메뉴 건너뛰기




Volumn 753, Issue 1-2, 2006, Pages 178-194

Minimal dark matter

Author keywords

[No Author keywords available]

Indexed keywords


EID: 33747797977     PISSN: 05503213     EISSN: None     Source Type: Journal    
DOI: 10.1016/j.nuclphysb.2006.07.012     Document Type: Article
Times cited : (1169)

References (76)
  • 1
    • 0030103124 scopus 로고    scopus 로고
    • For a recent review about supersymmetric DM see
    • For a recent review about supersymmetric DM see. Jungman G., Kamionkowski M., and Griest K. Phys. Rep. 267 (1996) 195
    • (1996) Phys. Rep. , vol.267 , pp. 195
    • Jungman, G.1    Kamionkowski, M.2    Griest, K.3
  • 2
    • 0033553730 scopus 로고    scopus 로고
    • The fine-tuning argument was invented to motivate new physics at the weak scale. The other side of the coin was addressed, after LEP2 negative searches, in. hep-ph/9811386
    • The fine-tuning argument was invented to motivate new physics at the weak scale. The other side of the coin was addressed, after LEP2 negative searches, in. Giusti L., Romanino A., and Strumia A. Nucl. Phys. B 550 (1999) 3. hep-ph/9811386
    • (1999) Nucl. Phys. B , vol.550 , pp. 3
    • Giusti, L.1    Romanino, A.2    Strumia, A.3
  • 4
    • 0000408260 scopus 로고
    • Strongly interacting, "hadronized", dark matter is subject to a number of constraints analysed in that leave only implausible windows open. The particular case of DM as a thermal relic seems fully excluded by direct detection experiments and heavy isotopes searches
    • Strongly interacting, "hadronized", dark matter is subject to a number of constraints analysed in. Starkman G.D., Gould A., Esmailzadeh R., and Dimopoulos S. Phys. Rev. D 41 (1990) 3594 that leave only implausible windows open. The particular case of DM as a thermal relic seems fully excluded by direct detection experiments and heavy isotopes searches
    • (1990) Phys. Rev. D , vol.41 , pp. 3594
    • Starkman, G.D.1    Gould, A.2    Esmailzadeh, R.3    Dimopoulos, S.4
  • 14
    • 33747794388 scopus 로고    scopus 로고
    • See also. hep-ph/0510036
    • See also. Vereshkov G.M., et al. hep-ph/0510036
    • Vereshkov, G.M.1
  • 20
    • 33747801779 scopus 로고    scopus 로고
    • C.A. Coulomb, Première Mémoire sur l'Électricitité et Magnétisme, Histoire de l'Académie Royale des Sciences, 1785, p. 569
  • 25
    • 33747764908 scopus 로고    scopus 로고
    • WMAP Science Team. astro-ph/0603449
    • Spergel D.N., et al. WMAP Science Team. astro-ph/0603449
    • Spergel, D.N.1
  • 27
    • 33747750609 scopus 로고    scopus 로고
    • CDMS Collaboration. astro-ph/0509259
    • CDMS Collaboration. astro-ph/0509259
  • 28
    • 18444417830 scopus 로고    scopus 로고
    • For the Xenon project see. astro-ph/0407575
    • For the Xenon project see. Aprile E., et al. Nucl. Phys. B (Proc. Suppl.) 138 (2005) 156. astro-ph/0407575
    • (2005) Nucl. Phys. B (Proc. Suppl.) , vol.138 , pp. 156
    • Aprile, E.1
  • 29
    • 33747760440 scopus 로고    scopus 로고
    • For the SuperCDMS project see. CDMS-II Collaboration. astro-ph/0503583
    • For the SuperCDMS project see. CDMS-II Collaboration. eConf C041213 (2004) 2529. astro-ph/0503583
    • (2004) eConf , vol.C041213 , pp. 2529
  • 30
    • 33747807983 scopus 로고    scopus 로고
    • Useful comparisons can be done using the tools in
    • Useful comparisons can be done using the tools in. http://dendera.berkeley.edu/plotter/entryform.html
  • 36
    • 1642397632 scopus 로고    scopus 로고
    • DAMA Collaboration. astro-ph/0307403
    • Bernabei R., et al., DAMA Collaboration. Riv. Nuovo Cimento 26 1 (2003) 1-73. astro-ph/0307403
    • (2003) Riv. Nuovo Cimento , vol.26 , Issue.1 , pp. 1-73
    • Bernabei, R.1
  • 37
    • 33747748508 scopus 로고    scopus 로고
    • For scans in different SUSY models, see for instance:. hep-ph/0505019
    • For scans in different SUSY models, see for instance:. Baek S., Cerdeno D.G., Kim Y.G., Ko P., and Munoz C. JHEP 0506 (2005) 017. hep-ph/0505019
    • (2005) JHEP , vol.506 , pp. 017
    • Baek, S.1    Cerdeno, D.G.2    Kim, Y.G.3    Ko, P.4    Munoz, C.5
  • 58
    • 3543008133 scopus 로고    scopus 로고
    • AMANDA Collaboration
    • Ahrens J., et al., AMANDA Collaboration. Phys. Rev. D 66 (2002) 032006
    • (2002) Phys. Rev. D , vol.66 , pp. 032006
    • Ahrens, J.1
  • 60
    • 4243290644 scopus 로고    scopus 로고
    • hep-ph/0205116
    • Crotty P.R. Phys. Rev. D 66 (2002) 063504. hep-ph/0205116
    • (2002) Phys. Rev. D , vol.66 , pp. 063504
    • Crotty, P.R.1
  • 61
    • 26444612160 scopus 로고    scopus 로고
    • hep-ph/0506298
    • Cirelli M., et al. Nucl. Phys. B 727 (2005) 99. hep-ph/0506298
    • (2005) Nucl. Phys. B , vol.727 , pp. 99
    • Cirelli, M.1
  • 63
    • 33747760441 scopus 로고    scopus 로고
    • See:
    • See:. http://wizard.roma2.infn.it/pamela
  • 64
    • 33747799355 scopus 로고    scopus 로고
    • See:
    • See:. http://ams.cern.ch/AMS
  • 70
    • 33747792103 scopus 로고    scopus 로고
    • T.C. Weekes, et al., in: Proceedings of the 25th ICRC, vol. 5, 1997, p. 173
  • 73
    • 0036373744 scopus 로고    scopus 로고
    • For discussions about realistic LHC upgrades see. Atlas Collaboration
    • For discussions about realistic LHC upgrades see. Azuelos G., et al., Atlas Collaboration. J. Phys. G 28 (2002) 2453
    • (2002) J. Phys. G , vol.28 , pp. 2453
    • Azuelos, G.1
  • 74
    • 33747780106 scopus 로고    scopus 로고
    • talk at the 2003 International Workshop on Future Hadron Colliders, web site
    • de Roeck A. talk at the 2003 International Workshop on Future Hadron Colliders, web site. http://conferences.fnal.gov/hadroncollider
    • de Roeck, A.1
  • 75
    • 33747751322 scopus 로고    scopus 로고
    • talk at the 2005 Les Houches Workshop, web site
    • Denegri D. talk at the 2005 Les Houches Workshop, web site. http://lappweb.in2p3.fr/conferences/LesHouches
    • Denegri, D.1
  • 76
    • 33747792777 scopus 로고    scopus 로고
    • For a recent review of chiral perturbation theory see. hep-ph/0101264
    • For a recent review of chiral perturbation theory see. Colangelo G., and Isidori G. hep-ph/0101264
    • Colangelo, G.1    Isidori, G.2


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.