Mixed sneutrino dark matter in light of the 2011 XENON and LHC results

In the context of supersymmetric models in which small Dirac neutrino masses are generated by supersymmetry breaking, a mainly right-handed (RH) mixed sneutrino can be an excellent cold dark matter (DM) candidate. We perform a global analysis of the Minimal Supersymmetric Standard Model (MSSM)+RH ne...

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Published inJournal of cosmology and astroparticle physics Vol. 2012; no. 9; p. 13
Main Authors Dumont, Béranger, Bélanger, Geneviève, Fichet, Sylvain, Kraml, Sabine, Schwetz, Thomas
Format Journal Article
LanguageEnglish
Published United States Institute of Physics (IOP) 01.09.2012
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ISSN1475-7516
1475-7508
1475-7516
DOI10.1088/1475-7516/2012/09/013

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Abstract In the context of supersymmetric models in which small Dirac neutrino masses are generated by supersymmetry breaking, a mainly right-handed (RH) mixed sneutrino can be an excellent cold dark matter (DM) candidate. We perform a global analysis of the Minimal Supersymmetric Standard Model (MSSM)+RH neutrino parameter space by means of Markov Chain Monte Carlo sampling. We include all relevant constraints from collider and dark matter searches, paying particular attention to nuclear and astrophysical uncertainties. Two distinct cases can satisfy all constraints: heavy sneutrino DM with mass of order 100 GeV, as well as light sneutrino DM with mass of about 3-6 GeV. We discuss the implications for direct and indirect dark matter searches, as well as for SUSY and Higgs searches at the LHC for both, the light and the heavy sneutrino dark matter case. The light sneutrino case is excluded by the 125-126 GeV Higgs signal.
AbstractList In the context of supersymmetric models in which small Dirac neutrino masses are generated by supersymmetry breaking, a mainly right-handed (RH) mixed sneutrino can be an excellent cold dark matter (DM) candidate. We perform a global analysis of the Minimal Supersymmetric Standard Model (MSSM)+RH neutrino parameter space by means of Markov Chain Monte Carlo sampling. We include all relevant constraints from collider and dark matter searches, paying particular attention to nuclear and astrophysical uncertainties. Two distinct cases can satisfy all constraints: heavy sneutrino DM with mass of order 100 GeV, as well as light sneutrino DM with mass of about 3-6 GeV. We discuss the implications for direct and indirect dark matter searches, as well as for SUSY and Higgs searches at the LHC for both, the light and the heavy sneutrino dark matter case. The light sneutrino case is excluded by the 125-126 GeV Higgs signal.
In the context of supersymmetric models in which small Dirac neutrino massesare generated by supersymmetry breaking, a mainly right-handed (RH) mixedsneutrino can be an excellent cold dark matter (DM) candidate. We perform aglobal analysis of the Minimal Supersymmetric Standard Model (MSSM)+RH neutrinoparameter space by means of Markov Chain Monte Carlo scans. We include allrelevant constraints from collider and dark matter searches, paying particularattention to nuclear and astrophysical uncertainties. Two distinct cases cansatisfy all constraints: heavy sneutrino DM with mass of order 100 GeV, as wellas light sneutrino DM with mass of about 3-6 GeV. We discuss the implicationsfor direct and indirect dark matter searches, as well as for SUSY and Higgssearches at the LHC for both, the light and the heavy sneutrino dark mattercase. The light sneutrino case is excluded by the 125-126 GeV Higgs signal.
