메뉴 건너뛰기




Volumn 66, Issue 6, 2002, Pages

The phase-space structure of a dark-matter halo: Implications for dark-matter direct detection experiments

Author keywords

[No Author keywords available]

Indexed keywords

ARTICLE; COSMIC RADIATION; COSMOLOGICAL PHENOMENA; COSMOS; ELEMENTARY PARTICLE; GRAVITY; MATHEMATICAL ANALYSIS; MOTION; SOLAR RADIATION; SPACE; VELOCITY;

EID: 0037105272     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.66.063502     Document Type: Article
Times cited : (111)

References (46)
  • 15
    • 0035954703 scopus 로고    scopus 로고
    • EDELWEISS Collaboration, A. Benoit, Phys. Lett. B 513, 15 (2001).
    • (2001) Phys. Lett. B , vol.513 , pp. 15
    • Benoit, A.1
  • 20
  • 42
    • 85038275395 scopus 로고    scopus 로고
    • astro-ph/0109296
    • P. Sikivie, astro-ph/0109296.
    • Sikivie, P.1
  • 45
    • 85038267463 scopus 로고    scopus 로고
    • This is because (Formula presented) and thus if (Formula presented) then (Formula presented)
    • This is because (Formula presented) and thus if (Formula presented) then (Formula presented)
  • 46
    • 85038341419 scopus 로고    scopus 로고
    • If initially (Formula presented) is the phase-space volume occupied by the satellite, and if (Formula presented) is its final volume, then (Formula presented) where, as discussed above, (Formula presented) is the volume given by the orbit, and is much larger than the original volume of the satellite.
    • If initially (Formula presented) is the phase-space volume occupied by the satellite, and if (Formula presented) is its final volume, then (Formula presented) where, as discussed above, (Formula presented) is the volume given by the orbit, and is much larger than the original volume of the satellite.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.