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Volumn 81, Issue 6, 2010, Pages

Neutrino dark energy with more than one neutrino species

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EID: 77951271855     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.81.063001     Document Type: Article
Times cited : (5)

References (61)
  • 3
    • 34347334578 scopus 로고    scopus 로고
    • APJSA2 0067-0049 10.1086/513700
    • D.N. Spergel, Astrophys. J. Suppl. Ser. 170, 377 (2007). APJSA2 0067-0049 10.1086/513700
    • (2007) Astrophys. J. Suppl. Ser. , vol.170 , pp. 377
    • Spergel, D.N.1
  • 6
    • 0033147122 scopus 로고    scopus 로고
    • (Supernova Cosmology Project Collaboration), ASJOAB 0004-637X 10.1086/307221
    • S. Perlmutter (Supernova Cosmology Project Collaboration), Astrophys. J. 517, 565 (1999). ASJOAB 0004-637X 10.1086/307221
    • (1999) Astrophys. J. , vol.517 , pp. 565
    • Perlmutter, S.1
  • 8
    • 35348887272 scopus 로고    scopus 로고
    • ASJOAB 0004-637X 10.1086/518642
    • W.M. Wood-Vasey, Astrophys. J. ASJOAB 0004-637X 666, 694 (2007). 10.1086/518642
    • (2007) Astrophys. J. , vol.666 , pp. 694
    • Wood-Vasey, W.M.1
  • 9
    • 77951278624 scopus 로고    scopus 로고
    • arXiv:hep-ph/0010126.
    • P.Q. Hung, arXiv:hep-ph/0010126.
    • Hung, P.Q.1
  • 10
    • 0344011970 scopus 로고    scopus 로고
    • Dark energy and neutrino mass limits from baryogenesis
    • DOI 10.1103/PhysRevD.68.087301
    • P. Gu, X. Wang, and X. Zhang, Phys. Rev. D PRVDAQ 0556-2821 68, 087301 (2003). 10.1103/PhysRevD.68.087301 (Pubitemid 44628721)
    • (2003) Physical Review D , vol.68 , Issue.8 , pp. 087301
    • Gu, P.1    Wang, X.2    Zhang, X.3
  • 12
    • 84877998250 scopus 로고    scopus 로고
    • Neutrino models of dark energy
    • DOI 10.1103/PhysRevD.71.023527
    • R.D. Peccei, Phys. Rev. D PRVDAQ 1550-7998 71, 023527 (2005). 10.1103/PhysRevD.71.023527 (Pubitemid 44966561)
    • (2005) Physical Review D , vol.71 , Issue.2 , pp. 023527
    • Peccei, R.D.1
  • 13
    • 77951279838 scopus 로고    scopus 로고
    • arXiv:astro-ph/0611912.
    • L. Schrempp, arXiv:astro-ph/0611912.
