메뉴 건너뛰기




Volumn 75, Issue 11, 2007, Pages

U-boson production in e+e- annihilations, ψ and Υ decays, and light dark matter

Author keywords

[No Author keywords available]

Indexed keywords


EID: 34347390224     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.75.115017     Document Type: Article
Times cited : (460)

References (78)
  • 1
    • 13544268515 scopus 로고
    • PYLBAJ 0370-2693 10.1016/0370-2693(80)90488-8
    • P. Fayet, Phys. Lett. B 95, 285 (1980); PYLBAJ 0370-2693 10.1016/0370-2693(80)90488-8
    • (1980) Phys. Lett. B , vol.95 , pp. 285
    • Fayet, P.1
  • 2
    • 0347925113 scopus 로고
    • NUPBBO 0550-3213 10.1016/0550-3213(81)90122-X
    • P. Fayet Nucl. Phys. NUPBBO 0550-3213 B187, 184 (1981). 10.1016/0550-3213(81)90122-X
    • (1981) Nucl. Phys. , vol.187 , pp. 184
    • Fayet, P.1
  • 3
    • 0001456347 scopus 로고
    • PYLBAJ 0370-2693 10.1016/0370-2693(76)90319-1
    • P. Fayet, Phys. Lett. B 64, 159 (1976); PYLBAJ 0370-2693 10.1016/0370-2693(76)90319-1
    • (1976) Phys. Lett. B , vol.64 , pp. 159
    • Fayet, P.1
  • 4
    • 24444437248 scopus 로고
    • PYLBAJ 0370-2693 10.1016/0370-2693(77)90852-8
    • P. Fayet Phys. Lett. B 69, 489 (1977). PYLBAJ 0370-2693 10.1016/0370-2693(77)90852-8
    • (1977) Phys. Lett. B , vol.69 , pp. 489
    • Fayet, P.1
  • 5
    • 0000182532 scopus 로고
    • NUPBBO 0550-3213 10.1016/0550-3213(75)90636-7
    • P. Fayet, Nucl. Phys. NUPBBO 0550-3213 B90, 104 (1975). 10.1016/0550-3213(75)90636-7
    • (1975) Nucl. Phys. , vol.90 , pp. 104
    • Fayet, P.1
  • 6
    • 4244077868 scopus 로고
    • PYLBAJ 0370-2693 10.1016/0370-2693(77)90414-2
    • P. Fayet, Phys. Lett. B 70, 461 (1977); PYLBAJ 0370-2693 10.1016/0370-2693(77)90414-2
    • (1977) Phys. Lett. B , vol.70 , pp. 461
    • Fayet, P.1
  • 7
    • 23544432701 scopus 로고
    • PYLBAJ 0370-2693 10.1016/0370-2693(79)90836-0
    • P. Fayet Phys. Lett. B 86, 272 (1979); PYLBAJ 0370-2693 10.1016/0370-2693(79)90836-0
    • (1979) Phys. Lett. B , vol.86 , pp. 272
    • Fayet, P.1
  • 8
    • 0011038269 scopus 로고
    • PYLBAJ 0370-2693 10.1016/0370-2693(86)90626-X
    • P. Fayet Phys. Lett. B 175, 471 (1986). PYLBAJ 0370-2693 10.1016/0370-2693(86)90626-X
    • (1986) Phys. Lett. B , vol.175 , pp. 471
    • Fayet, P.1
  • 9
    • 1542342232 scopus 로고
    • PYLBAJ 0370-2693 10.1016/0370-2693(81)90596-7
    • P. Fayet and M. Mézard, Phys. Lett. B 104, 226 (1981). PYLBAJ 0370-2693 10.1016/0370-2693(81)90596-7
    • (1981) Phys. Lett. B , vol.104 , pp. 226
    • Fayet, P.1    Mézard, M.2
  • 10
    • 13244254757 scopus 로고
    • PYLBAJ 0370-2693 10.1016/0370-2693(80)90217-8
    • P. Fayet, Phys. Lett. B 96, 83 (1980). PYLBAJ 0370-2693 10.1016/0370-2693(80)90217-8
    • (1980) Phys. Lett. B , vol.96 , pp. 83
    • Fayet, P.1
  • 11
    • 1542469732 scopus 로고
