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Physical Review Letters

Volumn 114, Issue 16, 2015, Pages

Modeling the dynamics of tidally interacting binary neutron stars up to the merger

(4) Bernuzzi, Sebastiano a,b Nagar, Alessandro c Dietrich, Tim d Damour, Thibault c

a CALIFORNIA INSTITUTE OF TECHNOLOGY (United States)

b UNIVERSITY OF PARMA (Italy)

c INSTITUT DES HAUTES ÉTUDES SCIENTIFIQUES (France)

d FRIEDRICH SCHILLER UNIVERSITY JENA (Germany)

Author keywords

[No Author keywords available]

Indexed keywords

DYNAMICS; EQUATIONS OF STATE; FLOCCULATION; GRAVITATION; GRAVITATIONAL EFFECTS; GRAVITY WAVES; MERGING; NEUTRONS;

AMPLIFICATION EFFECTS; BINARY NEUTRON STARS; FITTING PARAMETERS; GRAVITATIONAL-WAVE SIGNALS; NUMERICAL RELATIVITY; RELATIVISTIC DYNAMICS; SEMI-ANALYTICAL MODEL; TIDAL INTERACTIONS;

STARS;

EID: 84929590780 PISSN: 00319007 EISSN: 10797114 Source Type: Journal
DOI: 10.1103/PhysRevLett.114.161103 Document Type: Article

Times cited : (309)

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* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.