    • Schrempp, L.1
  • 15
    • 19544373122 scopus 로고    scopus 로고
    • PRLTAO 0031-9007 10.1103/PhysRevLett.93.091801
    • D.B. Kaplan, A.E. Nelson, and N. Weiner, Phys. Rev. Lett. 93, 091801 (2004). PRLTAO 0031-9007 10.1103/PhysRevLett.93.091801
    • (2004) Phys. Rev. Lett. , vol.93 , pp. 091801
    • Kaplan, D.B.1    Nelson, A.E.2    Weiner, N.3
  • 16
    • 28844509572 scopus 로고    scopus 로고
    • Solar mass-varying neutrino oscillations
    • DOI 10.1103/PhysRevLett.95.211802, 211802
    • V. Barger, P. Huber, and D. Marfatia, Phys. Rev. Lett. 95, 211802 (2005). PRLTAO 0031-9007 10.1103/PhysRevLett.95.211802 (Pubitemid 41777037)
    • (2005) Physical Review Letters , vol.95 , Issue.21 , pp. 1-4
    • Barger, V.1    Huber, P.2    Marfatia, D.3
  • 17
    • 20744437774 scopus 로고    scopus 로고
    • Mass varying neutrinos in the Sun
    • DOI 10.1016/j.nuclphysb.2005.04.034, PII S0550321305003299
    • M. Cirelli, M.C. Gonzalez-Garcia, and C. Pena-Garay, Nucl. Phys. NUPBBO 0550-3213 B719, 219 (2005). 10.1016/j.nuclphysb.2005.04.034 (Pubitemid 40854765)
    • (2005) Nuclear Physics B , vol.719 , Issue.1-2 , pp. 219-233
    • Cirelli, M.1    Gonzalez-Garcia, M.C.2    Pena-Garay, C.3
  • 23
    • 33645760721 scopus 로고    scopus 로고
    • Cosmology of mass-varying neutrinos driven by quintessence: Theory and observations
    • DOI 10.1103/PhysRevD.73.083515
    • A.W. Brookfield, C. van de Bruck, D.F. Mota, and D. Tocchini-Valentini, Phys. Rev. D PRVDAQ 1550-7998 73, 083515 (2006). 10.1103/PhysRevD.73.083515 (Pubitemid 44642689)
    • (2006) Physical Review D , vol.73 , Issue.8 , pp. 083515
    • Brookfield, A.W.1    Van De Bruck, C.2    Mota, D.F.3    Tocchini-Valentini, D.4
  • 24
    • 84891648080 scopus 로고    scopus 로고
    • JHEPFG 1029-8479 10.1088/1126-6708/2006/05/021
    • R. Takahashi and M. Tanimoto, J. High Energy Phys. JHEPFG 1029-8479 05 (2006) 021. 10.1088/1126-6708/2006/05/021
    • J. High Energy Phys. , vol.2006 , Issue.5 , pp. 021
    • Takahashi, R.1    Tanimoto, M.2
  • 25
    • 77951268466 scopus 로고    scopus 로고
    • arXiv:astro-ph/0606034.
    • C. Spitzer, arXiv:astro-ph/0606034.
    • Spitzer, C.1
  • 26
    • 33645677262 scopus 로고    scopus 로고
    • JHEPFG 1029-8479 10.1088/1126-6708/2006/03/042
    • R. Fardon, A.E. Nelson, and N. Weiner, J. High Energy Phys. JHEPFG 1029-8479 03 (2006) 042. 10.1088/1126-6708/2006/03/042
    • J. High Energy Phys. , vol.2006 , Issue.3 , pp. 042
    • Fardon, R.1    Nelson, A.E.2    Weiner, N.3
  • 28
    • 42049088297 scopus 로고    scopus 로고
    • PRPLCM 0370-1573 10.1016/j.physrep.2007.12.004
    • M.C. Gonzalez-Garcia and M. Maltoni, Phys. Rep. 460, 1 (2008). PRPLCM 0370-1573 10.1016/j.physrep.2007.12.004
    • (2008) Phys. Rep. , vol.460 , pp. 1
    • Gonzalez-Garcia, M.C.1    Maltoni, M.2
  • 29
    • 47249108515 scopus 로고    scopus 로고
    • 1475-7516 10.1088/1475-7516/2008/06/005
    • K. Ichiki and Y.Y. Keum, J. Cosmol. Astropart. Phys. 1475-7516 06 (2008) 005. 10.1088/1475-7516/2008/06/005
    • J. Cosmol. Astropart. Phys. , vol.2008 , Issue.6 , pp. 005
    • Ichiki, K.1    Keum, Y.Y.2
  • 31
    • 34548446280 scopus 로고    scopus 로고
    • PYLBAJ 0370-2693 10.1016/j.physletb.2007.07.061