    • PYLBAJ 0370-2693 10.1016/0370-2693(83)90076-X
    • C. Bouchiat and C.A. Piketty, Phys. Lett. B 128, 73 (1983). PYLBAJ 0370-2693 10.1016/0370-2693(83)90076-X
    • (1983) Phys. Lett. B , vol.128 , pp. 73
    • Bouchiat, C.1    Piketty, C.A.2
  • 12
    • 13244275429 scopus 로고    scopus 로고
    • PYLBAJ 0370-2693 10.1016/j.physletb.2004.12.065
    • C. Bouchiat and P. Fayet, Phys. Lett. B 608, 87 (2005). PYLBAJ 0370-2693 10.1016/j.physletb.2004.12.065
    • (2005) Phys. Lett. B , vol.608 , pp. 87
    • Bouchiat, C.1    Fayet, P.2
  • 13
    • 24444437035 scopus 로고
    • PYLBAJ 0370-2693 10.1016/0370-2693(86)91545-5
    • P. Fayet, Phys. Lett. B 171, 261 (1986); PYLBAJ 0370-2693 10.1016/0370-2693(86)91545-5
    • (1986) Phys. Lett. B , vol.171 , pp. 261
    • Fayet, P.1
  • 14
    • 0642385801 scopus 로고
    • PYLBAJ 0370-2693 10.1016/0370-2693(86)90271-6
    • P. Fayet Phys. Lett. B 172, 363 (1986); PYLBAJ 0370-2693 10.1016/0370-2693(86)90271-6
    • (1986) Phys. Lett. B , vol.172 , pp. 363
    • Fayet, P.1
  • 15
    • 0346179479 scopus 로고
    • PYLBAJ 0370-2693 10.1016/0370-2693(89)91294-X
    • P. Fayet Phys. Lett. B 227, 127 (1989). PYLBAJ 0370-2693 10.1016/0370-2693(89)91294-X
    • (1989) Phys. Lett. B , vol.227 , pp. 127
    • Fayet, P.1
  • 16
    • 21444458965 scopus 로고    scopus 로고
    • CQGRDG 0264-9381 10.1088/0264-9381/13/11A/004
    • P. Fayet, Classical Quantum Gravity CQGRDG 0264-9381 13, A19 (1996); 10.1088/0264-9381/13/11A/004
    • (1996) Classical Quantum Gravity , vol.13 , pp. 19
    • Fayet, P.1
  • 17
    • 34347387270 scopus 로고    scopus 로고
    • hep-ph/0111282.
    • P. Fayet C. R. Acad. Sci. t. 2, Série IV, 1257 (2001), hep-ph/0111282.
    • (2001) C. R. Acad. Sci. , pp. 1257
    • Fayet, P.1
  • 18
    • 4043165824 scopus 로고
    • PRLTAO 0031-9007 10.1103/PhysRevLett.59.849
    • E.G. Adelberger, Phys. Rev. Lett. 59, 849 (1987); PRLTAO 0031-9007 10.1103/PhysRevLett.59.849
    • (1987) Phys. Rev. Lett. , vol.59 , pp. 849
    • Adelberger, E.G.1
  • 19
    • 0001663871 scopus 로고
    • PRVDAQ 0556-2821 10.1103/PhysRevD.42.3267
    • E.G. Adelberger Phys. Rev. D 42, 3267 (1990); PRVDAQ 0556-2821 10.1103/PhysRevD.42.3267
    • (1990) Phys. Rev. D , vol.42 , pp. 3267
    • Adelberger, E.G.1
  • 20
    • 0001134120 scopus 로고
    • PRVDAQ 0556-2821 10.1103/PhysRevD.50.3614
    • Y. Su, Phys. Rev. D 50, 3614 (1994); PRVDAQ 0556-2821 10.1103/PhysRevD.50.3614
    • (1994) Phys. Rev. D , vol.50 , pp. 3614
    • Su, Y.1
  • 21
    • 34047129044 scopus 로고    scopus 로고
    • PRLTAO 0031-9007 10.1103/PhysRevLett.98.131104
    • E.G. Adelberger, Phys. Rev. Lett. 98, 131104 (2007). PRLTAO 0031-9007 10.1103/PhysRevLett.98.131104
    • (2007) Phys. Rev. Lett. , vol.98 , pp. 131104
    • Adelberger, E.G.1
  • 22
    • 1542378355 scopus 로고    scopus 로고