Author Schwetz, Thomas
Bélanger, Geneviève
Fichet, Sylvain
Kraml, Sabine
Dumont, Béranger
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Cites_doi 10.1103/PhysRevD.77.115015
10.1007/JHEP07(2011)026
10.1016/j.physletb.2012.08.021
10.1098/rspa.1946.0056
10.1103/PhysRevD.79.063509
10.1103/PhysRevD.82.023530
10.1140/epjc/s10052-008-0662-y
10.1103/PhysRevD.75.065001
10.1103/PhysRevLett.108.231801
10.1088/1742-6596/110/1/012014
10.1016/j.cpc.2010.11.033
10.1103/PhysRevLett.107.141301
10.1086/592738
10.1103/PhysRevLett.108.081806
10.1214/ss/1177011136
10.1007/JHEP03(2010)108
10.1016/j.physletb.2010.04.054
10.1016/j.physletb.2012.08.020
10.1103/PhysRevD.64.053005
10.1111/j.1365-2966.2007.11964.x
10.1063/1.3264550
10.1016/S0010-4655(97)00123-9
10.1088/0004-637X/756/1/89
10.1103/PhysRevLett.107.051301
10.1088/1475-7516/2012/01/015
10.1086/323684
10.1088/0067-0049/192/2/18
10.1088/0004-637X/692/2/1075
10.1080/00107510802066753
10.1088/1126-6708/2007/11/029
10.1016/j.physletb.2009.05.034
10.1088/0034-4885/74/2/026201
10.1088/1126-6708/2009/11/026
10.1103/PhysRevLett.106.131301
10.1017/CBO9780511617270
10.1007/JHEP06(2011)129
10.1140/epjc/s10052-012-1874-8
10.1103/PhysRevD.71.087302
10.1016/0370-1573(95)00058-5
10.1103/PhysRevD.80.055026
10.1088/1126-6708/2008/10/080
10.1103/RevModPhys.59.671
10.1088/1475-7516/2010/11/017
10.1051/0004-6361/200913381
10.1017/CBO9780511770739
10.1103/PhysRevD.66.032005
10.1103/PhysRevLett.107.241302
10.1016/j.physletb.2009.06.009
10.1103/PhysRevD.64.115011
10.1088/0954-3899/38/8/085003
10.1088/0034-4885/70/11/R02
10.1016/j.cpc.2006.11.009
10.1103/PhysRevLett.101.161802
10.1103/PhysRevD.73.015013
10.1103/PhysRevD.73.051301
10.1103/PhysRevD.79.023510
10.1016/j.cpc.2011.07.015
10.1088/1475-7516/2012/05/005
10.1086/304888
10.1016/S0370-2693(00)00260-4
10.1007/JHEP12(2011)088
10.1103/PhysRevLett.106.131302
10.1088/0954-3899/34/2/R01
10.1088/0004-637X/712/1/260
10.1103/PhysRevLett.107.131302
10.1103/PhysRevLett.105.121101
10.1016/S0370-2693(98)00196-8
10.1103/PhysRevD.86.043515
10.1051/0004-6361/201014385
10.1016/j.cpc.2008.11.019
10.1088/1475-7516/2011/11/027
10.1103/PhysRevLett.98.022002
10.1086/321496
10.1016/0370-2693(96)00386-3
10.1103/PhysRevD.79.095009
10.1007/JHEP09(2010)111
10.1016/j.physrep.2007.12.004
10.1103/PhysRevD.84.095008
10.1103/PhysRevD.81.035019
10.1088/1475-7516/2011/12/014
10.1016/j.cpc.2009.09.003
10.1016/j.physrep.2004.08.031
10.1103/PhysRevD.73.072003
10.1103/PhysRevD.76.041302
10.1016/j.physletb.2004.11.047
10.1016/j.physletb.2012.02.051
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References A. Thomas (63)
89
M. Drees (11) 2004
110
111
F. Deppisch (24) 2008; 2008
112
113
114
116
P.J. McMillan (70)
95
98
99
12
Particle Data Group collaboration (73) 2010; 37
14
15
16
D.G. Cerdeno (37) 2011; 2011
17
18
19
CDMS collaboration (94)
1
2
C. Arina (41) 2007; 2007
S. Gillessen . (68) 2009; 692
3
R. Allahverdi (30)
LEP2 SUSY Working Group (79)
G. Bélanger (45) 2011; 07
7
J.F. Navarro (101) 1997; 490
9
T. Schwetz (92) 2011; 08
Z. Kang (35)
C. Arina (21)
D. Stöckinger (90) 2007; 34
20
S.P. Martin (10)
22
23
25
27
28
29
CMS collaboration (97) 2011
G. Bélanger (39) 2011; 2011
G. Bhattacharyya (5) 2011; 74
