Dissipative effects in the effective field theory of inflation

Journal of High Energy Physics

Volumn 2012, Issue 1, 2012, Pages

  Nacir, Diana Ĺopez ^a   Porto, Rafael A ^b,c   Senatored, Leonardo ^d   Zaldarriaga, Matias ^b  

^a UNIVERSIDAD DE BUENOS AIRES   (Argentina)

^b INSTITUTE FOR ADVANCED STUDY   (United States)

^c Department of Earth and Environmental Sciences   (United States)

^d STANFORD UNIVERSITY   (United States)

Author keywords

Cosmology of Theories beyond the SM; Quantum Dissipative Systems; Space Time Symmetries

Indexed keywords

EID: 84857342081     PISSN: 11266708     EISSN: 10298479     Source Type: Journal    
DOI: 10.1007/JHEP01(2012)075     Document Type: Article

References (65)

1. I.Z. Rothstein, TASIlectures on effective field theories, hep-ph/0308266 [INSPIRE].
2. J. Polchinski, Effective field theory and the Fermi surface, hep-th/9210046 [INSPIRE].
3. W.D. Goldberger and I.Z. Rothstein, An effective field theory of gravity for extended objects, Phys. Rev. D 73 (2006) 104029 [hep-th/0409156] [INSPIRE].
4. R.A. Porto, Post-Newtonian corrections to the motion ofspinning bodies in NRGR, Phys. Rev. D 73 (2006) 104031 [gr-qc/0511061] [INSPIRE].
5. W.D. Goldberger and A. Ross, Gravitational radiative corrections from effective field theory, Phys. Rev. D 81 (2010) 124015 [arXiv:0912.4254] [INSPIRE].
6. R.A. Porto, A. Ross and I.Z. Rothstein, Spin induced multipole moments for the gravitational wavefluxfrom binary inspirals to third post-Newtonian order, JCAP 03 (2011) 009 [arXiv: 1007.1312] [INSPIRE].
7. R.A. Porto, Next to leading order spin-orbit effects in the motion of inspiralling compact binaries, Class. Quant. Grav. 27 (2010) 205001 [arXiv:1005.5730] [INSPIRE].
8. R.A. Porto and I.Z. Rothstein, Spin(1)Spin(2) effects in the motion of inspiralling compact binaries at third order in the post-Newtonian expansion, Phys. Rev. D 78 (2008) 044012 [Erratumibid. D 81 (2010) 029904] [arXiv:0802.0720] [INSPIRE].
9. R.A. Porto and I.Z. Rothstein, Next to leading order Spin(1)Spin(1) effects in the motion of inspiralling compact binaries, Phys. Rev. D 78 (2008) 044013 [Erratum ibid. D 81 (2010) 029905] [arXiv:0804.0260] [INSPIRE].
10. R.A. Porto and I.Z. Rothstein, The hyperfine Einstein-Infeld- Hoffmannpotential, Phys. Rev. Lett. 97 (2006) 021101 [gr-qc/0604099] [INSPIRE].
11. R.A. Porto and I.Z. Rothstein, Comment on 'on the next-to-leading order gravitational spin(1) - spin(2) dynamics' by J. Steinhoff et al, arXiv:0712.2032 [INSPIRE].
12. J.B. Gilmore and A. Ross, Effective field theory calculation ofsecond post-Newtonian binary dynamics, Phys. Rev. D 78 (2008) 124021 [arXiv:0810.1328] [INSPIRE].
13. S. Foffa and R. Sturani, Effective field theory calculation of conservative binary dynamics at thirdpost-Newtonian order, Phys. Rev. D 84 (2011) 044031 [arXiv:1104.1122] [INSPIRE].
14. W.D. Goldberger, Les Houches lectures on effective field theories and gravitational radiation hep-ph/0701129 [INSPIRE].
15. R.A. Porto and R. Sturani, Scalar gravity: post-Newtonian corrections via an effective field theory approach, gr-qc/0701105 [INSPIRE].
16. D. Baumann, A. Nicolis, L. Senatore and M. Zaldarriaga, Cosmological non-linearities as an effectivefluid, arXiv:1004.2488 [INSPIRE].
17. C. Cheung, P. Creminelli, A. Fitzpatrick, J. Kaplan and L. Senatore, The effective field theory ofinflation, JHEP 03 (2008) 014 [arXiv:0709.0293] [INSPIRE].