    • NUPBBO 0550-3213 10.1016/j.nuclphysb.2004.01.015
    • C. Bœhm and P. Fayet, Nucl. Phys. NUPBBO 0550-3213 B683, 219 (2004). 10.1016/j.nuclphysb.2004.01.015
    • (2004) Nucl. Phys. , vol.683 , pp. 219
    • Bœhm, C.1    Fayet, P.2
  • 23
    • 42749098501 scopus 로고    scopus 로고
    • PRVDAQ 0556-2821 10.1103/PhysRevD.70.023514
    • P. Fayet, Phys. Rev. D 70, 023514 (2004); PRVDAQ 0556-2821 10.1103/PhysRevD.70.023514
    • (2004) Phys. Rev. D , vol.70 , pp. 023514
    • Fayet, P.1
  • 24
    • 34347406089 scopus 로고    scopus 로고
    • hep-ph/0408357.
    • P. Fayet hep-ph/0408357.
    • Fayet, P.1
  • 25
    • 0042933926 scopus 로고    scopus 로고
    • AAEJAF 0004-6361 10.1051/0004-6361:20031056
    • P. Jean, Astron. Astrophys. 407, L55 (2003). AAEJAF 0004-6361 10.1051/0004-6361:20031056
    • (2003) Astron. Astrophys. , vol.407 , pp. 55
    • Jean, P.1
  • 26
    • 2142827149 scopus 로고    scopus 로고
    • PRLTAO 0031-9007 10.1103/PhysRevLett.92.101301
    • C. Bœhm, Phys. Rev. Lett. 92, 101301 (2004); PRLTAO 0031-9007 10.1103/PhysRevLett.92.101301
    • (2004) Phys. Rev. Lett. , vol.92 , pp. 101301
    • Bœhm, C.1
  • 27
    • 3142562557 scopus 로고    scopus 로고
    • PRVDAQ 0556-2821 10.1103/PhysRevD.69.101302
    • C. Bœhm, P. Fayet, and J. Silk, Phys. Rev. D 69, 101302 (2004). PRVDAQ 0556-2821 10.1103/PhysRevD.69.101302
    • (2004) Phys. Rev. D , vol.69 , pp. 101302
    • Bœhm, C.1    Fayet, P.2    Silk, J.3
  • 28
    • 0003131619 scopus 로고
    • NUPBBO 0550-3213 10.1016/0550-3213(74)90113-8
    • P. Fayet, Nucl. Phys. NUPBBO 0550-3213 B78, 14 (1974). 10.1016/0550-3213(74)90113-8
    • (1974) Nucl. Phys. , vol.78 , pp. 14
    • Fayet, P.1
  • 29
    • 34347404455 scopus 로고    scopus 로고
    • This gauging was also motivated by other reasons, like, at the time, making squarks and sleptons heavy through spontaneously-generated D terms rather than using (universal) explicit dimension-2 m 2 squark and slepton mass2 terms, as already introduced in the first paper of Ref. but breaking explicitly the supersymmetry. Generating spontaneously these m 2 terms led us to gauge an extra-U(1)A symmetry acting axially (in the simplest case) on quarks and leptons. m 2 terms are now usually generated through gravity-induced breaking.
    • This gauging was also motivated by other reasons, like, at the time, making squarks and sleptons heavy through spontaneously-generated D terms rather than using (universal) explicit dimension-2 m 2 squark and slepton mass2 terms, as already introduced in the first paper of Ref. but breaking explicitly the supersymmetry. Generating spontaneously these m 2 terms led us to gauge an extra-U(1)A symmetry acting axially (in the simplest case) on quarks and leptons. m 2 terms are now usually generated through gravity-induced breaking.
