宇宙暴脹 (Chinese Wikipedia)

Analysis of information sources in references of the Wikipedia article "宇宙暴脹" in Chinese language version.

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archive.org

Barbara Sue Ryden. Introduction to cosmology. Addison-Wesley. 2003. ISBN 978-0-8053-8912-8.
Misner, Charles W.; Coley, A A; Ellis, G F R; Hancock, M. The isotropy of the universe. Astrophysical Journal. 1968, 151 (2): 431. Bibcode:1998CQGra..15..331W. doi:10.1088/0264-9381/15/2/008.
Misner, Charles; Thorne, Kip S. and Wheeler, John Archibald. Gravitation. San Francisco: W. H. Freeman. 1973: 489–490, 525–526. ISBN 0-7167-0344-0.
R. C. Tolman. Relativity, Thermodynamics, and Cosmology. Oxford: Clarendon Press. 1934. ISBN 0-486-65383-8. LCCN 34032023. Reissued (1987) New York: Dover ISBN 0-486-65383-8.
Dicke, Robert H. Gravitation and the Universe. Philadelphia: American Philosopical Society. 1970.
Phillip James Edwin Peebles. Principles of Physical Cosmology. Princeton University Press. 1993. ISBN 0-691-01933-9.
Martin, Rees. Before the Beginning. 1998: 185. ISBN 0-201-15142-1. Skeptics about exotic physics might not be hugely impressed by a theoretical argument to explain the absence of particles that are themselves only hypothetical. Preventive medicine can readily seem 100 percent effective against a disease that doesn't exist!
Linde, Andrei. Lectures on Inflationary Cosmology. 1994-10-12. arXiv:hep-th/9410082 .
J.B. Hartle. Gravity: An Introduction to Einstein's General Relativity 1st. Addison Wesley. 2003: 411. ISBN 0-8053-8662-9.
Guth, Alan. The Inflationary Universe. Addison–Wesley. 1997. ISBN 0-201-14942-7.
Carroll, Sean M.; Jennifer Chen. Spontaneous inflation and the origin of the arrow of time. 2004. Bibcode:2004hep.th...10270C. arXiv:hep-th/0410270  |class=被忽略 (帮助).
Earman, John; Mosterín, Jesús. A Critical Look at Inflationary Cosmology. Philosophy of Science. March 1999, 66: 1–49. JSTOR 188736. doi:10.2307/188736 (不活跃 2014-03-25).

archive.today

見：Lyth, David H. What would we learn by detecting a gravitational wave signal in the cosmic microwave background anisotropy?. Physical Review Letters. 1997, 78 (10): 1861–3 [2020-10-06]. Bibcode:1997PhRvL..78.1861L. arXiv:hep-ph/9606387 . doi:10.1103/PhysRevLett.78.1861. （原始内容存档于2012-06-29）.

