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Cited by 51

The DOI matches its Crossref record; 5 of the 5 references it cites were found in a registry or an index.

From stable to unstable anomaly-induced inflation

Netto, Tibério de Paula, Pelinson, Ana M., Shapiro, Ilya L., Starobinsky, Alexei A.·2016·The European Physical Journal C
DOI 10.1140/epjc/s10052-016-4390-4
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Crossref · 10.1140/epjc/s10052-016-4390-4

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Figures

Image 1
CC-BY · From the PDF
Image 2
CC-BY · From the PDF
Fig. 1 Numerical solution for the Hubble parameter H ( t ) in the units of Planck time τ ≡ t / tP for the MSM particle content and ˜ f = 10 -4
Fig. 1 Numerical solution for the Hubble parameter H ( t ) in the units of Planck time τ ≡ t / tP for the MSM particle content and ˜ f = 10 -4CC-BY · From the PDF
Fig. 2 The same case as in Fig. 1, but at larger scale. MSM and ˜ f = 10 -4
Fig. 2 The same case as in Fig. 1, but at larger scale. MSM and ˜ f = 10 -4CC-BY · From the PDF
Fig. 3 Numerical solution for the Hubble parameter H in units of Planck time τ ≡ t / tP for the photon case and ˜ f = 10 -4
Fig. 3 Numerical solution for the Hubble parameter H in units of Planck time τ ≡ t / tP for the photon case and ˜ f = 10 -4CC-BY · From the PDF
Fig. 4 Part of the plot from Figs. 1 and 2, but with much smaller scale in the H axis
Fig. 4 Part of the plot from Figs. 1 and 2, but with much smaller scale in the H axisCC-BY · From the PDF
Fig. 5 Phase diagram of Eq. (35) with MSSM particle content
Fig. 5 Phase diagram of Eq. (35) with MSSM particle contentCC-BY · From the PDF
Fig. 6 Phase diagram of Eq. (35) with MSM particle content
Fig. 6 Phase diagram of Eq. (35) with MSM particle contentCC-BY · From the PDF
Fig. 7 Integral curve corresponding to Eq. (37) and ˜ f = 10 -4 we find
Fig. 7 Integral curve corresponding to Eq. (37) and ˜ f = 10 -4 we findCC-BY · From the PDF
Fig. 8 Theplotof H ( t ) for the theory with one photon and a 4 = 5 × 10 8
Fig. 8 Theplotof H ( t ) for the theory with one photon and a 4 = 5 × 10 8CC-BY · From the PDF

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Citations

Cites

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Research works printed but not linked: 77