  • 30
    • 34347374248 scopus 로고    scopus 로고
    • The last two terms, proportional to N2 and N3, are also forbidden by the continuous R-symmetry if it is imposed. This one gets reduced to R-parity in the presence of gravity, owing to the gravitino and gaugino mass terms, in particular. It is still possible to use R-symmetry to forbid the N3 term (corresponding to dimension-4 terms in the Lagrangian density), while allowing for gravity-induced terms of dimensions ≤3 associated with m3/2, for which R-symmetry is reduced to R-parity.
    • The last two terms, proportional to N2 and N3, are also forbidden by the continuous R-symmetry if it is imposed. This one gets reduced to R-parity in the presence of gravity, owing to the gravitino and gaugino mass terms, in particular. It is still possible to use R-symmetry to forbid the N3 term (corresponding to dimension-4 terms in the Lagrangian density), while allowing for gravity-induced terms of dimensions ≤3 associated with m3/2, for which R-symmetry is reduced to R-parity.
  • 31
    • 33750731866 scopus 로고
    • PRVDAQ 0556-2821 10.1103/PhysRevD.16.1791
    • R.D. Peccei and H.R. Quinn, Phys. Rev. D 16, 1791 (1977). PRVDAQ 0556-2821 10.1103/PhysRevD.16.1791
    • (1977) Phys. Rev. D , vol.16 , pp. 1791
    • Peccei, R.D.1    Quinn, H.R.2
  • 32
    • 33744718336 scopus 로고
    • PRLTAO 0031-9007 10.1103/PhysRevLett.40.279
    • F. Wilczek, Phys. Rev. Lett. 40, 279 (1978). PRLTAO 0031-9007 10.1103/PhysRevLett.40.279
    • (1978) Phys. Rev. Lett. , vol.40 , pp. 279
    • Wilczek, F.1
  • 33
    • 4243883666 scopus 로고
    • PRLTAO 0031-9007 10.1103/PhysRevLett.40.223
    • S. Weinberg, Phys. Rev. Lett. 40, 223 (1978). PRLTAO 0031-9007 10.1103/PhysRevLett.40.223
    • (1978) Phys. Rev. Lett. , vol.40 , pp. 223
    • Weinberg, S.1
  • 34
    • 0344771356 scopus 로고
    • PYLBAJ 0370-2693 10.1016/0370-2693(84)91195-X
    • P. Fayet, Phys. Lett. B 142, 263 (1984). PYLBAJ 0370-2693 10.1016/0370-2693(84)91195-X
    • (1984) Phys. Lett. B , vol.142 , pp. 263
    • Fayet, P.1
  • 35
    • 0002426998 scopus 로고
    • NUPBBO 0550-3213 10.1016/0550-3213(84)90116-0
    • P. Fayet, Nucl. Phys. NUPBBO 0550-3213 B246, 89 (1984). 10.1016/0550-3213(84)90116-0
    • (1984) Nucl. Phys. , vol.246 , pp. 89
    • Fayet, P.1
  • 36
    • 0346179478 scopus 로고
    • NUPBBO 0550-3213 10.1016/0550-3213(90)90381-M
    • P. Fayet, Nucl. Phys. NUPBBO 0550-3213 B347, 743 (1990). 10.1016/0550-3213(90)90381-M
    • (1990) Nucl. Phys. , vol.347 , pp. 743
    • Fayet, P.1
  • 37
    • 33749183284 scopus 로고    scopus 로고
    • PRVDAQ 0556-2821 10.1103/PhysRevD.74.054034
    • P. Fayet, Phys. Rev. D 74, 054034 (2006). PRVDAQ 0556-2821 10.1103/PhysRevD.74.054034
    • (2006) Phys. Rev. D , vol.74 , pp. 054034
    • Fayet, P.1
  • 38
    • 1642393430 scopus 로고    scopus 로고
    • JPGPED 0954-3899 10.1088/0954-3899/30/3/004
    • C. Bœhm, T.A. Ensslin, and J. Silk, J. Phys. G JPGPED 0954-3899 30, 279 (2004). 10.1088/0954-3899/30/3/004
    • (2004) J. Phys. G , vol.30 , pp. 279
    • Bœhm, C.1    Ensslin, T.A.2    Silk, J.3
  • 39
    • 34347405458 scopus 로고    scopus 로고
    • astro-ph/0609566.
