Binary Coalescences as Sources of Ultrahigh-Energy Cosmic Rays-Reference-Cited by-同舟云学术

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Binary Coalescences as Sources of Ultrahigh-Energy Cosmic Rays

Published:2024-02-27 Issue:9 Volume:132 Page:
ISSN:0031-9007
Container-title:Physical Review Letters
language:en
Short-container-title:Phys. Rev. Lett.

Author:

Pereira Jonas P.^ORCID,Coimbra-Araújo Carlos H.,dos Anjos Rita C.^ORCID,Coelho Jaziel G.^ORCID

Funder

Conselho Nacional de Desenvolvimento Científico e Tecnológico

Fundação de Amparo à Pesquisa do Estado de São Paulo

Fundação Araucária

L’Oreal Brazil

Fenômenos Extremos do Universo

National Laboratory for Scientific Computing

Publisher

American Physical Society (APS)

Link

http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevLett.132.091401/fulltext

Reference103 articles.

1. Observation of Gravitational Waves from a Binary Black Hole Merger

2. GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral

3. Multi-messenger Observations of a Binary Neutron Star Merger

4. GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo during the Second Part of the Third Observing Run

5. Population of Merging Compact Binaries Inferred Using Gravitational Waves through GWTC-3

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1. 4D Embedded Rotating Black Hole as a Particle Accelerator in the Presence of Magnetic Fields;Universe;2024-09-04

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