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Volumn 67, Issue 2, 2003, Pages

LISA, binary stars, and the mass of the graviton

Author keywords

[No Author keywords available]

Indexed keywords

ARTICLE; ASTRONOMY; COSMOS; ELECTROMAGNETIC FIELD; GRAVITY; MASS; MATHEMATICAL ANALYSIS; MEASUREMENT; SPACE; WAVEFORM;

EID: 4744371559     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.67.024015     Document Type: Article
Times cited : (53)

References (24)
  • 4
    • 85038317980 scopus 로고    scopus 로고
    • P. Bender et al., LISA Pre-Phase: A Report, 2nd ed., 1998
    • P. Bender et al., LISA Pre-Phase: A Report, 2nd ed., 1998.
  • 6
    • 85038279654 scopus 로고    scopus 로고
    • For details regarding the proposed science for the SIM mission, see Science with the Space Interferometry Mission, edited by S. Unwin and S. Turyshev, 2002; available from the SIM website, http://sim.jpl.nasa.gov/
    • For details regarding the proposed science for the SIM mission, see Science with the Space Interferometry Mission, edited by S. Unwin and S. Turyshev, 2002; available from the SIM website, http://sim.jpl.nasa.gov/.
  • 8
    • 85038267382 scopus 로고    scopus 로고
    • Unless otherwise noted, geometric units where (Formula presented) are used throughout
    • Unless otherwise noted, geometric units where (Formula presented) are used throughout.
  • 11
    • 85038335094 scopus 로고    scopus 로고
    • Note that this value for (Formula presented) is specified for the 1 way position noise budget, as is the expression in Eq. (10), and has many constituent noises. Often, pure shot noise is considered as the limiting source of noise for the LISA floor; in that case, Eq. (10) should be replaced by Eq. (13) of Ref. 10
    • Note that this value for (Formula presented) is specified for the 1 way position noise budget, as is the expression in Eq. (10), and has many constituent noises. Often, pure shot noise is considered as the limiting source of noise for the LISA floor; in that case, Eq. (10) should be replaced by Eq. (13) of Ref. 10.
  • 12
    • 85038271313 scopus 로고    scopus 로고
    • The low frequency approximation is adequate for our purposes here. If one uses the full sensitivity curve (available at http://www.srl.caltech.edu/(Formula presented)shane/sensitivity/) instead, the results obtained differ only insubstantially
    • The low frequency approximation is adequate for our purposes here. If one uses the full sensitivity curve (available at http://www.srl.caltech.edu/(Formula presented)shane/sensitivity/) instead, the results obtained differ only insubstantially.
  • 17
    • 85038307309 scopus 로고    scopus 로고
    • astro-ph/0111358
    • K. Wu et al., astro-ph/0111358.
    • Wu, K.1
  • 18
    • 85038321494 scopus 로고    scopus 로고
    • G.L. Israel, W. Hummel, S. Covino, S. Campana, I. Appenzeller, W. Gässler, K.-H. Mantel, G. Marconi, C.W. Mauche, U. Munari, I. Negueruela, H. Nicklas, G. Rupprecht, R.L. Smart, O. Stahl, and L. Stella, astro-ph/0203043
    • G.L. Israel, W. Hummel, S. Covino, S. Campana, I. Appenzeller, W. Gässler, K.-H. Mantel, G. Marconi, C.W. Mauche, U. Munari, I. Negueruela, H. Nicklas, G. Rupprecht, R.L. Smart, O. Stahl, and L. Stella, astro-ph/0203043.
  • 19
    • 85038343036 scopus 로고    scopus 로고
    • astro-ph/0104388
    • D.R. Lorimer, astro-ph/0104388.
    • Lorimer, D.R.1
  • 20
    • 85038302521 scopus 로고    scopus 로고
    • astro-ph/0005214
    • V.M. Kaspi, astro-ph/0005214.
    • Kaspi, V.M.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.