    • S. Schanne, astro-ph/0609566.
    • Schanne, S.1
  • 40
    • 33744777236 scopus 로고    scopus 로고
    • MNRAA4 0035-8711 10.1111/j.1365-2966.2006.10226.x
    • Y. Ascasibar, Mon. Not. R. Astron. Soc. MNRAA4 0035-8711 368, 1695 (2006). 10.1111/j.1365-2966.2006.10226.x
    • (2006) Mon. Not. R. Astron. Soc. , vol.368 , pp. 1695
    • Ascasibar, Y.1
  • 41
    • 33744494285 scopus 로고    scopus 로고
    • PRVDAQ 0556-2821 10.1103/PhysRevD.73.103518
    • Y. Rasera, Phys. Rev. D 73, 103518 (2006). PRVDAQ 0556-2821 10.1103/PhysRevD.73.103518
    • (2006) Phys. Rev. D , vol.73 , pp. 103518
    • Rasera, Y.1
  • 42
    • 34347381470 scopus 로고    scopus 로고
    • In particular, we may have S-wave-dominated halo annihilations, with typical mχ 3 to 30 MeV, and a cross section (scaling like mχ2) which depends on the dark matter profile: (σχχ→e+e-vrel)halo (.2fbto.2pb)(mχ/(10MeV))2, as can be seen from Fig. 7 of Ref. , small compared to the cross section at freeze-out, to be provided by the P-wave term.
    • In particular, we may have S-wave-dominated halo annihilations, with typical mχ 3 to 30 MeV, and a cross section (scaling like mχ2) which depends on the dark matter profile: (σχχ→e+e-vrel)halo (.2fbto.2pb)(mχ/(10MeV))2, as can be seen from Fig. 7 of Ref., small compared to the cross section at freeze-out, to be provided by the P-wave term.
  • 43
    • 27144471047 scopus 로고    scopus 로고
    • PRLTAO 0031-9007 10.1103/PhysRevLett.94.171301
    • J.F. Beacom, N.F. Bell, and G. Bertone, Phys. Rev. Lett. 94, 171301 (2005); PRLTAO 0031-9007 10.1103/PhysRevLett.94.171301
    • (2005) Phys. Rev. Lett. , vol.94 , pp. 171301
    • Beacom, J.F.1    Bell, N.F.2    Bertone, G.3
  • 45
    • 33747699114 scopus 로고    scopus 로고
    • PRLTAO 0031-9007 10.1103/PhysRevLett.97.071102
    • J.F. Beacom and H. Yüksel, Phys. Rev. Lett. 97, 071102 (2006); PRLTAO 0031-9007 10.1103/PhysRevLett.97.071102
    • (2006) Phys. Rev. Lett. , vol.97 , pp. 071102
    • Beacom, J.F.1    Yüksel, H.2
  • 47
    • 33748764158 scopus 로고    scopus 로고
    • PRVDAQ 0556-2821 10.1103/PhysRevD.74.063514
    • P. Sizun, M. Cassé, and S. Schanne, Phys. Rev. D 74, 063514 (2006). PRVDAQ 0556-2821 10.1103/PhysRevD.74.063514
    • (2006) Phys. Rev. D , vol.74 , pp. 063514
    • Sizun, P.1    Cassé, M.2    Schanne, S.3
  • 48
    • 33744799426 scopus 로고    scopus 로고
    • PRLTAO 0031-9007 10.1103/PhysRevLett.96.211302
    • P. Fayet, D. Hooper, and G. Sigl, Phys. Rev. Lett. 96, 211302 (2006). PRLTAO 0031-9007 10.1103/PhysRevLett.96.211302
    • (2006) Phys. Rev. Lett. , vol.96 , pp. 211302
    • Fayet, P.1    Hooper, D.2    Sigl, G.3
  • 49
    • 34347405707 scopus 로고    scopus 로고
    • In the case of a LDM particle lighter than about 10 MeV, this supernovae analysis points in the direction of a small coupling fν of the U boson to neutrinos, significantly smaller than its coupling fe to electrons. This would make it even more difficult than indicated in Ref. to attempt detecting U bosons with high-energy neutrino telescopes. Indeed, having fν fe (then 310-6mU(MeV), cf. Sec. 14) would lead to relatively large neutrino-LDM interactions (as for the large LDM interactions with electrons, responsible for their annihilations into e+e-), in conflict with the results of Ref. for such light dark matter particles.
