메뉴 건너뛰기




Volumn 72, Issue 8, 2005, Pages

Do current WIMP direct measurements constrain light relic neutralinos?

Author keywords

[No Author keywords available]

Indexed keywords


EID: 29744432426     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.72.083521     Document Type: Article
Times cited : (47)

References (43)
  • 1
    • 0038408692 scopus 로고    scopus 로고
    • PRVDAQ 0556-2821 10.1103/PhysRevD.67.063519
    • A. Bottino, N. Fornengo, and S. Scopel, Phys. Rev. D 67, 063519 (2003). PRVDAQ 0556-2821 10.1103/PhysRevD.67.063519
    • (2003) Phys. Rev. D , vol.67 , pp. 063519
    • Bottino, A.1    Fornengo, N.2    Scopel, S.3
  • 6
    • 20144365141 scopus 로고    scopus 로고
    • APHYEE 0927-6505 10.1016/j.astropartphys.2005.01.006
    • G. Angloher (CRESST Collaboration), Astropart. Phys. 23, 325 (2005). APHYEE 0927-6505 10.1016/j.astropartphys.2005.01.006
    • (2005) Astropart. Phys. , vol.23 , pp. 325
    • Angloher, G.1
  • 7
    • 33644552158 scopus 로고    scopus 로고
    • PRVDAQ 0556-2821 10.1103/PhysRevD.71.122002
    • V. Sanglard (EDELWEISS Collaboration), Phys. Rev. D 71, 122002 (2005). PRVDAQ 0556-2821 10.1103/PhysRevD.71.122002
    • (2005) Phys. Rev. D , vol.71 , pp. 122002
    • Sanglard, V.1
  • 8
    • 21144443074 scopus 로고    scopus 로고
    • APHYEE 0927-6505 10.1016/j.astropartphys.2005.02.004
    • G.J. Alner (UK Dark Matter Collaboration), Astropart. Phys. 23, 444 (2005). APHYEE 0927-6505 10.1016/j.astropartphys.2005.02.004
    • (2005) Astropart. Phys. , vol.23 , pp. 444
    • Alner, G.J.1
  • 9
    • 29744467923 scopus 로고    scopus 로고
    • astro-ph/0507190.
    • D.S. Akerib (CDMS Collaboration) astro-ph/0507190.
    • Akerib, D.S.1
  • 10
    • 0000864212 scopus 로고
    • ASJOAB 0004-637X 10.1086/168638
    • P.J.T. Leonard and S. Tremaine, Astrophys. J. 353, 486 (1990). ASJOAB 0004-637X 10.1086/168638
    • (1990) Astrophys. J. , vol.353 , pp. 486
    • Leonard, P.J.T.1    Tremaine, S.2
  • 12
    • 0037105272 scopus 로고    scopus 로고
    • PRVDAQ 0556-2821 10.1103/PhysRevD.66.063502
    • The class of models discussed in Ref. represents a quite exhaustive summary of dark matter distribution functions as possible departures from the isothermal sphere model. Notice, however, that it does not include the possibility of nonthermal components in the f(v→), which could in principle modify the high-velocity tail of the velocity DF (see, for instance: A. Helmi, S.D.M. White, V. Springel, Phys. Rev. D 66, 063502 (2002)). PRVDAQ 0556-2821 10.1103/PhysRevD.66.063502
    • (2002) Phys. Rev. D , vol.66 , pp. 063502
    • Helmi, A.1    White, S.D.M.2    Springel, V.3
  • 13
    • 0041336762 scopus 로고    scopus 로고
    • PRVDAQ 0556-2821 10.1103/PhysRevD.68.023004
    • For other analyses, see for instance: A.M. Green, Phys. Rev. D 68, 023004 (2003); PRVDAQ 0556-2821 10.1103/PhysRevD.68.023004
    • (2003) Phys. Rev. D , vol.68 , pp. 023004
    • Green, A.M.1
  • 14
    • 85039601939 scopus 로고    scopus 로고
    • PRVDAQ 0556-2821 10.1103/PhysRevD.69.109902
    • A.M. Green Phys. Rev. D 69, 109902(E) (2004); PRVDAQ 0556-2821 10.1103/PhysRevD.69.109902
    • (2004) Phys. Rev. D , vol.69
    • Green, A.M.1
  • 15
    • 4544362478 scopus 로고    scopus 로고
    • PRVDAQ 0556-2821 10.1103/PhysRevD.66.083003
    • A.M. Green, Phys. Rev. D 66, 083003 (2002); PRVDAQ 0556-2821 10.1103/PhysRevD.66.083003
    • (2002) Phys. Rev. D , vol.66 , pp. 083003
    • Green, A.M.1
  • 16
    • 0035084150 scopus 로고    scopus 로고
    • PRVDAQ 0556-2821 10.1103/PhysRevD.63.043005
    • A.M. Green, Phys. Rev. D 63, 043005 (2001); PRVDAQ 0556-2821 10.1103/PhysRevD.63.043005
    • (2001) Phys. Rev. D , vol.63 , pp. 043005
    • Green, A.M.1
