PL EN


Preferencje help
Widoczny [Schowaj] Abstrakt
Liczba wyników
Czasopismo
2011 | 9 | 3 | 628-643
Tytuł artykułu

WIMP event rates in directional experiments: The diurnal variation signature

Treść / Zawartość
Warianty tytułu
Języki publikacji
EN
Abstrakty
EN
The recent WMAP data have confirmed that exotic dark matter together with the vacuum energy (cosmological constant) dominate in the flat Universe. Modern particle theories provide viable cold dark matter candidates with masses in the GeV-TeV region. All such candidates will be called WIMPs (Weakly Interacting Massive Particles). The nature of dark matter can only be unraveled by its direct detection in the laboratory. In this work we present some theoretical elements relevant to the direct dark matter detection experiments, paying particular attention to directional experiments, i.e. experiments in which not only the energy but the direction of the recoiling nucleus is observed. Since the direction of observation is fixed with respect to the Earth, while the Earth is rotating around its axis, in a directional experiment the angle between the direction of observation and the Sun’s direction of motion will change during the day. So, since the event rates sensitively depend on this angle, the observed signal in such experiments will exhibit very interesting and characteristic periodic diurnal variation.
Słowa kluczowe
Wydawca

Czasopismo
Rocznik
Tom
9
Numer
3
Strony
628-643
Opis fizyczny
Daty
wydano
2011-06-01
online
2011-02-26
Twórcy
  • Theoretical Physics Division, University of Ioannina, Ioannina, Gr 451 10, Greece, vergados@uoi.gr
  • Department of Theoretical Physics, Aristotle University of Thessaloniki, 54124, Thessaloniki, Greece, moustaki@auth.gr
Bibliografia
  • [1] S. Hanary et al., Astrophys. J. 545, L5 (2000) http://dx.doi.org/10.1086/317322[Crossref]
  • [2] J.H.P. Wu et al., Phys. Rev. Lett. 87, 251303 (2001) http://dx.doi.org/10.1103/PhysRevLett.87.251303[Crossref]
  • [3] M.G. Santos et al., Phys. Rev. Lett. 88, 241302 (2002) http://dx.doi.org/10.1103/PhysRevLett.88.241302[Crossref]
  • [4] P.D. Mauskopf et al., Astrophys. J. 536, L59 (2002) http://dx.doi.org/10.1086/312743[Crossref]
  • [5] S. Mosi et al., Prog. Part. Nucl. Phys. 48, 243 (2002) http://dx.doi.org/10.1016/S0146-6410(02)00131-X[Crossref]
  • [6] S.B. Ruhl et al., arXiv:astro-ph/0212229 and references therein
  • [7] N.W. Halverson et al., Astrophys. J. 568, 38 (2002) http://dx.doi.org/10.1086/338879[Crossref]
  • [8] L.S. Sievers et al., arXiv:astro-ph/0205287 and references therein
  • [9] G.F. Smoot et al. (COBE Collaboration), Astrophys. J. 396, L1 (1992) http://dx.doi.org/10.1086/186504[Crossref]
  • [10] A.H. Jaffe et al., Phys. Rev. Lett. 86, 3475 (2001) http://dx.doi.org/10.1103/PhysRevLett.86.3475[Crossref]
  • [11] D.N. Spergel et al., Astrophys. J. Suppl. S. 148, 175 (2003) http://dx.doi.org/10.1086/377226[Crossref]
  • [12] D. Spergel et al., Astrophys. J. Suppl. S. 170, 377 (2007) http://dx.doi.org/10.1086/513700[Crossref]
  • [13] D.P. Bennett et al., Phys. Rev. Lett. 74, 2867 (1995) http://dx.doi.org/10.1103/PhysRevLett.74.2867[Crossref]
  • [14] P. Ullio, M. Kamioknowski, J. High Energy Phys. 0103, 049 (2001) http://dx.doi.org/10.1088/1126-6708/2001/03/049[Crossref]
  • [15] A. Bottino et al., Phys. Lett B 402, 113 (1997) http://dx.doi.org/10.1016/S0370-2693(97)00390-0[Crossref]
  • [16] R. Arnowitt, P. Nath, Phys. Rev. Lett. 74, 4592 (1995) http://dx.doi.org/10.1103/PhysRevLett.74.4592[Crossref]