31
32
33
The Tevatron Electroweak Working Group (72)
34
36
38
R. Catena (60) 2010; 08
G.F. Giudice (4) 2008; 110
R. Catena (61) 2012; 2012
XENON100 collaboration (115)
G. Bélanger (40) 2010; 2010
S.E. Koposov (69) 2010; 712
D. Maurin (104) 2001; 555
LEP2 SUSY Working Group (81)
42
43
44
J. Bovy (62) 2012; 756
47
WMAP collaboration (46) 2011; 192
48
49
CMS (86) 2011
G. Bélanger (51) 2009; 2009
50
C. Grojean (6)
52
53
54
55
56
57
58
59
R. Mohapatra . (8) 2007; 70
CMS collaboration (83) 2011
F. Donato . (105) 2001; 563
D. Maurin (103)
64
65
66
Heavy Flavor Averaging Group collaboration (84)
ALEPH (78) 2000
71
J. Kopp (91) 2012; 03
74
75
76
77
A. Ghez . (67) 2008; 689
J. Herrero-Garcia (93)
D.G. Cerdeno (26) 2009; 08
G. Bertone . (96) 2012; 2012
100
102
K. Hagiwara (88) 2011; 38
80
107
108
P. Binetruy (13) 2006
82
109
85
87
S. Kraml (106)
References_xml – ident: 44
  doi: 10.1103/PhysRevD.77.115015
– ident: 34
  doi: 10.1007/JHEP07(2011)026
– year: 2006
  ident: 13
  publication-title: Supersymmetry: theory, experiment and cosmology
– ident: 114
  doi: 10.1016/j.physletb.2012.08.021
– ident: 116
  doi: 10.1098/rspa.1946.0056
– ident: 93
– ident: 107
  doi: 10.1103/PhysRevD.79.063509
– ident: 59
  doi: 10.1103/PhysRevD.82.023530
– ident: 47
  doi: 10.1140/epjc/s10052-008-0662-y
– ident: 19
  doi: 10.1103/PhysRevD.75.065001
– ident: 98
  doi: 10.1103/PhysRevLett.108.231801
– volume: 110
  start-page: 012014
  issn: 1742-6596
  year: 2008
  ident: 4
  publication-title: J. Phys. Conf. Ser.
  doi: 10.1088/1742-6596/110/1/012014
– ident: 54
  doi: 10.1016/j.cpc.2010.11.033
– ident: 77
  doi: 10.1103/PhysRevLett.107.141301
– volume: 689
  start-page: 1044
  issn: 0004-637X
  year: 2008
  ident: 67
  publication-title: Astrophys. J.
  doi: 10.1086/592738
– ident: 38
  doi: 10.1103/PhysRevLett.108.081806
– ident: 63
– ident: 52
  doi: 10.1214/ss/1177011136
– ident: 32
  doi: 10.1007/JHEP03(2010)108
– ident: 33
  doi: 10.1016/j.physletb.2010.04.054
– ident: 113
  doi: 10.1016/j.physletb.2012.08.020
– ident: 72
– ident: 30
– ident: 15
  doi: 10.1103/PhysRevD.64.053005
– ident: 71
  doi: 10.1111/j.1365-2966.2007.11964.x
– ident: 106
– ident: 29
  doi: 10.1063/1.3264550
– ident: 56
  doi: 10.1016/S0010-4655(97)00123-9
– volume: 756
  issn: 0004-637X
  year: 2012
  ident: 62
  publication-title: Astrophys. J.
  doi: 10.1088/0004-637X/756/1/89
– ident: 74
  doi: 10.1103/PhysRevLett.107.051301
– volume: 2012
  start-page: 015
  issn: 1475-7516
  year: 2012
  ident: 96
  publication-title: J. Cosmol. Astropart. Phys.
  doi: 10.1088/1475-7516/2012/01/015
– volume: 563
  start-page: 172
  issn: 0004-637X
  year: 2001
  ident: 105
  publication-title: Astrophys. J.
  doi: 10.1086/323684
– ident: 103
– volume: 192
  start-page: 18
  issn: 0067-0049
  year: 2011
  ident: 46
  publication-title: Astrophys. J. Suppl.
  doi: 10.1088/0067-0049/192/2/18
– volume: 692
  start-page: 1075
  issn: 0004-637X
  year: 2009
  ident: 68
  publication-title: Astrophys. J.
  doi: 10.1088/0004-637X/692/2/1075
– ident: 50
  doi: 10.1080/00107510802066753
– volume: 2007
  start-page: 029
  issn: 1126-6708
  year: 2007
  ident: 41
  publication-title: J. High Energy Phys.
