-
1
-
-
0036630540
-
-
For recent surveys, see
-
For recent surveys, see J. Erler, P. Langacker, and T.J. Li, Phys. Rev. D 66, 015002 (2002);
-
(2002)
Phys. Rev. D
, vol.66
, pp. 015002
-
-
Erler, J.1
Langacker, P.2
Li, T.J.3
-
4
-
-
0001178413
-
-
Mod. Phys. Lett. A 11, 1247 (1996).
-
(1996)
Mod. Phys. Lett. A
, vol.11
, pp. 1247
-
-
-
5
-
-
0002175470
-
-
For a review, see, edited by G.L. Kane World Scientific, Singapore
-
For a review, see, M. Cvetič and P. Langacker, in Perspectives on Supersymmetry, edited by G.L. Kane (World Scientific, Singapore, 1998), p. 312.
-
(1998)
Perspectives on Supersymmetry
, pp. 312
-
-
Cvetič, M.1
Langacker, P.2
-
6
-
-
33847419574
-
-
For a review, see, hep-ph/0203079
-
For a review, see C.T. Hill and E.H. Simmons, hep-ph/0203079.
-
-
-
Hill, C.T.1
Simmons, E.H.2
-
8
-
-
0000119447
-
-
Cvetič, D.A. Demir, J.R. Espinosa, L.L. Everett, and P. Langacker, Phys. Rev. D 56, 2861 (1997);
-
(1997)
Phys. Rev. D
, vol.56
, pp. 2861
-
-
Cvetič1
Demir, D.A.2
Espinosa, J.R.3
Everett, L.L.4
Langacker, P.5
-
9
-
-
33847372388
-
-
58, 119905(E) (1998).
-
58, 119905(E) (1998).
-
-
-
-
11
-
-
4243722746
-
-
CDF Collaboration
-
CDF Collaboration, F. Abe et al., Phys. Rev. Lett. 79, 2192 (1997).
-
(1997)
Phys. Rev. Lett
, vol.79
, pp. 2192
-
-
Abe, F.1
-
12
-
-
2342430573
-
-
ALEPH Collaboration
-
ALEPH Collaboration, R. Barate et al., Eur. Phys. J. C 12, 183 (2000);
-
(2000)
Eur. Phys. J. C
, vol.12
, pp. 183
-
-
Barate, R.1
-
13
-
-
0037814762
-
-
DELPHI Collaboration
-
DELPHI Collaboration, P. Abreu et al., Phys. Lett. B 485, 45 (2000).
-
(2000)
Phys. Lett. B
, vol.485
, pp. 45
-
-
Abreu, P.1
-
14
-
-
0002359229
-
-
J. Erler and P. Langacker, Phys. Lett. B 456, 68 (1999), and references therein.
-
J. Erler and P. Langacker, Phys. Lett. B 456, 68 (1999), and references therein.
-
-
-
-
15
-
-
0030949460
-
-
C.S. Wood et al., Science 275, 1759 (1997);
-
(1997)
Science
, vol.275
, pp. 1759
-
-
Wood, C.S.1
-
17
-
-
33847382271
-
-
The interpretation of these results is controversial. For recent discussion, see
-
The interpretation of these results is controversial. For recent discussion, see Ref. [12].
-
, vol.12
-
-
Ref1
-
20
-
-
3543067363
-
-
NuTeV Collaboration
-
NuTeV Collaboration, G.P. Zeller et al., Phys. Rev. Lett. 88, 091802 (2002).
-
(2002)
Phys. Rev. Lett
, vol.88
, pp. 091802
-
-
Zeller, G.P.1
-
21
-
-
0000573103
-
-
R. Casalbuoni, S. De Curtis, D. Dominici, and R. Gatto, Phys. Lett. B 460, 135 (1999);
-
(1999)
Phys. Lett. B
, vol.460
, pp. 135
-
-
Casalbuoni, R.1
De Curtis, S.2
Dominici, D.3
Gatto, R.4
-
24
-
-
33847380526
-
-
For reviews, see, hep-ph/9504216;
-
For reviews, see M. Cvetič and S. Godfrey, hep-ph/9504216;
-
-
-
Cvetič, M.1
Godfrey, S.2
-
25
-
-
0000729820
-
-
A. Leike, Phys. Rep. 317, 143 (1999);
-
(1999)
Phys. Rep
, vol.317
, pp. 143
-
-
Leike, A.1
-
26
-
-
33847353243
-
-
for a recent update, see S. Godfrey, in Proceedings of the APS/DPF/DPB Summer Study on the Future of Particle Physics, Snowmass, 2001, edited by N. Graf (eConf C010630), P344 and E3065.