    • In the case of a LDM particle lighter than about 10 MeV, this supernovae analysis points in the direction of a small coupling fν of the U boson to neutrinos, significantly smaller than its coupling fe to electrons. This would make it even more difficult than indicated in Ref. to attempt detecting U bosons with high-energy neutrino telescopes. Indeed, having fν fe (then 310-6mU(MeV), cf. Sec. 14) would lead to relatively large neutrino-LDM interactions (as for the large LDM interactions with electrons, responsible for their annihilations into e+e-), in conflict with the results of Ref. for such light dark matter particles.
  • 51
    • 0000899404 scopus 로고
    • ZPCFD2 0170-9739 10.1007/BF01561063
    • M. Böhm and Th. Sack, Z. Phys. C 35, 119 (1987). ZPCFD2 0170-9739 10.1007/BF01561063
    • (1987) Z. Phys. C , vol.35 , pp. 119
    • Böhm, M.1    Sack, Th.2
  • 52
    • 33746043357 scopus 로고    scopus 로고
    • PRLTAO 0031-9007 10.1103/PhysRevLett.97.030801
    • B. Odom, Phys. Rev. Lett. 97, 030801 (2006); PRLTAO 0031-9007 10.1103/PhysRevLett.97.030801
    • (2006) Phys. Rev. Lett. , vol.97 , pp. 030801
    • Odom, B.1
  • 53
    • 33746050369 scopus 로고    scopus 로고
    • PRLTAO 0031-9007 10.1103/PhysRevLett.97.030802
    • G. Gabrielse, Phys. Rev. Lett. 97, 030802 (2006). PRLTAO 0031-9007 10.1103/PhysRevLett.97.030802
    • (2006) Phys. Rev. Lett. , vol.97 , pp. 030802
    • Gabrielse, G.1
  • 54
    • 32644490141 scopus 로고    scopus 로고
    • PRVDAQ 0556-2821 10.1103/PhysRevD.73.013003
    • T. Kinoshita and M. Nio, Phys. Rev. D 73, 013003 (2006). PRVDAQ 0556-2821 10.1103/PhysRevD.73.013003
    • (2006) Phys. Rev. D , vol.73 , pp. 013003
    • Kinoshita, T.1    Nio, M.2
  • 55
    • 34347395096 scopus 로고    scopus 로고
    • Up to a recent time δae was constrained to verify δae (1.24±.95)10-11, i.e., approximately, -10-11 δae 310-11. The very recent measurement of the electron anomalous magnetic moment shifted the experimental value of ae downward by 1.7σ, with an uncertainty nearly 6 times lower than in the past. We still remain, however, with the uncertainties in the best determinations of α independently of ae, so that we can now write approximately, from the comparison between measured and "calculated" magnetic moments, -210-11 δae 210-11.
    • Up to a recent time δae was constrained to verify δae (1.24±.95)10-11, i.e., approximately, -10-11 δae 310-11. The very recent measurement of the electron anomalous magnetic moment shifted the experimental value of ae downward by 1.7σ, with an uncertainty nearly 6 times lower than in the past. We still remain, however, with the uncertainties in the best determinations of α independently of ae, so that we can now write approximately, from the comparison between measured and "calculated" magnetic moments, -210-11 δae 210-11.
  • 56
    • 33744751317 scopus 로고
    • NUPBBO 0550-3213 10.1016/0550-3213(78)90051-2
    • J.P. Leveille, Nucl. Phys. NUPBBO 0550-3213 B137, 63 (1978). 10.1016/0550-3213(78)90051-2
    • (1978) Nucl. Phys. , vol.137 , pp. 63
    • Leveille, J.P.1
  • 57
    • 34347374638 scopus 로고    scopus 로고
    • Such limits could be alleviated in the presence of extra contributions to ae and aμ, as from heavy (e.g. mirror) fermions in the case of spin-0 LDM particles. Conversely, U exchanges could help making acceptable such heavy fermion contributions to g-2, if present.
