Journal Article

GSI-2025-00162

http://join2-wiki.gsi.de/foswiki/pub/Main/Artwork/join2_logo100x88.png Gravitational-wave model for neutron star merger remnants with supervised learning

Soultanis, T. (Corresponding author)GSI* ; Maltsev, K. ; Bauswein, A.GSI* ; Chatziioannou, K. (Corresponding author) ; Röpke, F. K. ; Stergioulas, N.

2025
American Physical Society Ridge, NY

This record in other databases:

Please use a persistent id in citations: doi:10.1103/PhysRevD.111.023002

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Contributing Institute(s):

1. Nukleare Astrophysik & Struktur (KNA)

Research Program(s):

1. 612 - Cosmic Matter in the Laboratory (POF4-612) (POF4-612)
2. HEAVYMETAL - How Neutron Star Mergers make Heavy Elements (101071865) (101071865)
3. ElementsHessen - ELEMENTS : Exploring the Universe from microscopic to macroscopic scales (ELEMENTS cluster project) (ElementsHessen) (ElementsHessen)
4. SFB 1245 B07 - Zustandsgleichung und Nukleosynthese in Neutronensternverschmelzungen (B07) (437997523) (437997523)

Experiment(s):

1. no experiment theory work (theory)

Appears in the scientific report 2025

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Database coverage:
; Clarivate Analytics Master Journal List ; Current Contents - Electronics and Telecommunications Collection ; Current Contents - Physical, Chemical and Earth Sciences ; Ebsco Academic Search ; Essential Science Indicators ; IF >= 5 ; JCR ; SCOAP3 sponsored Journal ; SCOPUS ; Science Citation Index Expanded ; Web of Science Core Collection

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