgo, GW electromagnetic counterparts, multimessenger astrophysics, very-high-energy gamma-rays, Cherenkov Telescope Array
Status objave pri reviji:Objavljeno
Leto izida:2023
PID:20.500.12556/RUNG-8411 Novo okno
COBISS.SI-ID:164621571 Novo okno
NUK URN:URN:SI:UNG:REP:ARYTEWKD
Datum objave v RUNG:15.09.2023
Število ogledov:129
Število prenosov:2
Metapodatki:XML RDF-CHPDL DC-XML DC-RDF
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Skupna ocena:(0 glasov)
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Gradivo je del monografije

Naslov:38th International Cosmic Ray Conference
Podnaslov:ICRC2023
Kraj izida:Trieste, SISSA
Leto izida:2023

Gradivo je financirano iz projekta

Financer:ARRS - Agencija za raziskovalno dejavnost Republike Slovenije
Številka projekta:P1-0031
Naslov:Večglasniška astrofizika

Licence

Licenca:CC BY-NC-ND 4.0, Creative Commons Priznanje avtorstva-Nekomercialno-Brez predelav 4.0 Mednarodna
Povezava:http://creativecommons.org/licenses/by-nc-nd/4.0/deed.sl
Opis:Najbolj omejujoča licenca Creative Commons. Uporabniki lahko prenesejo in delijo delo v nekomercialne namene in ga ne smejo uporabiti za nobene druge namene.

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