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Volumn 92, Issue 11, 2004, Pages

Effects of the Sagittarius Dwarf Tidal Stream on Dark Matter Detectors

Author keywords

[No Author keywords available]

Indexed keywords

DETECTORS; ISOTHERMS; MODULATION; ORBITS; SATELLITES; SOLAR ENERGY; VECTORS;

EID: 2342567037     PISSN: 00319007     EISSN: None     Source Type: Journal    
DOI: 10.1103/PhysRevLett.92.111301     Document Type: Article
Times cited : (131)

References (20)
  • 4
    • 85032426438 scopus 로고    scopus 로고
    • K. Freese, P. Gondolo, and H. Newberg, astro-ph/ 0309279
    • K. Freese, P. Gondolo, and H. Newberg, astro-ph/ 0309279.
  • 6
    • 85032426917 scopus 로고    scopus 로고
    • note
    • Based on hierarchical clustering, it is likely that a clump contributes l%-5%. to the local dark matter density [7].
  • 14
    • 85032427859 scopus 로고    scopus 로고
    • note
    • We take X̂ the direction of the Galactic center, so the Sun is at (X, Y, Z) = (-8.5, 0, 0).
  • 18
    • 85032428872 scopus 로고    scopus 로고
    • note
    • The conversion from keVee to keV recoil energy is found from the quenching factor, 0.09 for I and 0.3 for Na.
  • 19
    • 85032425967 scopus 로고    scopus 로고
    • note
    • For DAMA, there are two steps, at lower energy due to I and at higher energy due to Na.
  • 20
    • 85032430254 scopus 로고    scopus 로고
    • note
    • Since the DAMA data are not public, we are compelled to leave the analysis to the experimentalists.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.