    • N. Kaloper, Phys. Lett. B 653, 109 (2007). PYLBAJ 0370-2693 10.1016/j.physletb.2007.07.061
    • (2007) Phys. Lett. B , vol.653 , pp. 109
    • Kaloper, N.1
  • 32
    • 48349141472 scopus 로고    scopus 로고
    • PRVDAQ 1550-7998 10.1103/PhysRevD.78.023015
    • L. Amendola, M. Baldi, and C. Wetterich, Phys. Rev. D PRVDAQ 1550-7998 78, 023015 (2008). 10.1103/PhysRevD.78.023015
    • (2008) Phys. Rev. D , vol.78 , pp. 023015
    • Amendola, L.1    Baldi, M.2    Wetterich, C.3
  • 33
    • 35348944408 scopus 로고    scopus 로고
    • PYLBAJ 0370-2693 10.1016/j.physletb.2007.08.060
    • C. Wetterich, Phys. Lett. B 655, 201 (2007). PYLBAJ 0370-2693 10.1016/j.physletb.2007.08.060
    • (2007) Phys. Lett. B , vol.655 , pp. 201
    • Wetterich, C.1
  • 34
    • 46349111093 scopus 로고    scopus 로고
    • NJOPFM 1367-2630 10.1088/1367-2630/10/3/033006
    • R. Bean, E.E. Flanagan, and M. Trodden, New J. Phys. 10, 033006 (2008). NJOPFM 1367-2630 10.1088/1367-2630/10/3/033006
    • (2008) New J. Phys. , vol.10 , pp. 033006
    • Bean, R.1    Flanagan, E.E.2    Trodden, M.3
  • 35
    • 47749092455 scopus 로고    scopus 로고
    • PRVDAQ 1550-7998 10.1103/PhysRevD.78.023009
    • R. Bean, E.E. Flanagan, and M. Trodden, Phys. Rev. D PRVDAQ 1550-7998 78, 023009 (2008). 10.1103/PhysRevD.78.023009
    • (2008) Phys. Rev. D , vol.78 , pp. 023009
    • Bean, R.1    Flanagan, E.E.2    Trodden, M.3
  • 36
    • 41049103067 scopus 로고    scopus 로고
    • PRVDAQ 1550-7998 10.1103/PhysRevD.77.045015
    • R. Takahashi and M. Tanimoto, Phys. Rev. D PRVDAQ 1550-7998 77, 045015 (2008). 10.1103/PhysRevD.77.045015
    • (2008) Phys. Rev. D , vol.77 , pp. 045015
    • Takahashi, R.1    Tanimoto, M.2
  • 37
    • 40149111521 scopus 로고    scopus 로고
    • PYLBAJ 0370-2693
    • P.H. Gu, Phys. Lett. B 661, 290 (2008). PYLBAJ 0370-2693
    • (2008) Phys. Lett. B , vol.661 , pp. 290
    • Gu, P.H.1
  • 38
  • 39
    • 46449130209 scopus 로고    scopus 로고
    • PYLBAJ 0370-2693 10.1016/j.physletb.2008.05.068
    • N. Brouzakis, N. Tetradis, and C. Wetterich, Phys. Lett. B 665, 131 (2008). PYLBAJ 0370-2693 10.1016/j.physletb.2008.05.068
    • (2008) Phys. Lett. B , vol.665 , pp. 131
    • Brouzakis, N.1    Tetradis, N.2    Wetterich, C.3
  • 40
    • 51749098777 scopus 로고    scopus 로고
    • PYLBAJ 0370-2693 10.1016/j.physletb.2008.03.059
    • J.R. Bhatt, P.H. Gu, U. Sarkar, and S.K. Singh, Phys. Lett. B 663, 83 (2008). PYLBAJ 0370-2693 10.1016/j.physletb.2008.03.059
    • (2008) Phys. Lett. B , vol.663 , pp. 83
    • Bhatt, J.R.1    Gu, P.H.2    Sarkar, U.3    Singh, S.K.4
  • 42
    • 43949095188 scopus 로고    scopus 로고
    • PRVDAQ 1550-7998 10.1103/PhysRevD.77.103003
    • V. Pettorino and C. Baccigalupi, Phys. Rev. D PRVDAQ 1550-7998 77, 103003 (2008). 10.1103/PhysRevD.77.103003
    • (2008) Phys. Rev. D , vol.77 , pp. 103003
    • Pettorino, V.1    Baccigalupi, C.2
  • 44
    • 41349101286 scopus 로고    scopus 로고
    • PYLBAJ 0370-2693 10.1016/j.physletb.2008.02.066
    • A.E. Bernardini and O. Bertolami, Phys. Lett. B 662, 97 (2008). PYLBAJ 0370-2693 10.1016/j.physletb.2008.02.066
    • (2008) Phys. Lett. B , vol.662 , pp. 97
    • Bernardini, A.E.1    Bertolami, O.2
  • 45
    • 77951291346 scopus 로고    scopus 로고
    • (unpublished).
