R^2 dark matter
| dc.contributor.author | Ruiz Cembranos, José Alberto | |
| dc.date.accessioned | 2023-06-20T04:06:23Z | |
| dc.date.available | 2023-06-20T04:06:23Z | |
| dc.date.issued | 2011 | |
| dc.description | © 2011 IOP Publishing Ltd. International Workshop on the Dark Side of the Universe (6º. 2010. Guanajuato, México). I am grateful to K. Olive, M. Peloso, and M. Voloshin for useful discussions. DOE grant DOE/DE-FG02-94ER40823, FPA 2005-02327 project (DGICYT, Spain), CAM/UCM 910309 project, and MICINN Consolider-Ingenio MULTIDARK CSD2009-00064. | |
| dc.description.abstract | There is a non-trivial four-derivative extension of the gravitational spectrum that is free of ghosts and phenomenologically viable. It is the so called R^2-gravity since it is defined by the only addition of a term proportional to the square of the scalar curvature. Just the presence of this term does not improve the ultraviolet behaviour of Einstein gravity but introduces one additional scalar degree of freedom that can account for the dark matter of our Universe. | |
| dc.description.department | Depto. de Física Teórica | |
| dc.description.faculty | Fac. de Ciencias Físicas | |
| dc.description.refereed | TRUE | |
| dc.description.sponsorship | U. S. Department of Energy (DOE) | |
| dc.description.sponsorship | Dirección General de Investigación Científica y Técnica (DGICYT) MINECO, España | |
| dc.description.sponsorship | Programa Consolider-Ingenio MULTIDARK | |
| dc.description.sponsorship | Ministerio de Economía y Competitividad (MINECO), España | |
| dc.description.sponsorship | Ministerio de Ciencia e Innovación (MICINN), España | |
| dc.description.status | pub | |
| dc.eprint.id | https://eprints.ucm.es/id/eprint/35933 | |
| dc.identifier.doi | 10.1088/1742-6596/315/1/012004 | |
| dc.identifier.issn | 1742-6588 | |
| dc.identifier.officialurl | http://dx.doi.org/10.1088/1742-6596/315/1/012004 | |
| dc.identifier.relatedurl | http://iopscience.iop.org/ | |
| dc.identifier.uri | https://hdl.handle.net/20.500.14352/44919 | |
| dc.issue.number | 1 | |
| dc.journal.title | Journal of physics: Conference series | |
| dc.language.iso | eng | |
| dc.publisher | IOP Publishing | |
| dc.relation.projectID | DOE/DE-FG02-94ER40823 | |
| dc.relation.projectID | FPA 2005-02327 | |
| dc.relation.projectID | CAM/UCM 910309 | |
| dc.relation.projectID | CSD2009-00064 | |
| dc.relation.projectID | Universidad Complutense de Madrid (UCM) | |
| dc.relation.projectID | Comunidad Autónoma de Madrid (CAM) | |
| dc.rights | Atribución 3.0 España | |
| dc.rights.accessRights | open access | |
| dc.rights.uri | https://creativecommons.org/licenses/by/3.0/es/ | |
| dc.subject.cdu | 53 | |
| dc.subject.keyword | Cosmological models | |
| dc.subject.keyword | General-relativity | |
| dc.subject.keyword | Field-theory | |