  1. I.L. Buchbinder, S.D. Odintsov, I.L. Shapiro, Effective Action in Quantum Gravity (IOP Publishing, Bristol, 1992)
  2. I.L. Shapiro, Class. Quant. Grav. 25, 103001 (2008). arXiv:0801.0216 · arXiv
  3. I.L. Shapiro, PoS-JHEP 03, 1 (2006). arXiv:hep-th/0610168 · arXiv
  4. M.J. Duff, Nucl. Phys. B 125, 334 (1977) · DOI · Paper page
  5. S. Deser, M.J. Duff, C. Isham, Nucl. Phys. B 111, 45 (1976) · DOI · Paper page
  6. Ya.B. Zeldovich, A.A. Starobinsky, Sov. Phys. JETP 34, 1159 (1972)
  7. L. Parker, S.A. Fulling, Phys. Rev. D 9, 341 (1974) · DOI · Paper page
  8. M.J. Duff, Class. Quant. Grav. 11, 1387 (1994). arXiv:hep-th/9308075 · arXiv
  9. P.C.W. Davies, Phys. Lett. D64, 402 (1977) · DOI
  10. M.V. Fischetti, J.B. Hartle, B.L. Hu, Phys. Rev. D 20, 1757 (1979) · DOI · Paper page
  11. A.A. Starobinsky, Nonsingular model of the universe with the quantum-gravitational de Sitter stage and its observational consequences. In: Proc. of the Second Seminar “Quantum Theory of Gravity” (Moscow, 13–15 October 1981) (INR Press, Moscow, 1982), pp. 58–72
  12. A. Vilenkin, Phys. Rev. D 32, 2511 (1985) · DOI
  13. P. Anderson, Phys. Rev. D 28, 271 (1983) · DOI · Paper page
  14. P. Anderson, Phys. Rev. D 29, 615 (1984) · DOI · Paper page
  15. P. Anderson, Phys. Rev. D 29, 1567 (1986) · DOI
  16. M.B. Mijić, M.S. Moris, W.-M. Suen, Phys. Rev. D 34, 2934 (1986) · DOI
  17. W.-M. Suen, P.R. Anderson, Phys. Rev. D 35, 2940 (1987) · DOI
  18. S.W. Hawking, T. Hertog, H.S. Real, Phys. Rev. D 63, 083504 (2001) · DOI · Paper page
  19. V.F. Mukhanov, G.V. Chibisov, JETP Lett. 33, 532 (1981)
  20. A.A. Starobinsky, JETP Lett. 34, 438 (1981)
  21. A.A. Starobinsky, Sov. Astron. Lett. 9, 302 (1983)
  22. A.A. Starobinsky, JETP Lett. 30, 682 (1979)
  23. R.J. Riegert, Phys. Lett. B 134, 56 (1980) · DOI
  24. E.S. Fradkin, A.A. Tseytlin, Phys. Lett. B 134, 187 (1980) · DOI
  25. I. Antoniadis, E. Mottola, Phys. Rev. D 45, 2013 (1992) · DOI
  26. I.L. Shapiro, A.G. Jacksenaev, Phys. Lett. B 324, 284 (1994) · DOI
  27. P.O. Mazur, E. Mottola, Phys. Rev. D 64, 104022 (2001). arXiv:hep-th/0106151 · DOI
  28. A.M. Polyakov, Phys. Lett. B 103, 207 (1981) · DOI · Paper page
  29. I.L. Buchbinder, S.D. Odintsov, I.L. Shapiro, Phys. Lett. B 162, 92 (1985) · DOI
  30. J.C. Fabris, A.M. Pelinson, I.L. Shapiro, Grav. Cosmol. 6, 59 (2000)
  31. J.C. Fabris, A.M. Pelinson, I.L. Shapiro, Nucl. Phys. B 597, 539 (2001) · DOI
  32. V. Müller, H.-J. Schmidt, A.A. Starobinsky, Phys. Lett. B 202, 198 (1988) · DOI
  33. I.L. Shapiro, Int. J. Mod. Phys. D 11, 1159 (2002). arXiv:hep-ph/0103128 · DOI
  34. T. Appelquist, J. Carazzone, Phys. Rev. D 11, 2856 (1975) · DOI
  35. E.V. Gorbar, I.L. Shapiro, J HEP 02, 021 (2003). arXiv:hep-ph/0210388 · DOI
  36. E.V. Gorbar, I.L. Shapiro, JHEP 06, 004 (2003). arXiv:hep-ph/0303124 · DOI
  37. I.L. Shapiro, J. Solà, Phys. Lett. B 530, 10 (2002) · DOI · Paper page
  38. A.M. Pelinson, I.L. Shapiro, F.I. Takakura, Nucl. Phys. B 648, 417 (2003). arXiv:hep-ph/0208184 · DOI · Paper page
  39. A.M. Pelinson, I.L. Shapiro, F.I. Takakura, Nucl. Phys. B (PS) 127, 182 (2004). arXiv:hep-ph/0311308 · DOI
  40. P.A.R. Ade et al., Planck 2015 Results. XIII. Cosmological Parameters. arXiv:1502.01589 · arXiv
  41. J.C. Fabris, A.M. Pelinson, F.O. Salles, I.L. Shapiro, JCAP 02, 019 (2012). arXiv:1112.5202 · arXiv
  42. F.O. de Salles, I.L. Shapiro, Phys. Rev. D 89, 084054 (2014). arXiv:1401.4583 · DOI
  43. M. Asorey, E.V. Gorbar, I.L. Shapiro, Class. Quant. Grav. 21, 163 (2003) · DOI