-
for a recent update, see S. Godfrey, in Proceedings of the APS/DPF/DPB Summer Study on the Future of Particle Physics, Snowmass, 2001, edited by N. Graf (eConf C010630), P344 and E3065.
-
-
-
-
27
-
-
0002427675
-
-
edited by P. van Nieuwenhuizen and D. Freedman North-Holland, Amsterdam
-
M. Gell-Mann, P. Ramond, and R. Slansky, in Supergravity, edited by P. van Nieuwenhuizen and D. Freedman (North-Holland, Amsterdam, 1979), p. 315;
-
(1979)
Supergravity
, pp. 315
-
-
Gell-Mann, M.1
Ramond, P.2
Slansky, R.3
-
28
-
-
33847387007
-
-
T. Yanagida, in Proceeding of the Workshop on Unified Theory and the Baryon Number of the Universe, edited by O. Sawada and A. Sogamoto (KEK Report 79318, Bukuba, Japan, 1979);
-
T. Yanagida, in Proceeding of the Workshop on Unified Theory and the Baryon Number of the Universe, edited by O. Sawada and A. Sogamoto (KEK Report 79318, Bukuba, Japan, 1979);
-
-
-
-
31
-
-
33750639446
-
-
Phys. Rev. D 23, 165 (1981).
-
(1981)
Phys. Rev. D
, vol.23
, pp. 165
-
-
-
32
-
-
0001185643
-
-
See, for example
-
See, for example, R.N. Mohapatra and J.W. Valle, Phys. Rev. D 34, 1642 (1986),
-
(1986)
Phys. Rev. D
, vol.34
, pp. 1642
-
-
Mohapatra, R.N.1
Valle, J.W.2
-
33
-
-
0008297335
-
-
and references therein; for an extension to U(1)' models, see A.E. Faraggi, Phys. Lett. B 245, 435 (1990);
-
and references therein; for an extension to U(1)' models, see A.E. Faraggi, Phys. Lett. B 245, 435 (1990);
-
-
-
-
35
-
-
1542575342
-
These could arise, for example, in a variant on the model in P. Langacker
-
These could arise, for example, in a variant on the model in P. Langacker, Phys. Rev. D 58, 093017 (1998).
-
(1998)
Phys. Rev. D
, vol.58
, pp. 093017
-
-
-
36
-
-
0033588756
-
-
See, for example
-
See, for example, K.R. Dienes, E. Dudas, and T. Gherghetta, Nucl. Phys. B557, 25 (1999);
-
(1999)
Nucl. Phys
, vol.B557
, pp. 25
-
-
Dienes, K.R.1
Dudas, E.2
Gherghetta, T.3
-
38
-
-
0037080641
-
-
N. Arkani-Hamed, S. Dimopoulos, G.R. Dvali, and J. March-Russel, Phys. Rev. D 65, 024032 (2002);
-
(2002)
Phys. Rev. D
, vol.65
, pp. 024032
-
-
Arkani-Hamed, N.1
Dimopoulos, S.2
Dvali, G.R.3
March-Russel, J.4
-
39
-
-
0037053151
-
-
T. Appelquist, B. Dobrescu, E. Ponton, and H. Yee, ibid. 65, 105019 (2002);
-
(2002)
Phys. Rev. D
, vol.65
, pp. 105019
-
-
Appelquist, T.1
Dobrescu, B.2
Ponton, E.3
Yee, H.4
-
40
-
-
85038302822
-
-
H. Davoudiasl, P. Langacker, and M. Perelstein, ibid. 65, 105015 (2002), and references therein.
-
H. Davoudiasl, P. Langacker, and M. Perelstein, ibid. 65, 105015 (2002), and references therein.
-
-
-
-
43
-
-
33847395698
-
-
11, 2558 (1975);
-
11, 2558 (1975);
-
-
-
-
48
-
-
0036838130
-
-
For a general review of neutrinos in cosmology, see
-
For a general review of neutrinos in cosmology, see A.D. Dolgov, Phys. Rep. 370, 333 (2002).