  doi: 10.1088/1126-6708/2007/11/029
– ident: 25
  doi: 10.1016/j.physletb.2009.05.034
– volume: 74
  issn: 0034-4885
  year: 2011
  ident: 5
  publication-title: Rept. Prog. Phys.
  doi: 10.1088/0034-4885/74/2/026201
– ident: 80
– volume: 2009
  start-page: 026
  issn: 1126-6708
  year: 2009
  ident: 51
  publication-title: J. High Energy Phys.
  doi: 10.1088/1126-6708/2009/11/026
– ident: 48
  doi: 10.1103/PhysRevLett.106.131301
– volume: 08
  year: 2010
  ident: 60
  publication-title: JCAP
– ident: 10
– volume: 07
  year: 2011
  ident: 45
  publication-title: JHEP
– ident: 70
– ident: 12
  doi: 10.1017/CBO9780511617270
– year: 2011
  ident: 86
– ident: 36
  doi: 10.1007/JHEP06(2011)129
– ident: 99
  doi: 10.1140/epjc/s10052-012-1874-8
– ident: 6
– ident: 111
  doi: 10.1103/PhysRevD.71.087302
– ident: 1
  doi: 10.1016/0370-1573(95)00058-5
– ident: 28
  doi: 10.1103/PhysRevD.80.055026
– volume: 2008
  start-page: 080
  issn: 1126-6708
  year: 2008
  ident: 24
  publication-title: J. High Energy Phys.
  doi: 10.1088/1126-6708/2008/10/080
– ident: 7
  doi: 10.1103/RevModPhys.59.671
– volume: 2010
  start-page: 017
  issn: 1475-7516
  year: 2010
  ident: 40
  publication-title: J. Cosmol. Astropart. Phys.
  doi: 10.1088/1475-7516/2010/11/017
– ident: 21
– ident: 65
  doi: 10.1051/0004-6361/200913381
– ident: 112
– ident: 3
  doi: 10.1017/CBO9780511770739
– ident: 95
  doi: 10.1103/PhysRevD.66.032005
– ident: 100
  doi: 10.1103/PhysRevLett.107.241302
– ident: 109
  doi: 10.1016/j.physletb.2009.06.009
– ident: 14
  doi: 10.1103/PhysRevD.64.115011
– volume: 38
  start-page: 085003
  issn: 0954-3899
  year: 2011
  ident: 88
  publication-title: J. Phys.
  doi: 10.1088/0954-3899/38/8/085003
– volume: 70
  start-page: 1757
  issn: 0034-4885
  year: 2007
  ident: 8
  publication-title: Rept. Prog. Phys.
  doi: 10.1088/0034-4885/70/11/R02
– ident: 55
  doi: 10.1016/j.cpc.2006.11.009
– ident: 22
  doi: 10.1103/PhysRevLett.101.161802
– ident: 49
  doi: 10.1103/PhysRevD.73.015013
– ident: 35
– ident: 18
  doi: 10.1103/PhysRevD.73.051301
– year: 2004
  ident: 11
  publication-title: Theory and phenomenology of sparticles: an account of four-dimensional N=1 supersymmetry in high energy physics
– ident: 23
  doi: 10.1103/PhysRevD.79.023510
– ident: 58
  doi: 10.1016/j.cpc.2011.07.015
– ident: 94
– volume: 2012
  start-page: 005
  issn: 1475-7516
  year: 2012
  ident: 61
  publication-title: J. Cosmol. Astropart. Phys.
  doi: 10.1088/1475-7516/2012/05/005
– volume: 490
  start-page: 493
  issn: 0004-637X
  year: 1997
  ident: 101
  publication-title: Astrophys. J.
  doi: 10.1086/304888
– ident: 17
  doi: 10.1016/S0370-2693(00)00260-4
– volume: 37
  issn: 0954-3899
  year: 2010
  ident: 73
  publication-title: J. Phys.