arxiv.org

這是因為暴脹勢可以寫作φ/m_Pl的泰勒級數，其中φ為暴脹場，m_Pl為普朗克質量。對於單單一個項，比如質量項m_φ⁴(φ/m_Pl)²，慢滾條件在φ比m_Pl大很多的情況下得到滿足。有效場論就是這種情況，高階項會使暴脹的條件不再得到滿足。這些高階項不存在，也可以看做是一種微調。見：Alabidi, Laila; Lyth, David H. Inflation models and observation. JCAP. 2006, 0605 (5): 016. Bibcode:2006JCAP...05..016A. arXiv:astro-ph/0510441 . doi:10.1088/1475-7516/2006/05/016.
Andrew, Liddle, An introduction to cosmological inflation, 1998 [2014-06-03], （原始内容存档于2014-10-20） |booktitle=被忽略 (帮助)
Tsujikawa, Shinji. Introductory review of cosmic inflation. ArXiv.or. 28 Apr 2003 [2014-06-03]. （原始内容存档于2015-03-26）.
Ade, P. A. R.; Aikin, R. W.; Barkats, D.; Benton, S. J.; Bischoff, C. A.; Bock, J. J.; Brevik, J. A.; Buder, I.; Bullock, E.; Dowell, C. D.; Duband, L.; Filippini, J. P.; Fliescher, S.; Golwala, S. R.; Halpern, M.; Hasselfield, M.; Hildebrandt, S. R.; Hilton, G. C.; Hristov, V. V.; Irwin, K. D.; Karkare, K. S.; Kaufman, J. P.; Keating, B. G.; Kernasovskiy, S. A.; Kovac, J. M.; Kuo, C. L.; Leitch, E. M.; Lueker, M.; Mason, P.; Netterfield, C. B.; Nguyen, H. T.; O'Brient, R.; Ogburn, R. W. IV; Orlando, A.; Pryke, C.; Reintsema, C. D.; Richter, S.; Schwartz, R.; Sheehy, C. D.; Staniszewski, Z. K.; Sudiwala, R. W.; Teply, G. P.; Tolan, J. E.; Turner, A. D.; Vieregg, A. G.; Wong, C. L.; Yoon, K. W. BICEP2 I: Detection of B-mode Polarization at Degree Angular Scales (PDF). 17 March 2014 [2014年4月2日]. arXiv:1403.3985 . （原始内容 (PDF)存档于2014年3月17日）.
Ade, P.A.R. et al (BICEP2 Collaboration). Detection of B-Mode Polarization at Degree Angular Scales by BICEP2. Physical Review Letters. 19 June 2014, 112: 241101. arXiv:1403.3985 . doi:10.1103/PhysRevLett.112.241101.
Planck Collaboration Team. Planck intermediate results. XXX. The angular power spectrum of polarized dust emission at intermediate and high Galactic latitudes. ArXiv. 19 September 2014 [22 September 2014]. arXiv:1409.5738 . （原始内容存档于2019-05-02）.
Luis Gonzalez-Mestres. Space, Time and Superluminal Particles. 24 February 1997 [2014-04-02]. （原始内容存档于2013-10-29）.
Kofman, Lev; Linde, Andrei; Starobinsky, Alexei. Reheating after inflation. Physical Review Letters. 1994, 73 (5): 3195–3198. Bibcode:1986CQGra...3..811K. arXiv:hep-th/9405187 . doi:10.1088/0264-9381/3/5/011.
See, e.g. Yao, W.–M.; Amsler, C.; Asner, D.; Barnett, R. M.; Beringer, J.; Burchat, P. R.; Carone, C. D.; Caso, C.; Dahl, O.; d'Ambrosio, G.; De Gouvea, A.; Doser, M.; Eidelman, S.; Feng, J. L.; Gherghetta, T.; Goodman, M.; Grab, C.; Groom, D. E.; Gurtu, A.; Hagiwara, K.; Hayes, K. G.; Hernández-Rey, J. J.; Hikasa, K.; Jawahery, H.; Kolda, C.; Kwon, Y.; Mangano, M. L.; Manohar, A. V.; Masoni, A.; et al. Review of Particle Physics. J. Phys. G. 2006, 33 (1): 1 [2014-06-03]. Bibcode:2006JPhG...33....1Y. arXiv:astro-ph/0601168 . doi:10.1088/0954-3899/33/1/001. （原始内容存档于2017-09-07）.
Linde, Andrei. Lectures on Inflationary Cosmology. 1994-10-12. arXiv:hep-th/9410082 .
Tegmark, M.; et al. Cosmological constraints from the SDSS luminous red galaxies. Physical Review D. August 2006, 74 (12): 123507. Bibcode:2006PhRvD..74l3507T. arXiv:astro-ph/0608632 . doi:10.1103/PhysRevD.74.123507.
Boyle, Latham A.; Steinhardt, PJ; Turok, N. Inflationary predictions for scalar and tensor fluctuations reconsidered. Physical Review Letters. 2006, 96 (11): 111301. Bibcode:2006PhRvL..96k1301B. PMID 16605810. arXiv:astro-ph/0507455 . doi:10.1103/PhysRevLett.96.111301.
Tegmark, Max. What does inflation really predict?. JCAP. 2005, 0504 (4): 001. Bibcode:2005JCAP...04..001T. arXiv:astro-ph/0410281 . doi:10.1088/1475-7516/2005/04/001.