    • L. Schrempp (unpublished).
    • Schrempp, L.1
  • 46
    • 41449097775 scopus 로고    scopus 로고
    • PRVDAQ 1550-7998 10.1103/PhysRevD.77.063515
    • P.P. Avelino, L.M.G. Beca, and C.J. Martins, Phys. Rev. D PRVDAQ 1550-7998 77, 063515 (2008). 10.1103/PhysRevD.77.063515
    • (2008) Phys. Rev. D , vol.77 , pp. 063515
    • Avelino, P.P.1    Beca, L.M.G.2    Martins, C.J.3
  • 47
    • 47249116993 scopus 로고    scopus 로고
    • JHEPFG 1029-8479 10.1088/1126-6708/2008/06/058
    • K. Ichiki and Y.Y. Keum, J. High Energy Phys. JHEPFG 1029-8479 06 (2008) 058. 10.1088/1126-6708/2008/06/058
    • J. High Energy Phys. , vol.2008 , Issue.6 , pp. 058
    • Ichiki, K.1    Keum, Y.Y.2
  • 50
    • 70049104399 scopus 로고    scopus 로고
    • PRVDAQ 1550-7998 10.1103/PhysRevD.80.045016
    • J.R. Bhatt and U. Sarkar, Phys. Rev. D PRVDAQ 1550-7998 80, 045016 (2009). 10.1103/PhysRevD.80.045016
    • (2009) Phys. Rev. D , vol.80 , pp. 045016
    • Bhatt, J.R.1    Sarkar, U.2
  • 51
    • 51849111490 scopus 로고    scopus 로고
    • PRVDAQ 1550-7998 10.1103/PhysRevD.78.064018For more information on the evolution of perturbations see.
    • B. Li, D.F. Mota, and D.J. Shaw, Phys. Rev. D PRVDAQ 1550-7998 78, 064018 (2008). 10.1103/PhysRevD.78.064018
    • (2008) Phys. Rev. D , vol.78 , pp. 064018
    • Li, B.1    Mota, D.F.2    Shaw, D.J.3
  • 53
    • 34247885874 scopus 로고    scopus 로고
    • PRVDAQ 1550-7998 10.1103/PhysRevD.75.103504Or scalar field potentials that resemble that of a cosmological constant-e.g. a very small fractional power-law.One could of course argue that a model with three scalar fields each coupled to one neutrino state would be a natural model to investigate, however, we are merely interested in a proof of concept here, so we stick to the simpler scenario with just one scalar field. In addition this is the standard assumption in the literature.Note that this assumption makes no difference qualitatively, a smaller coupling would only act to delay the instabilities slightly.
