Recent advances on multimessenger astrophysics: Centaurus A, GW 170817 and KM3-230213A

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A90232%2F25%3A00641936" target="_blank" >RIV/68378271:90232/25:00641936 - isvavai.cz</a>

Výsledek na webu

<a href="https://doi.org/10.1142/S0217751X25300169" target="_blank" >https://doi.org/10.1142/S0217751X25300169</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.1142/S0217751X25300169" target="_blank" >10.1142/S0217751X25300169</a>

Jazyk výsledku

angličtina

Název v původním jazyce

Recent advances on multimessenger astrophysics: Centaurus A, GW 170817 and KM3-230213A

Popis výsledku v původním jazyce

We review recent advances in multimessenger astrophysics, with particular emphasis on Centaurus A and on two pivotal events: the gravitational-wave detection GW 170817 and the ultra-high-energy neutrino KM3-230213A. Centaurus A is the prototype multimessenger source. The GW 170817 event, arising from a binary neutron star merger, marked a transformative moment in astronomy through the joint observation of gravitational waves and a broad spectrum of electromagnetic signals. The KM3-230213A neutrino, detected by the KM3NeT Collaboration, is the most energetic neutrino observed to date and poses significant challenges for current models, given its tension with null results from IceCube and the Pierre Auger Observatory. We assess astrophysical interpretations, including galactic, cosmogenic and transient extragalactic sources, as well as implications for cosmic-ray acceleration. These cases underscore the scientific potential of high-energy multimessenger events in probing both the extreme universe and new physics.

Název v anglickém jazyce

Recent advances on multimessenger astrophysics: Centaurus A, GW 170817 and KM3-230213A

Popis výsledku anglicky

We review recent advances in multimessenger astrophysics, with particular emphasis on Centaurus A and on two pivotal events: the gravitational-wave detection GW 170817 and the ultra-high-energy neutrino KM3-230213A. Centaurus A is the prototype multimessenger source. The GW 170817 event, arising from a binary neutron star merger, marked a transformative moment in astronomy through the joint observation of gravitational waves and a broad spectrum of electromagnetic signals. The KM3-230213A neutrino, detected by the KM3NeT Collaboration, is the most energetic neutrino observed to date and poses significant challenges for current models, given its tension with null results from IceCube and the Pierre Auger Observatory. We assess astrophysical interpretations, including galactic, cosmogenic and transient extragalactic sources, as well as implications for cosmic-ray acceleration. These cases underscore the scientific potential of high-energy multimessenger events in probing both the extreme universe and new physics.

Druh

J_imp - Článek v periodiku v databázi Web of Science

CEP obor

—

OECD FORD obor

10303 - Particles and field physics

Projekt

—

Návaznosti

—

Rok uplatnění

2025

Kód důvěrnosti údajů

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Název periodika

International Journal of Modern Physics. A

ISSN

0217-751X

e-ISSN

1793-656X

Svazek periodika

40

Číslo periodika v rámci svazku

30

Stát vydavatele periodika

SG - Singapurská republika

Počet stran výsledku

22

Strana od-do

2530016

Kód UT WoS článku

001565708000001

EID výsledku v databázi Scopus

2-s2.0-105015358657