Komatsu, E.; Smith, K. M.; Dunkley, J.; Bennett, C. L.; Gold, B.; Hinshaw, G.; Jarosik, N.; Larson, D.; Nolta, M. R.; Page, L.; Spergel, D. N.; Halpern, M.; Hill, R. S.; Kogut, A.; Limon, M.; Meyer, S. S.; Odegard, N.; Tucker, G. S.; Weiland, J. L.; Wollack, E.; Wright, E. L. Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation. The Astrophysical Journal Supplement Series. January 2010, 192 (2): 18. Bibcode:2011ApJS..192...18K. arXiv:1001.4538 . doi:10.1088/0067-0049/192/2/18.
Spergel, D. N.; et al. First year Wilkinson Microwave Anisotropy Probe (WMAP) observations: determination of cosmological parameters. Astrophysical Journal Supplement Series. 2003, 148 (1): 175–194. Bibcode:2003ApJS..148..175S. arXiv:astro-ph/0302209 . doi:10.1086/377226.
Loeb, A.; Zaldarriaga, M. Measuring the small-scale power spectrum of cosmic density fluctuations through 21 cm tomography prior to the epoch of structure formation. Physical Review Letters. 2004, 92 (21): 211301. Bibcode:2004PhRvL..92u1301L. PMID 15245272. arXiv:astro-ph/0312134 . doi:10.1103/PhysRevLett.92.211301.
見：Lyth, David H. What would we learn by detecting a gravitational wave signal in the cosmic microwave background anisotropy?. Physical Review Letters. 1997, 78 (10): 1861–3 [2020-10-06]. Bibcode:1997PhRvL..78.1861L. arXiv:hep-ph/9606387 . doi:10.1103/PhysRevLett.78.1861. （原始内容存档于2012-06-29）.
Brandenberger, Robert H. Challenges for inflationary cosmology. 10th International Symposium on Particles, Strings and Cosmology. November 2004. arXiv:astro-ph/0411671 .
A. Borde, A. Guth and A. Vilenkin. Inflationary space-times are incomplete in past directions. Physical Review Letters. 2003, 90 (15): 151301. Bibcode:2003PhRvL..90o1301B. PMID 12732026. arXiv:gr-qc/0110012 . doi:10.1103/PhysRevLett.90.151301.
A. Borde and A. Vilenkin. Eternal inflation and the initial singularity. Physical Review Letters. 1994, 72 (21): 3305–9. Bibcode:1994PhRvL..72.3305B. arXiv:gr-qc/9312022 . doi:10.1103/PhysRevLett.72.3305.
Carroll, Sean M.; Chen, Jennifer. Does inflation provide natural initial conditions for the universe?. Gen. Rel. Grav. 2005, 37 (10): 1671–4. Bibcode:2005GReGr..37.1671C. arXiv:gr-qc/0505037 . doi:10.1007/s10714-005-0148-2.
Carroll, Sean M.; Jennifer Chen. Spontaneous inflation and the origin of the arrow of time. 2004. Bibcode:2004hep.th...10270C. arXiv:hep-th/0410270  |class=被忽略 (帮助).
Aguirre, Anthony; Gratton, Steven. Inflation without a beginning: A null boundary proposal. Physical Review D. 2003, 67 (8): 083515. Bibcode:2003PhRvD..67h3515A. arXiv:gr-qc/0301042 . doi:10.1103/PhysRevD.67.083515.
Aguirre, Anthony; Gratton, Steven. Steady-State Eternal Inflation. Physical Review D. 2002, 65 (8): 083507. Bibcode:2002PhRvD..65h3507A. arXiv:astro-ph/0111191 . doi:10.1103/PhysRevD.65.083507.
Albrecht, Andreas; Sorbo, Lorenzo. Can the universe afford inflation?. Physical Review D. 2004, 70 (6): 063528. Bibcode:2004PhRvD..70f3528A. arXiv:hep-th/0405270 . doi:10.1103/PhysRevD.70.063528.
Martin, Jerome; Brandenberger, Robert. The trans-Planckian problem of inflationary cosmology. Physical Review D. 2001, 63 (12): 123501. Bibcode:2001PhRvD..63l3501M. arXiv:hep-th/0005209 . doi:10.1103/PhysRevD.63.123501.
Martin, Jerome; Ringeval, Christophe. Superimposed Oscillations in the WMAP Data?. Physical Review D. 2004, 69 (8): 083515. Bibcode:2004PhRvD..69h3515M. arXiv:astro-ph/0310382 . doi:10.1103/PhysRevD.69.083515.
Robert H. Brandenberger, "A Status Review of Inflationary Cosmology", proceedings Journal-ref: BROWN-HET-1256 (2001), (available from
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Kachru, Shamit; Kallosh, Renata; Linde, Andrei; Maldacena, Juan; McAllister, Liam; Trivedi, Sandip P. Towards inflation in string theory. JCAP. 2003, 0310 (10): 013. Bibcode:2003JCAP...10..013K. arXiv:hep-th/0308055 . doi:10.1088/1475-7516/2003/10/013.
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uk.arxiv.org