| dc.subject.keyword | Gravity | |
| dc.subject.keyword | Consequences | |
| dc.subject.keyword | Inflation | |
| dc.subject.keyword | Geometry | |
| dc.subject.keyword | Relics | |
| dc.subject.ucm | Física (Física) | |
| dc.subject.unesco | 22 Física | |
| dc.title | R^2 dark matter | |
| dc.type | journal article | |
| dc.volume.number | 315 | |
| dcterms.references | [1] J. A. R. Cembranos, Phys. Rev. Lett. 102, 141301 (2009) [arXiv:0809.1653 [hep-ph]]. [2] P. Jordan, Nature (London) 164, 637 (1949); M. Fierz, Helv. Phys. Acta 29, 128 (1956); C. Brans and R. Dicke, Phys. Rev. 124, 925 (1961); P. G. Bergmann, Int. J. Theor. Phys. 1, 25 (1968); K. Nordtvedt, Astrophys. J. 161, 1059 (1970); R. Wagoner, Phys. Rev. D1, 3209 (1970); T. Damour and K. Nordtvedt, Phys. Rev. Lett. 70, 2217 (1993); ibid., Phys. Rev. D 48, 3436 (1993); T. Damour and B. Pichon, Phys. Rev. D 59, 123502 (1999) [astro-ph/9807176]; C. Schimd, J. P. Uzan, and A. Riazuelo, Phys. Rev. D 71, 083512 (2005); J. A. R. Cembranos, K. A. Olive, M. Peloso and J. P. Uzan, JCAP 0907, 025 (2009) [0905.1989 [astro-ph.CO]]; J. A. R. Cembranos, AIP Conf. Proc. 1182, 288 (2009) [arXiv:0906.5297 [astro-ph.CO]]; A. de la Cruz-Dombriz et al., Phys. Rev. D 74, 087501 (2006) [gr-qc/0607118]; Phys. Rev. D 77, 123515 (2008) [0802.2999 [astro-ph]]; A. Coc, K. A. Olive, J. P. Uzan and E. Vangioni, Phys. Rev. D 73, 083525 (2006) [astro-ph/0601299]; [0811.1845 [astro-ph]]. [3] E. Witten, Nucl. Phys. B 268, 253 (1986); V. A. Kostelecky and S. Samuel, Phys. Lett. B 207, 169 (1988); Nucl. Phys. B 336, 263 (1990); I. Y. Aref'eva, A. S. Koshelev, D. M. Belov and P. B. Medvedev, Nucl. Phys. B 638, 3 (2002) [arXiv:hep-th/0011117]; I. Y. Aref'eva, L. V. Joukovskaya and A. S. Koshelev, JHEP 0309, 012 (2003) [arXiv:hep-th/0301137]; M. Fujita and H. Hata, Phys. Rev. D 70, 086010 (2004) [arXiv:hep-th/0403031]; T. Biswas, J. A. R. Cembranos and J. I. Kapusta, Phys. Rev. Lett. 104, 021601 (2010) [arXiv:0910.2274 [hep-th]]; arXiv:1005.0430 [hep-th]; arXiv:1006.4098 [hep-th]. [4] K. S. Stelle, Phys. Rev. D 16, 953 (1977). [5] K. S. Stelle, Gen. Rel. Grav. 9, 353 (1978). [6] J. Z. Simon, Phys. Rev. D 45, 1953 (1992). [7] A. A. Starobinsky, Phys. Lett. B 91, 99 (1980). [8] S. Gottlober, V. Muller and A. A. Starobinsky, Phys. Rev. D 43, 2510 (1991). [9] J. A. R. Cembranos, Phys. Rev. D 73, 064029 (2006) [arXiv:gr-qc/0507039]. [10] J. Knodlseder et al., Astron. Astrophys. 