-
1
-
-
4243734527
-
-
SuperKamiokande Collaboration hep-ex/0009001
-
(2000)
Phys. Rev. Lett
, vol.85
, pp. 3999
-
-
-
3
-
-
33744572748
-
-
MACRO Collaboration hep-ex/0106049
-
(2001)
Phys. Lett. B
, vol.517
, pp. 59
-
-
-
6
-
-
4644327605
-
-
Gallex Collaboration
-
(1999)
Phys. Lett. B
, vol.447
, pp. 127
-
-
-
7
-
-
0009783481
-
-
GNO Collaboration
-
(2000)
Phys. Lett. B
, vol.490
, pp. 16
-
-
-
9
-
-
0009818434
-
-
SNO Collaboration, nucl-ex/0204008
-
-
-
-
10
-
-
0009819901
-
-
SNO Collaboration, nucl-ex/0204009
-
-
-
-
11
-
-
0009853232
-
-
SAGE Collaboration, astro-ph/0204245
-
-
-
-
12
-
-
0009835586
-
-
SuperKamiokande Collaboration, hep-ex/0205075
-
-
-
-
13
-
-
0009868963
-
-
Bugey Collaboration
-
(1995)
Nucl. Phys. B
, vol.434
, pp. 503
-
-
-
14
-
-
0004366022
-
-
Chooz Collaboration, hep-ex/9907037
-
(1999)
Phys. Lett. B
, vol.466
, pp. 415
-
-
-
15
-
-
25344473834
-
-
also: Palo Verde Collaboration, hep-ex/9912050
-
(2000)
Phys. Rev. Lett
, vol.84
, pp. 3764
-
-
See1
-
16
-
-
0009852667
-
-
LSND Collaboration, hep-ex/0104049
-
-
-
-
19
-
-
0009851207
-
-
We use the results in: JHEP 0105 52, hep-ph/0102234, updated version with SNO, CC, NC and day/night data
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(2001)
-
-
Creminelli, P.1
-
20
-
-
0009821067
-
-
Our atmospheric fit is based on sub-GeV, multi-GeV, PC and UPμ SuperKamiokande data after 79 kton year, as described in: A. Strumia, hep-ph/0201134
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-
-
-
31
-
-
0009835761
-
-
ICARUS Collaboration, hep-ex/0103008
-
-
-
Arneodo, F.1
-
38
-
-
4243240788
-
-
Although the existence of additional (Majorana) phases was perhaps known even before, they were not discussed until the first of previous references, and soon after in: J. Schechter, J.W. Valle
-
(1980)
Phys. Rev. D
, vol.22
, pp. 2227
-
-
-
39
-
-
0009821069
-
-
Their observability in 0ν2β decay was first remarked in: M. Doi, T. Kotani, H. Nishiura, K. Okuda, E. Takasugi
-
(1981)
Phys. Lett. B
, vol.102
, pp. 323
-
-
-
49
-
-
0009855650
-
-
For reviews see, e.g., Neutrinos from supernovæ: experimental status and perspectives, Talk given at matter, antimatter and dark matter, Trento, Italy, October 29-30, 2001, and references therein; G.G. Raffelt, hep-ph/0201099
-
-
-
Cei, F.1
-
59
-
-
0009819587
-
-
For recent works see, e.g., hep-ph/0111112
-
-
-
Ringwald, A.1
-
61
-
-
0009874531
-
-
hep-ph/0109202, and references therein
-
-
-
Sigl, G.1
-
73
-
-
0003467192
-
-
Goals and features of GENIUS are well documented, in: H.V. Klapdor-Kleingrothaus (Ed.), World Scientific, This book includes many related theoretical works
-
(2001)
Sixty Years of Double Beta decay
-
-
-
79
-
-
0009823232
-
-
For instance, the Katrin sensitivity was obtained assuming ΔE = 1 eV (see also the homepage of the conference held ad Bad Liebenzell on January
-
(2001)
-
-
-
98
-
-
4243720999
-
Lepton number violation and neutrino mass
-
published in: Neutrino 1984, Dortmund, Germany-see especially Section 4 there
-
-
-
Wolfenstein, L.1
-
99
-
-
0002425293
-
-
More formal arguments (but of minor generality) were previously presented in:
-
(1981)
Phys. Lett. B
, vol.107
, pp. 77
-
-
Wolfenstein, L.1
-
120
-
-
0009822848
-
-
For a particularly clear discussion of the effects induced by neutrino Yukawa couplings see:
-
-
-
Lavignac, S.1
-
162
-
-
0009847976
-
-
μτ is small, though one could have rather guessed smallest element
-
(1980)
Phys. Lett. B
, vol.93
, pp. 389
-
-
-
163
-
-
0009835595
-
-
τ-breaking effects were considered, e.g., in: A.S. Joshipura, S.D. Rindani, hep-ph/9811252
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191
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0009847978
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Data available at the internet address:
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