  • [17] R. Arnowitt, P. Nath, Phys. Rev. D 54, 2374 (1996) http://dx.doi.org/10.1103/PhysRevD.54.2374[Crossref]
  • [18] V.A. Bednyakov, H.V. Klapdor-Kleingrothaus, S.G. Kovalenko, Phys. Lett. B 329, 5 (1994) http://dx.doi.org/10.1016/0370-2693(94)90509-6[Crossref]
  • [19] J. Ellis, L. Roszkowski, Phys. Lett. B 283, 252 (1992) http://dx.doi.org/10.1016/0370-2693(92)90016-W[Crossref]
  • [20] M.E. Gómez, J.D. Vergados, Phys. Lett. B 512, 252 (2001) http://dx.doi.org/10.1016/S0370-2693(01)00726-2[Crossref]
  • [21] M.E. Gómez, G. Lazarides, C. Pallis, Phys. Rev. D 61, 123512 (2000) http://dx.doi.org/10.1103/PhysRevD.61.123512[Crossref]
  • [22] M.E. Gómez, G. Lazarides, C. Pallis, Phys. Lett. B 487, 313 (2000) http://dx.doi.org/10.1016/S0370-2693(00)00841-8[Crossref]
  • [23] J. Ellis, R.A. Flores, Phys. Lett. B 263, 259 (1991) http://dx.doi.org/10.1016/0370-2693(91)90597-J[Crossref]
  • [24] J. Ellis, R.A. Flores, Phys. Lett. B 300, 175 (1993) http://dx.doi.org/10.1016/0370-2693(93)90767-C[Crossref]
  • [25] J. Ellis, R.A. Flores, Nucl. Phys. B 400, 25 (1993) http://dx.doi.org/10.1016/0550-3213(93)90396-7[Crossref]
  • [26] J.D. Vergados, J. Phys. G Nucl. Partic. 22, 253 (1996) http://dx.doi.org/10.1088/0954-3899/22/2/010[Crossref]
  • [27] J.D. Vergados, Lect. Notes Phys. 720, 69 (2007) http://dx.doi.org/10.1007/978-3-540-71013-4_3[Crossref]
  • [28] A. Djouadi, M.K. Drees, Phys. Lett. B 484, 183 (2000) http://dx.doi.org/10.1016/S0370-2693(00)00661-4[Crossref]
  • [29] S. Dawson, Nucl. Phys. B 359, 283 (1991) http://dx.doi.org/10.1016/0550-3213(91)90061-2[Crossref]
  • [30] M. Spira et al., Nucl. Phys. B 453, 17 (1995) http://dx.doi.org/10.1016/0550-3213(95)00379-7[Crossref]
  • [31] M. Drees, M.M. Nojiri, Phys. Rev. D 48, 3843 (1993) http://dx.doi.org/10.1103/PhysRevD.48.3483[Crossref]
  • [32] M. Drees, M.M. Nojiri, Phys. Rev. D 47, 4226 (1993) http://dx.doi.org/10.1103/PhysRevD.47.4226[Crossref]
  • [33] T.P. Cheng, Phys. Rev. D 38, 2869 (1988) http://dx.doi.org/10.1103/PhysRevD.38.2869[Crossref]
  • [34] H-Y. Cheng, Phys. Lett. B 219, 347 (1989) http://dx.doi.org/10.1016/0370-2693(89)90402-4[Crossref]
  • [35] M.T. Ressell et al., Phys. Rev. D 48, 5519 (1993) http://dx.doi.org/10.1103/PhysRevD.48.5519[Crossref]
  • [36] M.T. Ressell, D.J. Dean, Phys. Rev. C 56, 535 (1997) http://dx.doi.org/10.1103/PhysRevC.56.535[Crossref]
  • [37] P.C. Divari, T.S. Kosmas, J.D. Vergados, L.D. Skouras, Phys. Rev. C 61, 054612 (2000) http://dx.doi.org/10.1103/PhysRevC.61.054612[Crossref]
  • [38] M.W. Goodman, E. Witten, Phys. Rev. D 31, 3059 (1985) http://dx.doi.org/10.1103/PhysRevD.31.3059[Crossref]
  • [39] A. Drukier, A. Freeze, D. Spergel, Phys. Rev. D 33, 3495 (1986) http://dx.doi.org/10.1103/PhysRevD.33.3495[Crossref]
  • [40] D. Spergel, Phys. Rev. D 37, 1353 (1988) http://dx.doi.org/10.1103/PhysRevD.37.1353[Crossref]
  • [41] J.D. Vergados, P. Quentin, D. Strottman, Int. J. Mod. Phys. E 14, 751 (2005) http://dx.doi.org/10.1142/S0218301305003508[Crossref]
  • [42] J.D. Vergados, H. Ejiri, Phys. Lett. B 606, 305 (2005)
  • [43] C.C. Moustakidis, J.D. Vergados, H. Ejiri, Nucl. Phys. B 727, 406 (2005) http://dx.doi.org/10.1016/j.nuclphysb.2005.08.033[Crossref]
  • [44] C.C. Moustakidis, J.D. Vergados, H. Ejiri, Nucl. Phys. B 727, 406 (2005) http://dx.doi.org/10.1016/j.nuclphysb.2005.08.033[Crossref]
  • [45] B. Ahmed et al., Astropart. Phys. 19, 691 (2003) http://dx.doi.org/10.1016/S0927-6505(03)00115-4[Crossref]