    • Such limits could be alleviated in the presence of extra contributions to ae and aμ, as from heavy (e.g. mirror) fermions in the case of spin-0 LDM particles. Conversely, U exchanges could help making acceptable such heavy fermion contributions to g-2, if present.
  • 58
    • 33645580103 scopus 로고    scopus 로고
    • PRVDAQ 0556-2821 10.1103/PhysRevD.73.072003
    • G.W. Bennett, Phys. Rev. D 73, 072003 (2006). PRVDAQ 0556-2821 10.1103/PhysRevD.73.072003
    • (2006) Phys. Rev. D , vol.73 , pp. 072003
    • Bennett, G.W.1
  • 59
    • 1542362639 scopus 로고    scopus 로고
    • EPCFFB 1434-6044 10.1140/epjc/s2003-01362-6
    • M. Davier, Eur. Phys. J. C 31, 503 (2003); EPCFFB 1434-6044 10.1140/epjc/s2003-01362-6
    • (2003) Eur. Phys. J. C , vol.31 , pp. 503
    • Davier, M.1
  • 60
    • 34347399942 scopus 로고    scopus 로고
    • hep-ph/0611102.
    • K. Hagiwara, hep-ph/0611102.
    • Hagiwara, K.1
  • 61
    • 34347391029 scopus 로고    scopus 로고
    • hep-ph/0701163.
    • M. Davier, hep-ph/0701163.
    • Davier, M.1
  • 62
    • 0347664332 scopus 로고
    • PYLBAJ 0370-2693 10.1016/0370-2693(91)91477-D
    • P. Fayet and J. Kaplan, Phys. Lett. B 269, 213 (1991). PYLBAJ 0370-2693 10.1016/0370-2693(91)91477-D
    • (1991) Phys. Lett. B , vol.269 , pp. 213
    • Fayet, P.1    Kaplan, J.2
  • 63
    • 0000777878 scopus 로고
    • PRVDAQ 0556-2821 10.1103/PhysRevD.30.1433
    • D. Besson (CLEO Collaboration), Phys. Rev. D 30, 1433 (1984); PRVDAQ 0556-2821 10.1103/PhysRevD.30.1433
    • (1984) Phys. Rev. D , vol.30 , pp. 1433
    • Besson, D.1
  • 64
    • 45949131193 scopus 로고
    • PYLBAJ 0370-2693 10.1016/0370-2693(86)90501-0
    • H. Albrecht (ARGUS Collaboration), Phys. Lett. B 179, 403 (1986); PYLBAJ 0370-2693 10.1016/0370-2693(86)90501-0
    • (1986) Phys. Lett. B , vol.179 , pp. 403
    • Albrecht, H.1
  • 65
    • 33947709013 scopus 로고    scopus 로고
    • PRLTAO 0031-9007 10.1103/PhysRevLett.98.132001
    • O. Tajima (Belle Collaboration), Phys. Rev. Lett. 98, 132001 (2007); PRLTAO 0031-9007 10.1103/PhysRevLett.98.132001
    • (2007) Phys. Rev. Lett. , vol.98 , pp. 132001
    • Tajima, O.1
  • 66
    • 33846935668 scopus 로고    scopus 로고
    • PRVDAQ 0556-2821 10.1103/PhysRevD.75.031104
    • P. Rubin (CLEO Collaboration), Phys. Rev. D 75, 031104 (2007). PRVDAQ 0556-2821 10.1103/PhysRevD.75.031104
    • (2007) Phys. Rev. D , vol.75 , pp. 031104
    • Rubin, P.1
  • 67
    • 4243629209 scopus 로고
    • PRLTAO 0031-9007 10.1103/PhysRevLett.48.903
    • C. Edwards, Phys. Rev. Lett. 48, 903 (1982). PRLTAO 0031-9007 10.1103/PhysRevLett.48.903
    • (1982) Phys. Rev. Lett. , vol.48 , pp. 903
    • Edwards, C.1
  • 68
    • 0001124862 scopus 로고
