Article (Scientific journals)
Radiative seesaw: Warm dark matter, collider and lepton flavour violating signals
Aristizabal Sierra, Diego; Kubo, Jisuke; Restrepo, D. et al.
2009 • In Physical Review. D, Particles, Fields, Gravitation, and Cosmology, 79, p. 013011
Peer Reviewed verified by ORBi
 

Files


Full Text
radiative-seesaw-pheno.pdf
Author preprint (312.2 kB)
Download

All documents in ORBi are protected by a user license.

Send to



Details



Keywords :
Neutrino masses and mixings; Dark matter; Collider phenomenology
Abstract :
[en] Extending the standard model with three right-handed neutrinos (Nk) and a second Higgs doublet (η), odd under the discrete parity symmetry Z2, Majorana neutrino masses can be generated at one-loop order. In the resulting model, the lightest stable particle, either a boson or a fermion, might be a dark matter candidate. Here we assume a specific mass spectrum (M1≪M2
Disciplines :
Physics
Author, co-author :
Aristizabal Sierra, Diego ;  Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Physique des astroparticules
Kubo, Jisuke
Restrepo, D.
Suematsu, Daijiro
Zapata, Oscar
Language :
English
Title :
Radiative seesaw: Warm dark matter, collider and lepton flavour violating signals
Publication date :
January 2009
Journal title :
Physical Review. D, Particles, Fields, Gravitation, and Cosmology
ISSN :
1550-7998
eISSN :
1550-2368
Publisher :
American Physical Society, College Park, United States - Maryland
Volume :
79
Pages :
013011
Peer reviewed :
Peer Reviewed verified by ORBi
Available on ORBi :
since 20 January 2014

Statistics


Number of views
227 (1 by ULiège)
Number of downloads
188 (0 by ULiège)