  44. S.M. Christensen, Phys. Rev. D 17, 946 (1978) · DOI · Paper page
  45. J.S. Dowker, R. Chritchley, Phys. Rev. D 16, 3390 (1976) · DOI · Paper page
  46. Z. Komargodski, A. Schwimmer, JHEP 1112, 099 (2011). arXiv:1107.3987 [hep-th] · DOI
  47. Z. Komargodski, JHEP 1207, 069 (2012). arXiv: 1112.4538 [hep-th] · arXiv
  48. M.A. Luty, J. Polchinski, R. Rattazzi, JHEP 1301, 152 (2013). arXiv: 1204.5221 [hep-th] · DOI
  49. A.M. Pelinson, I.L. Shapiro, Phys. Lett. B 694, 467 (2011). arXiv:1005.1313 · DOI
  50. S.G. Mamaev, V.M. Mostepanenko, Sov. Phys. JETP 51, 9 (1980)
  51. R.D. Peccei, J. Solà, C. Wetterich, Phys. Lett. B 195, 183 (1987) · DOI · Paper page
  52. A. Codello, G. D’Odorico, C. Pagani, R. Percacci, Class. Quant. Grav. 30, 115015 (2013). arXiv:1210.3284 · arXiv
  53. I.L. Shapiro, J. Solà, JHEP 02, 006 (2002) · DOI
  54. B.L. Nelson, P. Panangaden, Phys. Rev. D 25, 1019 (1982) · DOI
  55. I.L. Buchbinder, Theor. Math. Phys. 61, 393 (1984)
  56. D.J. Toms, Phys. Lett. B 126, 37 (1983) · DOI
  57. H.J. de Vega, N.G. Sanchez, Dark energy is the cosmological quantum vacuum energy of light particles. In: The Axion and the Lightest Neutrino. arXiv:astro-ph/0701212 · arXiv
  58. L.A. Kofman, A.D. Linde, A.A. Starobinsky, Phys. Lett. B 157, 361 (1985) · DOI
  59. S. Gottlöber, V. Müller, A.A. Starobinsky, Phys. Rev. D 43, 2510 (1991) · DOI
  60. Q.-G. Huang, JCAP 1402, 035 (2014). arXiv:1309.3514 · arXiv
  61. T. Asaka, S. Iso, H. Kawai, K. Kohri, T. Noumi, T. Terada, Reinterpretation of the Starobinsky Model. arXiv:1507.04344 · arXiv
  62. S.V. Ketov, A.A. Starobinsky, JCAP 1208, 022 (2012). arXiv:1203.0805 · arXiv
  63. I.L. Buchbinder, I.L. Shapiro, E.G. Yagunov, Mod. Phys. Lett. A 5, 1599 (1990) · DOI
  64. S.J. Hathrell, Ann. Phys. 139, 136 (1982) · DOI
  65. G. de Berredo-Peixoto, E.V. Gorbar, I.L. Shapiro, Class. Quant. Grav. 21, 2281 (2004). arXiv:hep-th/0311229 · arXiv
  66. M. Asorey, G. de Berredo-Peixoto, I.L. Shapiro, Phys. Rev. D 74, 124011 (2006). arXiv:hep-th/0609138 · DOI
  67. F.L. Bezrukov, M. Shaposhnikov, Phys. Lett. B 659, 703 (2008) · DOI
  68. A.O. Barvinsky, A. Yu, A.A. Kamenshchik, Starobinsky. JCAP 0811, 021 (2008). arXiv:0809.2104 · arXiv
  69. A.O. Barvinsky, A.Y. Kamenshchik, C. Kiefer, A.A. Starobinsky, C. Steinwachs, JCAP 0912, 003 (2009). arXiv:0904.1698 · arXiv
  70. A.O. Barvinsky, A.Y. Kamenshchik, C. Kiefer, A.A. Starobinsky, C. Steinwachs, Eur. Phys. J. C 72, 2219 (2012). arXiv:0910.1041 · DOI
  71. F.L. Bezrukov, M. Shaposhnikov, JHEP 0907, 089 (2009). arXiv:0904.1537 · arXiv
  72. F.L. Bezrukov, A. Magnin, M. Shaposhnikov, Phys. Lett. B 675, 88 (2009). arXiv:0812.4950 · DOI
  73. E.V. Gorbar, I.L. Shapiro, JHEP 0402, 060 (2004). arXiv:hep-ph/0311190 · DOI
  74. I.L. Shapiro, J. Solà, JHEP 0202, 006 (2002) · DOI
  75. I.L. Shapiro, J. Solà, Phys. Lett. B 682, 105 (2009) · DOI
  76. M. Maggiore, Dark Energy and Dimensional Transmutation in $${R}^{2}$$ R 2 Gravity. arXiv:1506.06217 · arXiv
  77. I.L. Shapiro, P.M. Teixeira, A. Wipf, Eur. Phys. J. C 75(6), 262 (2015). arXiv:1503.00874 · arXiv

Cited by

Metadata

Authors
Netto, T. D. P., Pelinson, A. M., Shapiro, I. L., & Starobinsky, A. A.
Venue
The European Physical Journal C
Publisher
Springer Science and Business Media LLC
Published
2016-10
Volume
76
Issue
10
ISSN
  • 1434-6044
  • 1434-6052
DOI
10.1140/epjc/s10052-016-4390-4
Cited by
51
References
5
Language
en
Licence
creativecommons.org/licenses/by/4.0 (unspecified)

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