    • PRVDAQ 0556-2821 10.1103/PhysRevD.26.717
    • D. Sivertz, Phys. Rev. D 26, 717 (1982); PRVDAQ 0556-2821 10.1103/PhysRevD.26.717
    • (1982) Phys. Rev. D , vol.26 , pp. 717
    • Sivertz, D.1
  • 69
    • 0346809973 scopus 로고
    • PYLBAJ 0370-2693 10.1016/0370-2693(90)90254-4
    • D. Antreasyan (Crystal Ball Collaboration), Phys. Lett. B 251, 204 (1990); PYLBAJ 0370-2693 10.1016/0370-2693(90)90254-4
    • (1990) Phys. Lett. B , vol.251 , pp. 204
    • Antreasyan, D.1
  • 70
    • 25544459269 scopus 로고
    • PRVDAQ 0556-2821 10.1103/PhysRevD.51.2053
    • R. Balest (CLEO Collaboration), Phys. Rev. D 51, 2053 (1995). PRVDAQ 0556-2821 10.1103/PhysRevD.51.2053
    • (1995) Phys. Rev. D , vol.51 , pp. 2053
    • Balest, R.1
  • 71
    • 0001872108 scopus 로고
    • PYLBAJ 0370-2693 10.1016/0370-2693(81)91172-2
    • Y. Asano, Phys. Lett. B 107, 159 (1981); PYLBAJ 0370-2693 10.1016/0370-2693(81)91172-2
    • (1981) Phys. Lett. B , vol.107 , pp. 159
    • Asano, Y.1
  • 72
    • 4243558184 scopus 로고    scopus 로고
    • PRLTAO 0031-9007 10.1103/PhysRevLett.88.041803
    • S. Adler, Phys. Rev. Lett. 88, 041803 (2002); PRLTAO 0031-9007 10.1103/PhysRevLett.88.041803
    • (2002) Phys. Rev. Lett. , vol.88 , pp. 041803
    • Adler, S.1
  • 73
    • 0037142057 scopus 로고    scopus 로고
    • PYLBAJ 0370-2693 10.1016/S0370-2693(02)01911-1
    • S. Adler Phys. Lett. B 537, 211 (2002); PYLBAJ 0370-2693 10.1016/S0370-2693(02)01911-1
    • (2002) Phys. Lett. B , vol.537 , pp. 211
    • Adler, S.1
  • 74
    • 4344627215 scopus 로고    scopus 로고
    • PRLTAO 0031-9007 10.1103/PhysRevLett.93.031801
    • V.V. Anisimovsky, Phys. Rev. Lett. 93, 031801 (2004). PRLTAO 0031-9007 10.1103/PhysRevLett.93.031801
    • (2004) Phys. Rev. Lett. , vol.93 , pp. 031801
    • Anisimovsky, V.V.1
  • 75
    • 4243600539 scopus 로고
    • PRLTAO 0031-9007 10.1103/PhysRevLett.56.2672
    • G. Mageras, Phys. Rev. Lett. 56, 2672 (1986). PRLTAO 0031-9007 10.1103/PhysRevLett.56.2672
    • (1986) Phys. Rev. Lett. , vol.56 , pp. 2672
    • Mageras, G.1
  • 76
    • 0002445694 scopus 로고
    • PRVDAQ 0556-2821 10.1103/PhysRevD.47.11
    • R.C. Allen, Phys. Rev. D 47, 11 (1993); PRVDAQ 0556-2821 10.1103/PhysRevD.47.11
    • (1993) Phys. Rev. D , vol.47 , pp. 11
    • Allen, R.C.1
  • 77
    • 0034884641 scopus 로고    scopus 로고
    • PRVDAQ 0556-2821 10.1103/PhysRevD.63.112001
    • L.B. Auerbach, Phys. Rev. D 63, 112001 (2001). PRVDAQ 0556-2821 10.1103/PhysRevD.63.112001
    • (2001) Phys. Rev. D , vol.63 , pp. 112001
    • Auerbach, L.B.1
  • 78
    • 34347403185 scopus 로고    scopus 로고
    • hep-ph/0701194.
    • D. Hooper, hep-ph/0701194.
    • Hooper, D.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.