Scopus citations®
 
108
Scopus citations®
without self-citations
69
OpenAlex citations
 
108

Bibliography


  • Q.R. Ahmad (SNO Collaboration), Phys. Rev. Lett. 89, 011301 (2002). PRLTAO 0031-9007 10.1103/PhysRevLett.89.011301
  • Y. Fukuda (Super-Kamiokande Collaboration), Phys. Rev. Lett. 81, 1562 (1998). PRLTAO 0031-9007 10.1103/PhysRevLett.81.1562
  • K. Eguchi (KamLAND Collaboration), Phys. Rev. Lett. 90, 021802 (2003). PRLTAO 0031-9007 10.1103/PhysRevLett.90.021802
  • D.N. Spergel (WMAP Collaboration), Astrophys. J. Suppl. Ser. 170, 377 (2007). APJSA2 0067-0049 10.1086/513700
  • P. Minkowski, Phys. Lett. 67B, 421 (1977); PYLBAJ 0370-2693 10.1016/0370-2693(77)90435-X
  • T. Yanagida, in KEK Lectures, edited by, O. Sawada, and, A. Sugamoto, (KEK, Ibaraki, Japan, 1979);
  • M. Gell-Mann, P. Ramond, and R. Slansky, in Supergravity, edited by, P. van Niewenhuizen, and, D. Freedman, (North-Holland, Amsterdam, 1979);
  • R.N. Mohapatra and G. Senjanovic, Phys. Rev. Lett. 44, 912 (1980); PRLTAO 0031-9007 10.1103/PhysRevLett.44.912
  • J. Schechter and J.W.F. Valle, Phys. Rev. D PRVDAQ 0556-2821 22, 2227 (1980). 10.1103/PhysRevD.22.2227
  • M. Hirsch and J.W.F. Valle, New J. Phys. 6, 76 (2004); NJOPFM 1367-2630 10.1088/1367-2630/6/1/076
  • M. Hirsch, M.A. Diaz, W. Porod, J.C. Romao, and J.W.F. Valle, Phys. Rev. D PRVDAQ 0556-2821 62, 113008 (2000); 10.1103/PhysRevD.62.113008
  • M. Hirsch M.A. Diaz W. Porod J.C. Romao J.W.F. Valle Phys. Rev. D PRVDAQ 0556-2821 65, 119901(E) (2002). 10.1103/PhysRevD.65.119901
  • M. Hirsch, A. Vicente, and W. Porod, Phys. Rev. D PRVDAQ 0556-2821 77, 075005 (2008). 10.1103/PhysRevD.77.075005
  • J. Garayoa and T. Schwetz, J. High Energy Phys. JHEPFG 1029-8479 03 (2008) 009. 10.1088/1126-6708/2008/03/009
  • A. Zee, Phys. Lett. 93B, 389 (1980); PYLBAJ 0370-2693 10.1016/0370-2693(80)90349-4
  • A. Zee Phys. Lett. 95B, 461 (1980); PYLBAJ 0370-2693
  • D. Aristizabal Sierra and D. Restrepo, J. High Energy Phys. JHEPFG 1029-8479 08 (2006) 036. 10.1088/1126-6708/2006/08/036
  • A. Zee, Nucl. Phys. NUPBBO 0550-3213 B264, 99 (1986); 10.1016/0550-3213(86)90475-X
  • K.S. Babu, Phys. Lett. B 203, 132 (1988); PYLBAJ 0370-2693 10.1016/0370-2693(88)91584-5
  • K.S. Babu and C. Macesanu, Phys. Rev. D PRVDAQ 0556-2821 67, 073010 (2003); 10.1103/PhysRevD.67.073010
  • D. Aristizabal Sierra and M. Hirsch, J. High Energy Phys. JHEPFG 1029-8479 12 (2006) 052; 10.1088/1126-6708/2006/12/052
  • M. Nebot, J.F. Oliver, D. Palao, and A. Santamaria, Phys. Rev. D PRVDAQ 0556-2821 77, 093013 (2008). 10.1103/PhysRevD.77.093013
  • D. Aristizabal Sierra, M. Hirsch, and S.G. Kovalenko, Phys. Rev. D PRVDAQ 0556-2821 77, 055011 (2008); 10.1103/PhysRevD.77.055011
  • U. Mahanta, Phys. Rev. D PRVDAQ 0556-2821 62, 073009 (2000). 10.1103/PhysRevD.62.073009
  • S. Hannestad and G. Raffelt, J. Cosmol. Astropart. Phys. 1475-7516 04 (2004) 008; 10.1088/1475-7516/2004/04/008
  • P. Crotty, J. Lesgourgues, and S. Pastor, Phys. Rev. D PRVDAQ 0556-2821 69, 123007 (2004). 10.1103/PhysRevD.69.123007
  • J.R. Primack, arXiv:astro-ph/9707285.
  • P. Bode, J.P. Ostriker, and N. Turok, Astrophys. J. 556, 93 (2001); ASJOAB 0004-637X 10.1086/321541
  • B. Moore, T. Quinn, F. Governato, J. Stadel, and G. Lake, Mon. Not. R. Astron. Soc. 310, 1147 (1999); MNRAA4 0035-8711 10.1046/j.1365-8711.1999.03039.x
  • V. Avila-Reese, P. Colin, O. Valenzuela, E. D'Onghia, and C. Firmani, Astrophys. J. 559, 516 (2001). ASJOAB 0004-637X 10.1086/322411
  • M. Viel, J. Lesgourgues, M.G. Haehnelt, S. Matarrese, and A. Riotto, Phys. Rev. D PRVDAQ 1550-7998 71, 063534 (2005); 10.1103/PhysRevD.71.063534
  • M. Viel, G.D. Becker, J.S. Bolton, M.G. Haehnelt, M. Rauch, and W.L.W. Sargent, Phys. Rev. Lett. 100, 041304 (2008). PRLTAO 0031-9007 10.1103/PhysRevLett.100.041304
  • In this case WDM gives a contribution of ∼10% to the total DM relic density.
  • J. Kubo and D. Suematsu, Phys. Lett. B 643, 336 (2006); PYLBAJ 0370-2693 10.1016/j.physletb.2006.11.005
  • M. Lattanzi and J.W.F. Valle, Phys. Rev. Lett. 99, 121301 (2007); PRLTAO 0031-9007 10.1103/PhysRevLett.99.121301
  • C. Boehm, Y. Farzan, T. Hambye, S. Palomares-Ruiz, and S. Pascoli, Phys. Rev. D PRVDAQ 1550-7998 77, 043516 (2008); 10.1103/PhysRevD.77.043516
  • C. Arina, F. Bazzocchi, N. Fornengo, J.C. Romao, and J.W.F. Valle, Phys. Rev. Lett. 101, 161802 (2008); PRLTAO 0031-9007 10.1103/PhysRevLett.101.161802
