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Particle production from nonlocal gravitational effective action

dc.contributor.authorDobado González, Antonio
dc.contributor.authorLópez Maroto, Antonio
dc.date.accessioned2023-06-20T18:49:49Z
dc.date.available2023-06-20T18:49:49Z
dc.date.issued1999-11-15
dc.description©1999 The American Physical Society. A.L.M acknowledges support from SEUID-Royal Society. This work has been partially supported by Ministerio de Educación y Ciencia (Spain) CICYT (AEN96-1634).
dc.description.abstractIn this paper we show how the nonlocal effective action for gravity, obtained after integrating out the matter fields, can be used to compute particle production and spectra for different space-time metrics. Applying this technique to several examples, we End that the perturbative calculation of the effective action up to second order in curvatures yields exactly the same results for the total number of particles as the Bogolyubov transformations method, in the case of massless scaler fields propagating in a Robertson-Walker space-time. Using an adiabatic approximation we also obtain the corresponding spectra and compare the results with the traditional WKB approximation. [S0556-2821(99)02920-3].
dc.description.departmentDepto. de Física Teórica
dc.description.facultyFac. de Ciencias Físicas
dc.description.refereedTRUE
dc.description.sponsorshipMinisterio de Educación y Ciencia (Spain)
dc.description.sponsorshipCICYT
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/22709
dc.identifier.doi10.1103/PhysRevD.60.104045
dc.identifier.issn0556-2821
dc.identifier.officialurlhttp://prd.aps.org/abstract/PRD/v60/i10/e104045
dc.identifier.relatedurlhttp://prd.aps.org
dc.identifier.urihttps://hdl.handle.net/20.500.14352/58720
dc.issue.number10
dc.journal.titlePhysical Review D
dc.language.isoeng
dc.publisherAmerican Physical Society
dc.relation.projectIDAEN96-1634
dc.rights.accessRightsopen access
dc.subject.cdu53
dc.subject.keywordCovariant Perturbation-Theory
dc.subject.keywordLoop Effective Action
dc.subject.keywordEarly Universe
dc.subject.keywordInflation
dc.subject.keywordAnisotropy
dc.subject.keywordField
dc.subject.ucmFísica (Física)
dc.subject.unesco22 Física
dc.titleParticle production from nonlocal gravitational effective action
dc.typejournal article
dc.volume.number60
dcterms.references[1] L. Kofman, A. D. Linde, and A. A. Starobinsky, Phys. Rev. Lett. 73, 3195 (1994); Phys. Rev. D 56, 3258 (1997). [2] V. F. Mukhanov, H. A. Feldman, and R. H. Brandenberger, Phys. Rep. 215, 203 (1992); Y. Shtanov, J. Traschen, and R. Branderberger, Phys. Rev. D 51, 5438 (1995). [3] L. P. Grishchuk, Zh. Eksp. Teor. Fiz. 67, 825 (1975) [Sov. Phys. JETP 40, 409 (1975)]; L. P. Grishchuk, Ann. N.Y. Acad. Sci. 302, 439 (1977). [4] M. R. de Garcia Maia and J. D. Barrow, Phys. Rev. D 50, 6262 (1994). [5] N. D. Birrell and P. C. W. Davies, Quantum Fields in Curved Space (Cambridge University Press, Cambridge, England, 1982). [6] A. Dobado, A. Gómez-Nicola, A. L. Maroto, and J. R. Peláez, Effective Lagrangians for the Standard Model (Springer-Verlag, Berlin, 1997). [7] J. B. Hartle and B. L. Hu, Phys. Rev. D 20, 1772 (1979); 21, 2756 (1980). [8] J. Schwinger, Phys. Rev. 82, 664 (1951). [9] W. Heisenberg and H. Euler, Z. Phys. 98, 714 (1936). [10] L. Parker, in Recent Developments in Gravitation, Cargese 1978, edited by M. Le´vy and S. Deser (Plenum, New York, 1978). [11] S. Deser, M. J. Duff, and C. J. Isham, Nucl. Phys. B111, 45 (1976). [12] A. O. Barvinsky and G. A. Vilkovisky, Nucl. Phys. B282, 163 (1987); B333, 471 (1990); B333, 512 (1990); A. O. Barvinsky, Yu. V. Gusev, G. A. Vilkovisky, and V. V. Zhytnikov, ibid., B439, 561 (1995). [13]I. G. Avramidi, Nucl. Phys. B355, 712 (1991). [14] A. Dobado and A. L. Maroto, hep-th/9712198. [15] S. Weinberg, Gravitation and Cosmology (Wiley, New York, 1972). [16] L. Parker, Phys. Rev. Lett. 21, 562 (1968); Phys. Rev. 183, 1057 (1969); Asymptotic Structure of Space-Time, edited by F. P. Esposito and L. Witten (Plenum, New York, 1977). [17] L. Parker and A. Raval, Phys. Rev. D 57, 7327 (1998). [18] L. Parker, Nature (London) 261, 20 (1976). [19] Y. B. Zel’dovich and A. A. Starobinski, Pis’ma Zh. E ´ ksp. Teor. Fiz. 26, 373 (1977 [JETP Lett. 26, 252 (1977)]. [20] N. D. Birrell and P. C. W. Davies, J. Phys. A 13, 2109 (1980). [21] T. Damour, in Proceedings of the First Marcel Grossmann Meeting on General Relativity, edited by R. Ruffini (North-Holland, Amsterdam, 1977). [22] G. Scha¨fer, J. Phys. A 12, 2437 (1979). [23] E. Bre´zin and C. Itzykson, Phys. Rev. D 2, 1191 (1970). [24] A. G. Mirzabekian and G. A. Vilkovisky, Ann. Phys. (N.Y.) 270, 391 (1998).
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relation.isAuthorOfPublication.latestForDiscovery16523fad-99a9-422c-9a8e-c949ccffadec

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