-
(2002)
Phys. Rep
, vol.370
, pp. 333
-
-
Dolgov, A.D.1
-
54
-
-
0000020516
-
-
J. Yang, D.N. Schramm, G. Steigman, and R.T. Rood, Astrophys. J. 227, 697 (1979).
-
(1979)
Astrophys. J
, vol.227
, pp. 697
-
-
Yang, J.1
Schramm, D.N.2
Steigman, G.3
Rood, R.T.4
-
55
-
-
33847382757
-
-
For recent reviews, see G. Steigman, astro-ph/0009506; the articles by K.A. Olive, J.A. Peacock, B.D. Fields, and S. Sarkar, in [29] and [23].
-
For recent reviews, see G. Steigman, astro-ph/0009506; the articles by K.A. Olive, J.A. Peacock, B.D. Fields, and S. Sarkar, in [29] and [23].
-
-
-
-
56
-
-
85107715051
-
-
e, which lowers the nip ratio.
-
e, which lowers the nip ratio.
-
-
-
-
58
-
-
17644448246
-
-
Particle Data Group
-
Particle Data Group, K. Hagiwara et al., Phys. Rev. D 66, 010001 (2002).
-
(2002)
Phys. Rev. D
, vol.66
, pp. 010001
-
-
Hagiwara, K.1
-
59
-
-
85107713710
-
-
R) by an explicit calculation, so the difference is irrelevant for our purposes.
-
R) by an explicit calculation, so the difference is irrelevant for our purposes.
-
-
-
-
60
-
-
33847340984
-
-
R) and more stringent limits. Constraints on extended technicolor models were considered in [35].
-
R) and more stringent limits. Constraints on extended technicolor models were considered in [35].
-
-
-
-
61
-
-
0000520453
-
-
J.R. Ellis, K. Enqvist, D.V. Nanopoulos, and S. Sarkar, Phys. Lett. 167B, 457 (1986);
-
(1986)
Phys. Lett
, vol.167 B
, pp. 457
-
-
Ellis, J.R.1
Enqvist, K.2
Nanopoulos, D.V.3
Sarkar, S.4
-
66
-
-
33750947228
-
-
6 models, see P. Langacker and J. Wang, Phys. Rev. D 58, 115010 (1998).
-
6 models, see P. Langacker and J. Wang, Phys. Rev. D 58, 115010 (1998).
-
-
-
-
71
-
-
85107714642
-
-
6 Yukawa coupling relations must not be respected in order to prevent rapid proton decay [36].
-
6 Yukawa coupling relations must not be respected in order to prevent rapid proton decay [36].
-
-
-
-
72
-
-
16644392594
-
-
See, for example
-
See, for example, G. Cleaver, M. Cvetic, J.R. Espinosa, L.L. Everett, P. Langacker, and J. Wang, Phys. Rev. D 59, 055005 (1999);
-
(1999)
Phys. Rev. D
, vol.59
, pp. 055005
-
-
Cleaver, G.1
Cvetic, M.2
Espinosa, J.R.3
Everett, L.L.4
Langacker, P.5
Wang, J.6
-
74
-
-
33847403879
-
-
We ignore the possibility of kinetic mixing [38
-
We ignore the possibility of kinetic mixing [38].
-
-
-
-
75
-
-
0000077529
-
-
P. Langacker and M.X. Luo, Phys. Rev. D 45, 278 (1992), and references therein.
-
P. Langacker and M.X. Luo, Phys. Rev. D 45, 278 (1992), and references therein.
-
-
-
-
79
-
-
33847408718
-
-
Neutrino 79, edited by A. Haatuft and C. Jarlskog (Astvedt Industrier A/S, Norway, 1979), 2, p. 421.