– year: 2011
  ident: 97
– ident: 87
  doi: 10.1007/JHEP12(2011)088
– ident: 76
  doi: 10.1103/PhysRevLett.106.131302
– volume: 34
  start-page: R45
  issn: 0954-3899
  year: 2007
  ident: 90
  publication-title: J. Phys.
  doi: 10.1088/0954-3899/34/2/R01
– volume: 712
  start-page: 260
  issn: 0004-637X
  year: 2010
  ident: 69
  publication-title: Astrophys. J.
  doi: 10.1088/0004-637X/712/1/260
– ident: 75
  doi: 10.1103/PhysRevLett.107.131302
– ident: 102
  doi: 10.1103/PhysRevLett.105.121101
– ident: 16
  doi: 10.1016/S0370-2693(98)00196-8
– ident: 42
  doi: 10.1103/PhysRevD.86.043515
– ident: 84
– ident: 66
  doi: 10.1051/0004-6361/201014385
– ident: 53
  doi: 10.1016/j.cpc.2008.11.019
– volume: 2011
  start-page: 027
  issn: 1475-7516
  year: 2011
  ident: 37
  publication-title: J. Cosmol. Astropart. Phys.
  doi: 10.1088/1475-7516/2011/11/027
– ident: 85
  doi: 10.1103/PhysRevLett.98.022002
– volume: 03
  year: 2012
  ident: 91
  publication-title: JCAP
– volume: 08
  year: 2011
  ident: 92
  publication-title: JCAP
– volume: 555
  start-page: 585
  issn: 0004-637X
  year: 2001
  ident: 104
  publication-title: Astrophys. J.
  doi: 10.1086/321496
– ident: 79
– ident: 64
  doi: 10.1016/0370-2693(96)00386-3
– ident: 115
– ident: 108
  doi: 10.1103/PhysRevD.79.095009
– volume: 08
  year: 2009
  ident: 26
  publication-title: JCAP
– ident: 31
  doi: 10.1007/JHEP09(2010)111
– ident: 9
  doi: 10.1016/j.physrep.2007.12.004
– ident: 110
  doi: 10.1103/PhysRevD.84.095008
– ident: 27
  doi: 10.1103/PhysRevD.81.035019
– volume: 2011
  start-page: 014
  issn: 1475-7516
  year: 2011
  ident: 39
  publication-title: J. Cosmol. Astropart. Phys.
  doi: 10.1088/1475-7516/2011/12/014
– ident: 57
  doi: 10.1016/j.cpc.2009.09.003
– year: 2011
  ident: 83
  publication-title: Search for supersymmetry with the razor variables at CMS
– ident: 2
  doi: 10.1016/j.physrep.2004.08.031
– ident: 89
  doi: 10.1103/PhysRevD.73.072003
– ident: 81
– ident: 20
  doi: 10.1103/PhysRevD.76.041302
– ident: 43
  doi: 10.1016/j.physletb.2004.11.047
– year: 2000
  ident: 78
  publication-title: A combination of preliminary electroweak measurements and constraints on the standard model, Technical Report http://cdsweb.cern.ch/record/426819CERN-EP-2000-016
– ident: 82
  doi: 10.1016/j.physletb.2012.02.051
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Snippet In the context of supersymmetric models in which small Dirac neutrino masses are generated by supersymmetry breaking, a mainly right-handed (RH) mixed...
In the context of supersymmetric models in which small Dirac neutrino massesare generated by supersymmetry breaking, a mainly right-handed (RH) mixedsneutrino...
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SubjectTerms ASTROPHYSICS
ASTROPHYSICS, COSMOLOGY AND ASTRONOMY
CERN LHC
Cold dark matter
Computer simulation
COSMOLOGY
Dark matter
GEV RANGE
HIGGS BOSONS
HIGGS MODEL
High Energy Physics - Phenomenology
MARKOV PROCESS
MONTE CARLO METHOD
Monte Carlo methods
NEUTRINOS
NONLUMINOUS MATTER
PARTICLE IDENTIFICATION
Physics
REST MASS
Sampling
Searching
SPACE
SPARTICLES
STANDARD MODEL
SUPERSYMMETRY
SYMMETRY BREAKING
Xenon
Title Mixed sneutrino dark matter in light of the 2011 XENON and LHC results
URI https://www.proquest.com/docview/1673382342
https://www.proquest.com/docview/1678012308
https://hal.science/hal-01122257
https://www.osti.gov/biblio/22279875
Volume 2012
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