18. C. Cheung, A. Fitzpatrick, J. Kaplan and L. Senatore, On the consistency relation of the 3-pointfunction in single field inflation, JCAP 02 (2008) 021 [arXiv:0709.0295] [INSPIRE].
19. L. Senatore, K.M. Smith and M. Zaldarriaga, Non-Gaussianities in single field inflation and their optimal limits from the WMAP 5-year data, JCAP 01 (2010) 028 [arXiv:0905.3746] INSPIRE] .
20. L. Senatore and M. Zaldarriaga, On loops in inflation, JHEP 12 (2010) 008 [arXiv:0912.2734] [INSPIRE].
21. L. Senatore and M. Zaldarriaga, A naturally large four-point function in single field inflation JCAP 01 (2011) 003 [arXiv:1004.1201] [INSPIRE].
22. P. Creminelli, M.A. Luty, A. Nicolis and L. Senatore, Starting the universe: stable violation of the null energy condition and non-standard cosmologies, JHEP 12 (2006) 080 [hep-th/0606090] [INSPIRE].
23. N. Bartolo, M. Fasiello, S. Matarrese and A. Riotto, Large non-gaussianities in the effective field theory approach to single-field inflation: the bispectrum, JCAP 08 (2010) 008 [arXiv: 1004. 0893] [INSPIRE] .
24. N. Bartolo, M. Fasiello, S. Matarrese and A. Riotto, Large non-gaussianities in the effective field theory approach to single-field inflation: the trispectrum, JCAP 09 (2010) 035 [arXiv:1006.5411] [INSPIRE].
25. D. Baumann and D. Green, Equilateral non- Gaussianity and new physics on the horizon JCAP 09 (2011) 014 [arXiv:1102.5343] [INSPIRE].
26. D. Baumann, L. Senatore and M. Zaldarriaga, Scale-Invariance and the strong coupling problem, JCAP 05 (2011) 004 [arXiv:1101.3320] [INSPIRE].
27. D. Baumann and D. Green, Signatures ofsupersymmetryfrom the early universe, arXiv:1109.0292 [INSPIRE].
28. M.E. Peskin and D.V. Schroeder, An introduction to quantum field theory, Addison-Wesleay Reading U.S.A. (1995).
29. J. Distler, B. Grinstein, R.A. Porto and I.Z. Rothstein, Falsifying models of new physics via WW scattering, Phys. Rev. Lett. 98 (2007) 041601 [hep-ph/0604255] [INSPIRE].
30. L. Senatore and M. Zaldarriaga, The effective field theory of multifield inflation arXiv:1009.2093 [INSPIRE].
31. D. Green, B. Horn, L. Senatore and E. Silverstein, Trapped inflation Phys. Rev. D 80 (2009) 063533 [arXiv:0902.1006] [INSPIRE].
32. L. Kofman, A.D. Linde, X. Liu, A. Maloney, L. McAllister, et al., Beauty is attractive: moduli trapping at enhanced symmetrypoints, JHEP 05 (2004) 030 [hep-th/0403001] [INSPIRE].
33. E. Calzetta and B.L. Hu, Nonequilibrium quantum field theory, Cambridge University Press, Cambridge U.K. (2008).
34. W.D. Goldberger and I.Z. Rothstein, Dissipative effects in the worldline approach to black hole dynamics, Phys. Rev. D 73 (2006) 104030 [hep-th/0511133] [INSPIRE].
35. R.A. Porto, Absorption effects due to spin in the worldline approach to black hole dynamics, Phys. Rev. D 77 (2008) 064026 [arXiv:0710.5150] [INSPIRE].
36. S. Endlich, A. Nicolis, R.A. Porto and J. Wang, Dissipative effects in the effective field theory for hydrodynamics, work in progress.
37. S. Endlich, A. Nicolis, R. Rattazzi and J. Wang, The quantum mechanics ofperfectfluids, JHEP 04 (2011) 102 [arXiv:1011.6396] [INSPIRE].
38. S. Dubovsky L. Hui, A. Nicolis and D.T. Son, Effective field theory for hydrodynamics: thermodynamics and the derivative expansion, arXiv:1107.0731 [INSPIRE].
39. A. Berera, Warm inflation, Phys. Rev. Lett. 75 (1995) 3218 [astro-ph/9509049] [INSPIRE].
40. A. Berera, Thermalproperties of an inflationary universe, Phys. Rev. D 54 (1996) 2519 [hep-th/9601134] [INSPIRE].
