Possible direct method to determine the radius of a star from the spectrum of gravitational wave signals. II. Spectra for various cases

Physical Review D

Volumn 63, Issue 6, 2001, Pages

  Saijo, Motoyuki ^a   Nakamura, Takashi ^b  

^a UNIVERSITY OF ILLINOIS AT URBANA CHAMPAIGN   (United States)

^b KYOTO UNIVERSITY   (Japan)

Author keywords

[No Author keywords available]

Indexed keywords

ARTICLE; ASTRONOMY; GRAVITY; INTERFEROMETER; MATHEMATICAL ANALYSIS; NEUTRON; ROTATION; SIGNAL PROCESSING; SPECTRUM; WAVEFORM;

EID: 0034909304     PISSN: 05562821     EISSN: None     Source Type: Journal    
DOI: 10.1103/PhysRevD.63.064004     Document Type: Article

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