    • M. Kaplinghat and A. Rajaraman, Phys. Rev. D PRVDAQ 1550-7998 75, 103504 (2007). 10.1103/PhysRevD.75.103504
    • (2007) Phys. Rev. D , vol.75 , pp. 103504
    • Kaplinghat, M.1    Rajaraman, A.2
  • 54
    • 0008878002 scopus 로고    scopus 로고
    • A line-of-sight integration approach to cosmic microwave background anisotropies
    • DOI 10.1086/177793
    • U. Seljak and M. Zaldarriaga, Astrophys. J. 469, 437 (1996). ASJOAB 0004-637X 10.1086/177793 (Pubitemid 126132956)
    • (1996) Astrophysical Journal , vol.469 , Issue.NUMBER 1 , pp. 437-444
    • Seljak, U.1    Zaldarriaga, M.2
  • 55
    • 33744766990 scopus 로고
    • PRVDAQ 0556-2821 10.1103/PhysRevD.7.1888This definition has the advantage that the value of the coupling is determined by the VEV of the field itself, which means that there is no extra free parameter involved.
    • S.R. Coleman and E. Weinberg, Phys. Rev. D PRVDAQ 0556-2821 7, 1888 (1973). 10.1103/PhysRevD.7.1888
    • (1973) Phys. Rev. D , vol.7 , pp. 1888
    • Coleman, S.R.1    Weinberg, E.2
  • 56
    • 37649028663 scopus 로고    scopus 로고
    • Probing dark energy perturbations: The dark energy equation of state and speed of sound as measured by WMAP
    • DOI 10.1103/PhysRevD.69.083503
    • R. Bean and O. Dore, Phys. Rev. D PRVDAQ 0556-2821 69, 083503 (2004). 10.1103/PhysRevD.69.083503 (Pubitemid 44529433)
    • (2004) Physical Review D , vol.69 , Issue.8 , pp. 083503
    • Bean, R.1    Dore, O.2
  • 57
    • 33749159407 scopus 로고    scopus 로고
    • Constraints on the sound speed of dark energy
    • DOI 10.1103/PhysRevD.71.103519
    • S. Hannestad, Phys. Rev. D PRVDAQ 1550-7998 71, 103519 (2005). 10.1103/PhysRevD.71.103519 (Pubitemid 44643245)
    • (2005) Physical Review D , vol.71 , Issue.10 , pp. 103519
    • Hannestad, S.1
  • 58
    • 11944256794 scopus 로고
    • Cosmological perturbation theory in the synchronous and conformal newtonian gauges
    • DOI 10.1086/176550
    • C.-P. Ma and E. Bertschinger, Astrophys. J. ASJOAB 0004-637X 455, 7 (1995). 10.1086/176550 (Pubitemid 126000803)
    • (1995) Astrophysical Journal , vol.455 , Issue.NUMBER 1 , pp. 7-25
    • Ma, C.-P.1    Bertschinger, E.2
  • 59
    • 0037104545 scopus 로고    scopus 로고
    • Baryon bias and structure formation in an accelerating universe
    • DOI 10.1103/PhysRevD.66.043528
    • L. Amendola and D. Tocchini-Valentini, Phys. Rev. D PRVDAQ 0556-2821 66, 043528 (2002). 10.1103/PhysRevD.66.043528 (Pubitemid 44861164)
    • (2002) Physical Review D , vol.66 , Issue.4 , pp. 043528
    • Amendola, L.1    Tocchini-Valentini, D.2
  • 60
    • 33749158540 scopus 로고    scopus 로고
    • Growth of perturbations in dark matter coupled with quintessence
    • DOI 10.1103/PhysRevD.72.043516
    • T. Koivisto, Phys. Rev. D PRVDAQ 1550-7998 72, 043516 (2005). 10.1103/PhysRevD.72.043516 (Pubitemid 44654266)
    • (2005) Physical Review D , vol.72 , Issue.4 , pp. 043516
    • Koivisto, T.1
  • 61
    • 3042698418 scopus 로고    scopus 로고
    • PRVDAQ 0556-2821 10.1103/PhysRevD.69.103524
    • L. Amendola, Phys. Rev. D PRVDAQ 0556-2821 69, 103524 (2004). 10.1103/PhysRevD.69.103524
    • (2004) Phys. Rev. D , vol.69 , pp. 103524
    • Amendola, L.1


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