41. A. Berera and L.-Z. Fang, Thermally induced density perturbations in the inflation era, Phys. Rev. Lett. 74 (1995) 1912 [astro-ph/9501024] [INSPIRE].
42. A. Berera, The warm inflationary universe, Contemp. Phys. 47 (2006) 33 [arXiv:0809.4198] [INSPIRE].
43. A. Berera, I.G. Moss and R.O. Ramos, Warm inflation and its microphysical basis, Rept. Prog. Phys. 72 (2009) 026901 [arXiv:0808.1855] [INSPIRE].
44. M. Bastero-Gil and A. Berera, Warm inflation model building, Int. J. Mod. Phys. A 24 (2009) 2207 [arXiv:0902.0521] [INSPIRE].
45. U. Weiss, Quantum dissipative systems, World Scientific, Singapore (2008).
46. Y. Zhang, Path-integral formalism for classical Brownian motion in a general environment, Phys. Rev. E 47 (1993) 3745.
47. A.L. Fetter and J.D. Walecka, Quantum theory ofmany-particle systems, McGraw-Hill, San Francisco U.S.A. (1971).
48. C.R. Galley and M. Tiglio, Radiation reaction and gravitational waves in the effective field theory approach, Phys. Rev. D 79 (2009) 124027 [arXiv:0903.1122] [INSPIRE].
49. C.R. Galley, A.K. Leibovich and I.Z. Rothstein, Finite size corrections to the radiation reactionforce in classical electrodynamics, arXiv:1005.2617 [INSPIRE].
50. M. Favata, The gravitational-wave memory effect, Class. Quant. Grav. 27 (2010) 084036 [arXiv: 1003. 3486] [INSPIRE] .
51. F. Di Marco, F. Finelli and R. Brandenberger, Adiabatic and isocurvature perturbations for multifield generalized Einstein models, Phys. Rev. D 67 (2003) 063512 [astro-ph/0211276] [INSPIRE] .
52. WMAP collaboration, E. Komatsu et al., Seven-year Wilkinson microwave anisotropy probe (WMAP) observations: cosmological interpretation, Astrophys. J. Suppl. 192 (2011) 18 [arXiv :1001.4538] [INSPIRE] .
53. P. Creminelli and M. Zaldarriaga, Single field consistency relation for the 3-point function JCAP 10 (2004) 006 [astro-ph/0407059] [INSPIRE].
54. P. Creminelli, G. D'Amico, M. Musso and J. Norena, The (not so) squeezed limit of the primordial 3-point function, JCAP 11 (2011) 038 [arXiv:1106.1462] [INSPIRE].
55. C. Graham and I.G. Moss, Density fluctuations from warm inflation, JCAP 07 (2009) 013 [arXiv:0905.3500] [INSPIRE].
56. M. Bastero-Gil, A. Berera and R. Ramos, Shear viscous effects on the primordial power spectrumfrom warm inflation, JCAP 07 (2011) 030 [arXiv:1106.0701] [INSPIRE].
57. I.G. Moss and C.M. Graham, Particle production and reheating in the inflationary universe, Phys. Rev. D 78 (2008) 123526 [arXiv:0810.2039] [INSPIRE].
58. M. Bastero-Gil and A. Berera, Warm inflation dynamics in the low temperature regime, Phys. Rev. D 76 (2007) 043515 [hep-ph/0610343] [INSPIRE].
59. J.C. Bueno Sanchez, M. Bastero-Gil, A. Berera and K. Dimopoulos, Warm hilltop inflation, Phys. Rev. D 77 (2008) 123527 [arXiv:0802.4354] [INSPIRE].
60. J. Yokoyama and A.D. Linde, Is warm inflation possible?, Phys. Rev. D 60 (1999) 083509 [hep-ph/9809409] [INSPIRE].
61. L.M.H. Hall and I.G. Moss, Thermal effects on pure and hybrid inflation, Phys. Rev. D 71 (2005) 023514 [hep-ph/0408323] [INSPIRE].
62. S. Gupta, A. Berera, A. Heavens and S. Matarrese, Non-Gaussian signatures in the cosmic background radiation from warm inflation, Phys. Rev. D 66 (2002) 043510 [astro-ph/0205152] [INSPIRE].
63. L. Senatore, E. Silverstein and M. Zaldarriaga, New sources of gravitational waves during inflation, arXiv:1109.0542 [INSPIRE].
64. D. Forster, Hydrodynamics, fluctuations, broken symmetry, and correlation functions, Perseus books, New York U.S.A. (1975).
65. S. Weinberg, Cosmology, Oxford University Press, Oxford U.K. (2008).