  • 17
    • 0001351047 scopus 로고    scopus 로고
    • PRVDAQ 0556-2821 10.1103/PhysRevD.57.3256
    • M. Kamionkowski and A. Kinkhabwala, Phys. Rev. D 57, 3256 (1998); PRVDAQ 0556-2821 10.1103/PhysRevD.57.3256
    • (1998) Phys. Rev. D , vol.57 , pp. 3256
    • Kamionkowski, M.1    Kinkhabwala, A.2
  • 18
    • 4243296504 scopus 로고    scopus 로고
    • PRLTAO 0031-9007 10.1103/PhysRevLett.83.3597
    • J.D. Vergados, Phys. Rev. Lett. 83, 3597 (1999); PRLTAO 0031-9007 10.1103/PhysRevLett.83.3597
    • (1999) Phys. Rev. Lett. , vol.83 , pp. 3597
    • Vergados, J.D.1
  • 19
    • 0042641403 scopus 로고    scopus 로고
    • ASJOAB 0004-637X 10.1086/368350
    • J.D. Vergados and D. Owen, Astrophys. J. ASJOAB 0004-637X 589, 17 (2003); 10.1086/368350
    • (2003) Astrophys. J. , vol.589 , pp. 17
    • Vergados, J.D.1    Owen, D.2
  • 20
    • 33744943560 scopus 로고    scopus 로고
    • JHEPFG 1029-8479 10.1088/1126-6708/2001/03/049
    • P. Ullio and M. Kamionkowski, J. High Energy Phys. JHEPFG 1029-8479 03 (2001) 049; 10.1088/1126-6708/2001/03/049
    • J. High Energy Phys. , vol.2001 , Issue.3 , pp. 049
    • Ullio, P.1    Kamionkowski, M.2
  • 22
    • 0035073064 scopus 로고    scopus 로고
    • PRVDAQ 0556-2821 10.1103/PhysRevD.63.036006
    • G. Gelmini and P. Gondolo, Phys. Rev. D 63, 036006 (2001). PRVDAQ 0556-2821 10.1103/PhysRevD.63.036006
    • (2001) Phys. Rev. D , vol.63 , pp. 036006
    • Gelmini, G.1    Gondolo, P.2
  • 27
  • 29
    • 0000991345 scopus 로고
    • ASJOAB 0004-637X
    • D. Merrit, Astrophys. J. 90, 1027 (1985). ASJOAB 0004-637X
    • (1985) Astrophys. J. , vol.90 , pp. 1027
    • Merrit, D.1
  • 30
    • 21844509111 scopus 로고    scopus 로고
    • ASJOAB 0004-637X 10.1086/176724
    • C.S. Kochanek, Astrophys. J. 457, 228 (1996). ASJOAB 0004-637X 10.1086/176724
    • (1996) Astrophys. J. , vol.457 , pp. 228
    • Kochanek, C.S.1
  • 32
    • 0032185831 scopus 로고    scopus 로고
    • APHYEE 0927-6505 10.1016/S0927-6505(98)00025-5
    • F. Donato, N. Fornengo, and S. Scopel, Astropart. Phys. 9, 247 (1998). APHYEE 0927-6505 10.1016/S0927-6505(98)00025-5
    • (1998) Astropart. Phys. , vol.9 , pp. 247
    • Donato, F.1    Fornengo, N.2    Scopel, S.3
  • 33
    • 0036695356 scopus 로고    scopus 로고
    • PRVDAQ 0556-2821 10.1103/PhysRevD.66.032005
    • S. Yellin, Phys. Rev. D 66, 032005 (2002). PRVDAQ 0556-2821 10.1103/PhysRevD.66.032005
    • (2002) Phys. Rev. D , vol.66 , pp. 032005
    • Yellin, S.1
  • 38
    • 0141564910 scopus 로고    scopus 로고
    • PRVDAQ 0556-2821 10.1103/PhysRevD.68.035005
    • U. Chattopadhyay, A. Corsetti, and P. Nath, Phys. Rev. D 68, 035005 (2003); PRVDAQ 0556-2821 10.1103/PhysRevD.68.035005
    • (2003) Phys. Rev. D , vol.68 , pp. 035005
    • Chattopadhyay, U.1    Corsetti, A.2    Nath, P.3
  • 39
    • 0034621789 scopus 로고    scopus 로고
    • PYLBAJ 0370-2693 10.1016/S0370-2693(00)00512-8
    • J.L. Feng, K.T. Matchev, and F. Wilczek, Phys. Lett. B 482, 388 (2000); PYLBAJ 0370-2693 10.1016/S0370-2693(00)00512-8
    • (2000) Phys. Lett. B , vol.482 , pp. 388
    • Feng, J.L.1    Matchev, K.T.2    Wilczek, F.3
  • 40
    • 0030269221 scopus 로고    scopus 로고
    • APHYEE 0927-6505 10.1016/0927-6505(96)00027-8
    • L. Bergstrom and P. Gondolo, Astropart. Phys. 5, 263 (1996); APHYEE 0927-6505 10.1016/0927-6505(96)00027-8
    • (1996) Astropart. Phys. , vol.5 , pp. 263
    • Bergstrom, L.1    Gondolo, P.2
  • 43
    • 29744461052 scopus 로고    scopus 로고
    • RNUCAC 0035-5917
    • R. Bernabei (DAMA Collaboration), Riv. Nuovo Cimento RNUCAC 0035-5917 26N1, 1 (2003).
    • (2003) Riv. Nuovo Cimento , vol.261 , pp. 1
    • Bernabei, R.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.