-
Neutrino 79, edited by A. Haatuft and C. Jarlskog (Astvedt Industrier A/S, Norway, 1979), Vol. 2, p. 421.
-
-
-
-
80
-
-
85107713090
-
-
chiral to be comparable, but their precise relation is uncertain.
-
chiral to be comparable, but their precise relation is uncertain.
-
-
-
-
82
-
-
33847361336
-
-
for a recent discussion, see
-
for a recent discussion, see K.A. Olive and J.A. Peacock [29];
-
, vol.29
-
-
Olive, K.A.1
Peacock, J.A.2
-
83
-
-
0000995564
-
-
for a larger temperature range, see
-
for a larger temperature range, see P. Gondolo and G. Gelmini, Nucl. Phys. B360, 145 (1991).
-
(1991)
Nucl. Phys
, vol.B360
, pp. 145
-
-
Gondolo, P.1
Gelmini, G.2
-
84
-
-
85107713612
-
-
R into massive particles, because the final state mass effects are easily incorporated in the cross section formulae, whereas for the production rate one must explicitly consider the suppressed number density for the massive particles.
-
R into massive particles, because the final state mass effects are easily incorporated in the cross section formulae, whereas for the production rate one must explicitly consider the suppressed number density for the massive particles.
-
-
-
-
85
-
-
0004293858
-
-
See, for example, University of Chicago Press, Chicago
-
See, for example, J.J. Sakurai, Currents and Mesons (University of Chicago Press, Chicago, 1969).
-
(1969)
Currents and Mesons
-
-
Sakurai, J.J.1
-
86
-
-
33847374093
-
-
More complicated form factors are known to fit the experimental data better [50], but Eq. (4.6) is adequate for our purposes.
-
More complicated form factors are known to fit the experimental data better [50], but Eq. (4.6) is adequate for our purposes.
-
-
-
-
89
-
-
33847406089
-
-
See, for example, E.W. Kolb and M.S. Turner, The Early Universe (Addison-Wesley, Redwood City, CA, 1990); and [52].
-
See, for example, E.W. Kolb and M.S. Turner, The Early Universe (Addison-Wesley, Redwood City, CA, 1990); and [52].
-
-
-
-
91
-
-
85107715325
-
-
E6.
-
E6.
-
-
-
-
92
-
-
85107711882
-
-
The difference between current and constituent masses would be reduced if their effects in the annihilation rate were properly correlated with those in the expansion rate. However, as described in Sec. III, the effect on g(T) is small compared with the uncertainty from Tc, and will be neglected
-
c, and will be neglected.
-
-
-
-
93
-
-
33847405227
-
-
in preparation
-
P. Langacker (in preparation).
-
-
-
Langacker, P.1
-
94
-
-
85107713604
-
-
R may still be forbidden in the model.
-
R may still be forbidden in the model.
-
-
-
-
95
-
-
33847368040
-
-
R.
-
R.
-
-
-
-
97
-
-
0037124415
-
-
A.D. Dolgov, S.H. Hansen, S. Pastor, S.T. Petcov, G.G. Raffelt, and D.V. Semikoz, Nucl. Phys. B632, 363 (2002);
-
(2002)
Nucl. Phys
, vol.B632
, pp. 363
-
-
Dolgov, A.D.1
Hansen, S.H.2
Pastor, S.3
Petcov, S.T.4
Raffelt, G.G.5
Semikoz, D.V.6
-
101
-
-
33847391053
-
-
astro-ph/0302207
-
C.L. Bennett et al., astro-ph/0302207.
-
-
-
Bennett, C.L.1
-
103
-
-
33847346736
-
-
astro-ph/0302340
-
S. Hannestad, astro-ph/0302340.
-
-
-
Hannestad, S.1
-
105
-
-
33847368903
-
-
astro-ph/0302465
-
E. Pierpaoli, astro-ph/0302465.
-
-
-
Pierpaoli, E.1
|