  • [46] Y. Shimizu, M. Minoa, Y. Inoue, Nucl. Instrum. Meth. A 496, 347 (2003) http://dx.doi.org/10.1016/S0168-9002(02)01661-3[Crossref]
  • [47] V.A. Kudryavtsev, arXiv:astro-ph/0406126
  • [48] B. Morgan, A.M. Green, N.J.C. Spooner, Phys. Rev. D 71, 103507 (2005) http://dx.doi.org/10.1103/PhysRevD.71.103507[Crossref]
  • [49] B. Morgan, A.M. Green, Phys. Rev. D 72, 123501 (2005) http://dx.doi.org/10.1103/PhysRevD.72.123501[Crossref]
  • [50] A.M. Green, B. Morgan, Astropart. Phys. 27, 142 (2007) http://dx.doi.org/10.1016/j.astropartphys.2006.10.006[Crossref]
  • [51] C. Copi, J. Heo, L. Krauss, Phys. Lett. B 461, 43 (1999) http://dx.doi.org/10.1016/S0370-2693(99)00830-8[Crossref]
  • [52] C. Copi, L. Krauss, Phys. Rev. D 63, 043507 (2001) http://dx.doi.org/10.1103/PhysRevD.63.043507[Crossref]
  • [53] M.S. Alenazi, P. Gondolo, Phys. Rev. D 77, 043532 (2008) http://dx.doi.org/10.1103/PhysRevD.77.043532[Crossref]
  • [54] R.J. Creswick, S. Nussinov, F.T. Avignone III, arXiv:1007.0214[astro-ph.IM]
  • [55] M. Lisanti, J.G. Wacker, arXiv:0911.1997[hep-ph]
  • [56] J.D. Vergados, Phys. Rev. D 57, 103003 (2003) http://dx.doi.org/10.1103/PhysRevD.67.103003[Crossref]
  • [57] J.D. Vergados, J. Phys. G Nucl. Partic. 30, 1127 (2004) http://dx.doi.org/10.1088/0954-3899/30/9/012[Crossref]
  • [58] J.D. Vergados, A. Faessler, Phys. Rev. D 75, 055007 (2007) http://dx.doi.org/10.1103/PhysRevD.75.055007[Crossref]
  • [59] P. Sikivie, Phys. Rev. D 60, 063501 (1999) http://dx.doi.org/10.1103/PhysRevD.60.063501[Crossref]
  • [60] P. Sikivie, Phys. Lett. B 432, 139 (1998) http://dx.doi.org/10.1016/S0370-2693(98)00595-4[Crossref]
  • [61] J.D. Vergados, Phys. Rev. D 63, 06351 (2001) http://dx.doi.org/10.1103/PhysRevD.63.063511[Crossref]
  • [62] A.M. Green, Phys. Rev. D 63, 103003 (2001) http://dx.doi.org/10.1103/PhysRevD.63.103003[Crossref]
  • [63] G. Gelmini, P. Gondolo, Phys. Rev. D 64, 123504 (2001) http://dx.doi.org/10.1103/PhysRevD.64.023504[Crossref]
  • [64] A.M. Green, Phys. Rev. D 66, 083003 (2002) http://dx.doi.org/10.1103/PhysRevD.66.083003[Crossref]
  • [65] S. Ahlen et al., Int. J. Mod. Phys. A 25, 1 (2010) http://dx.doi.org/10.1142/S0217751X10048172[Crossref]
  • [66] C.J. Copi, L.M. Krauss, D. Simmons-Duffin, S.R. Stroiney, Phys. Rev. D 75, 023514 (2007) http://dx.doi.org/10.1103/PhysRevD.75.023514[Crossref]
  • [67] J.D. Vergados, D. Owen, Phys. Rev. D 75, 043503 (2007) http://dx.doi.org/10.1103/PhysRevD.75.043503[Crossref]
  • [68] J.D. Vergados, Astron. J. 137, 10 (2009)
  • [69] N. Tetradis, J.D. Vergados, A. Faessler, Phys. Rev. D 75, 023504 (2007) http://dx.doi.org/10.1103/PhysRevD.75.023504[Crossref]
  • [70] J.D. Vergados, S.H. Hansen, O. Host, Phys. Rev. D 77, 023509 (2008) http://dx.doi.org/10.1103/PhysRevD.77.023509[Crossref]
  • [71] R. Bernabei et al., Phys. Lett. B 424, 195 (1998) http://dx.doi.org/10.1016/S0370-2693(98)00172-5[Crossref]
  • [72] R. Bernabei et al., Phys. Lett. B 389, 757 (1996) http://dx.doi.org/10.1016/S0370-2693(96)01483-9[Crossref]
  • [73] J. Angle et al., Phys. Rev. Lett. 100, 021303 (2008) http://dx.doi.org/10.1103/PhysRevLett.100.021303[Crossref]
  • [74] D.S. Akerib et al. (CDMS Collaboration), Phys. Rev. Lett. 93, 211301 (2004) http://dx.doi.org/10.1103/PhysRevLett.93.211301[Crossref]
Typ dokumentu
Bibliografia
Identyfikatory
Identyfikator YADDA
bwmeta1.element.-psjd-doi-10_2478_s11534-010-0075-z
JavaScript jest wyłączony w Twojej przeglądarce internetowej. Włącz go, a następnie odśwież stronę, aby móc w pełni z niej korzystać.