  • E. Ma, Phys. Lett. B 662, 49 (2008). PYLBAJ 0370-2693 10.1016/j.physletb.2008.02.053
  • E. Ma, Phys. Rev. D PRVDAQ 1550-7998 73, 077301 (2006). 10.1103/PhysRevD.73.077301
  • J. Kubo, E. Ma, and D. Suematsu, Phys. Lett. B 642, 18 (2006). PYLBAJ 0370-2693 10.1016/j.physletb.2006.08.085
  • G. Passarino and M.J.G. Veltman, Nucl. Phys. NUPBBO 0550-3213 B160, 151 (1979). 10.1016/0550-3213(79)90234-7
  • A suppression mechanism based on a low-energy flavor symmetry in the same type of models, with a radiative neutrino mass generation, was proposed in.
  • Y. Kajiyama, J. Kubo, and H. Okada, Phys. Rev. D PRVDAQ 1550-7998 75, 033001 (2007). 10.1103/PhysRevD.75.033001
  • S. Dodelson and L.M. Widrow, Phys. Rev. Lett. 72, 17 (1994). PRLTAO 0031-9007 10.1103/PhysRevLett.72.17
  • T. Asaka, M. Laine, and M. Shaposhnikov, J. High Energy Phys. JHEPFG 1029-8479 01 (2007) 091. 10.1088/1126-6708/2007/01/091
  • A possible origin of this symmetry was discussed in.
  • A.D. Dolgov and S.H. Hansen, Astropart. Phys. 16, 339 (2002). APHYEE 0927-6505 10.1016/S0927-6505(01)00115-3
  • K. Abazajian, G.M. Fuller, and W.H. Tucker, Astrophys. J. 562, 593 (2001). ASJOAB 0004-637X 10.1086/323867
  • M. Mapelli, A. Ferrara, and E. Pierpaoli, Mon. Not. R. Astron. Soc. MNRAA4 0035-8711 369, 1719 (2006). 10.1111/j.1365-2966.2006.10408.x
  • A. Boyarsky, A. Neronov, O. Ruchayskiy, and M. Shaposhnikov, Mon. Not. R. Astron. Soc. 370, 213 (2006); MNRAA4 0035-8711
  • A. Boyarsky A. Neronov O. Ruchayskiy M. Shaposhnikov JETP Lett. 83, 133 (2006); JTPLA2 0021-3640 10.1134/S0021364006040011
  • A. Boyarsky, D. Iakubovskyi, O. Ruchayskiy, and V. Savchenko, Mon. Not. R. Astron. Soc. 387, 1361 (2008). MNRAA4 0035-8711 10.1111/j.1365-2966.2008. 13266.x
  • If the sterile neutrinos as WDM are generated in decays of some heavier particles, then the situation may change.
  • A. Kusenko, Phys. Rev. Lett. 97, 241301 (2006); PRLTAO 0031-9007 10.1103/PhysRevLett.97.241301
  • K. Petraki and A. Kusenko, Phys. Rev. D PRVDAQ 1550-7998 77, 065014 (2008); 10.1103/PhysRevD.77.065014
  • K. Petraki, Phys. Rev. D PRVDAQ 1550-7998 77, 105004 (2008); 10.1103/PhysRevD.77.105004
  • D. Boyanovsky, Phys. Rev. D PRVDAQ 1550-7998 78, 103505 (2008). 10.1103/PhysRevD.78.103505
  • U. Seljak, A. Makarov, P. McDonald, and H. Trac, Phys. Rev. Lett. 97, 191303 (2006). PRLTAO 0031-9007 10.1103/PhysRevLett.97.191303
  • M. Viel, J. Lesgourgues, M.G. Haehnelt, S. Matarrese, and A. Riotto, Phys. Rev. Lett. 97, 071301 (2006). PRLTAO 0031-9007 10.1103/PhysRevLett.97. 071301
  • D. Gorbunov, A. Khmelnitsky, and V. Rubakov, J. Cosmol. Astropart. Phys. 1475-7516 10 (2008) 041. 10.1088/1475-7516/2008/10/041
  • A. Palazzo, D. Cumberbatch, A. Slosar, and J. Silk, Phys. Rev. D PRVDAQ 1550-7998 76, 103511 (2007). 10.1103/PhysRevD.76.103511
  • "MEG experiment." Home page: http://meg.web.psi.ch/index.html.
  • A. Djouadi, Phys. Rep. 459, 1 (2008). PRPLCM 0370-1573 10.1016/j.physrep.2007.10.005
  • Q.H. Cao, E. Ma, and G. Rajasekaran, Phys. Rev. D PRVDAQ 1550-7998 76, 095011 (2007). 10.1103/PhysRevD.76.095011
  • M. Battaglia, A. Ferrari, A. Kiiskinen, and T. Maki, arXiv:hep-ex/ 0112015.
  • F. de Campos, O.J.P. Eboli, M.B. Magro, W. Porod, D. Restrepo, M. Hirsch, and J.W.F. Valle, J. High Energy Phys. JHEPFG 1029-8479 05 (2008) 048; 10.1088/1126-6708/2008/05/048
  • D. Aristizabal Sierra, W. Porod, D. Restrepo, and C.E. Yaguna, Phys. Rev. D PRVDAQ 1550-7998 78, 015015 (2008). 10.1103/PhysRevD.78.015015
  • M. Maltoni, T. Schwetz, M.A. Tortola, and J.W.F. Valle, New J. Phys. 6, 122 (2004). NJOPFM 1367-2630 10.1088/1367-2630/6/1/122
  • Online version 6 in arXiv:hep-ph/0405172 contains updated fits with data included up to Sep 2007.
  • R.M. Barnett, J.F. Gunion, and H.E. Haber, Phys. Lett. B 315, 349 (1993). PYLBAJ 0370-2693 10.1016/0370-2693(93)91623-U
  • B.C. Allanach, C.G. Lester, M.A. Parker, and B.R. Webber, J. High Energy Phys. JHEPFG 1029-8479 09 (2000) 004; 10.1088/1126-6708/2000/09/004
  • K. Kawagoe, M.M. Nojiri, and G. Polesello, Phys. Rev. D PRVDAQ 1550-7998 71, 035008 (2005); 10.1103/PhysRevD.71.035008
  • B.K. Gjelsten, D.J. Miller, and P. Osland, J. High Energy Phys. JHEPFG 1029-8479 12 (2004) 003; 10.1088/1126-6708/2004/12/003
  • D.J. Miller, P. Osland, and A.R. Raklev, J. High Energy Phys. JHEPFG 1029-8479 03 (2006) 034. 10.1088/1126-6708/2006/03/034

Similar publications



Contact ORBi