441, 513 (2005) [arXiv:astro-ph/0506026]. [11] C. Picciotto and M. Pospelov, Phys. Lett. B 605, 15 (2005) [arXiv:hep-ph/0402178]; D. Hooper and L. T. Wang, Phys. Rev. D 70, 063506 (2004) [arXiv:hep-ph/0402220]; S. Kasuya and M. Kawasaki, Phys. Rev. D 73, 063007 (2006) [arXiv:astro-ph/0602296]; M. Pospelov and A. Ritz, Phys. Lett. B 651, 208 (2007) [arXiv:hep-ph/0703128]. [12] J. A. R. Cembranos and L. E. Strigari, Phys. Rev. D 77, 123519 (2008) [arXiv:0801.0630 [astro-ph]]. [13] J. F. Beacom and H. Yuksel, Phys. Rev. Lett. 97, 071102 (2006) [arXiv:astro-ph/0512411]. [14] J. A. R. Cembranos, J. L. Feng and L. E. Strigari, Phys. Rev. Lett. 99, 191301 (2007) [arXiv:0704.1658 [astro-ph]]. [15] L. Covi, J. E. Kim and L. Roszkowski, Phys. Rev. Lett. 82, 4180 (1999) [hep-ph/9905212]; J. L. Feng, A. Rajaraman and F. Takayama, Phys. Rev. D 68, 085018 (2003) [hep-ph/0307375]; J. L. Feng, A. Rajaraman and F. Takayama, Int. J. Mod. Phys. D 13, 2355 (2004) [hep-th/0405248]; J. A. R. Cembranos, J. L. Feng, A. Rajaraman and F. Takayama, Phys. Rev. Lett. 95, 181301 (2005) [hep-ph/0507150]; J. A. R. Cembranos, J. L. Feng, L E. Strigari, Phys. Rev. D 75, 036004 (2007) [hep-ph/0612157]; 0708.0247 [hep-ph]; 0708.0239[hep-ph]. [16] H. Goldberg, Phys. Rev. Lett. 50, 1419 (1983). [17] J. R. Ellis et al., Nucl. Phys. B 238, 453 (1984). [18] G. Servant and T. M. P. Tait, Nucl. Phys. B 650, 391 (2003) [hep-ph/0206071]. [19] H. C. Cheng, J. L. Feng and K. T. Matchev, Phys. Rev. Lett. 89, 211301 (2002) [hep-ph/0207125]. [20] J. A. R. Cembranos, A. Dobado and A. L. Maroto, Phys. Rev. Lett. 90, 241301 (2003) [hep-ph/0302041]; and Phys. Rev. D 68, 103505 (2003) [hep-ph/0307062]. [21] J. Alcaraz et al., Phys. Rev.D67, 075010 (2003) [hep-ph/0212269]; J. A. R. Cembranos, A. Dobado and A. L. Maroto, AIP Conf.Proc. 670, 235 (2003) [hep-ph/0301009]; hep-ph/0402142; hep-ph/0406076; Int. J. Mod. Phys. D13, 2275 (2004) [hep-ph/0405165]; hep-ph/0411076; astro-ph/0411262; Phys. Rev. D 73, 035008 (2006) [hep-ph/0510399]; astro-ph/0503622; astro-ph/0512569; astro-ph/0611911; A. L. Maroto, Phys. Rev. D 69, 043509 (2004) [hep-ph/0310272]; Phys. Rev. D 69, 101304 (2004) [hep-ph/0402278]; J. A. R. Cembranos et al., 0708.0235 [hep-ph]; JCAP 0810, 039 (2008) [0803.0694 [astro-ph]]; [22] T. E. Clark et al., Phys. Lett. B 671, 383 (2009) [0709.4023 [hep-th]]; Nucl. Phys. B 810, 97 (2009) [0809.1083 [hep-th]]. [23] P. Achard et al., Phys. Lett. B597, 145 (2004) [hep-ex/0407017]; S. Heinemeyer et al., hep-ph/0511332; J. A. R. Cembranos, A. Rajaraman and F. Takayama, hep-ph/0512020; Europhys. Lett. 82, 21001 (2008) [hep-ph/0609244]; J. A. R. Cembranos, A. Dobado and A. L. Maroto, hep-ph/0107155; Phys. Rev. D65 026005 (2002) [hep-ph/0106322]; hep-ph/0307015; Phys. Rev. D70, 096001 (2004) [hep-ph/0405286]; hep-ph/0512302; Phys. Rev. D 73, 057303 (2006) [hep-ph/0507066]; J. Phys. A 40, 6631 (2007) [hep-ph/0611024]; A. Juste et al., hep-ph/0601112; J. A. R. Cembranos et al., hep-ph/0603067; AIP Conf. Proc. 903, 591 (2007) [hep-ph/0701011]; ILC Collaboration, 0709.1893 [hep-ph]; 0712.1950 [physics.acc-ph]; 0712.2356 [physics.ins-det]; and T. E. Clark et al., Phys. Rev. D 78, 115004 (2008) [0809.3999 [hep-ph]]. | |
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