Planck Collaboration Team. Planck intermediate results. XXX. The angular power spectrum of polarized dust emission at intermediate and high Galactic latitudes. ArXiv. 19 September 2014 [22 September 2014]. arXiv:1409.5738 . （原始内容存档于2019-05-02）.

bbc.com

Amos, Jonathan. Cosmic inflation: Confidence lowered for Big Bang signal. BBC News. 19 June 2014 [20 June 2014]. （原始内容存档于2014-06-21）.

bicepkeck.org

Staff. BICEP2 2014 Results Release. National Science Foundation. 17 March 2014 [18 March 2014]. （原始内容存档于2018-09-28）.
Ade, P. A. R.; Aikin, R. W.; Barkats, D.; Benton, S. J.; Bischoff, C. A.; Bock, J. J.; Brevik, J. A.; Buder, I.; Bullock, E.; Dowell, C. D.; Duband, L.; Filippini, J. P.; Fliescher, S.; Golwala, S. R.; Halpern, M.; Hasselfield, M.; Hildebrandt, S. R.; Hilton, G. C.; Hristov, V. V.; Irwin, K. D.; Karkare, K. S.; Kaufman, J. P.; Keating, B. G.; Kernasovskiy, S. A.; Kovac, J. M.; Kuo, C. L.; Leitch, E. M.; Lueker, M.; Mason, P.; Netterfield, C. B.; Nguyen, H. T.; O'Brient, R.; Ogburn, R. W. IV; Orlando, A.; Pryke, C.; Reintsema, C. D.; Richter, S.; Schwartz, R.; Sheehy, C. D.; Staniszewski, Z. K.; Sudiwala, R. W.; Teply, G. P.; Tolan, J. E.; Turner, A. D.; Vieregg, A. G.; Wong, C. L.; Yoon, K. W. BICEP2 I: Detection of B-mode Polarization at Degree Angular Scales (PDF). 17 March 2014 [2014年4月2日]. arXiv:1403.3985 . （原始内容 (PDF)存档于2014年3月17日）.

books.google.com

Guth, Alan H. The Inflationary Universe: The Quest for a New Theory of Cosmic Origins. Basic Books. 1997: 233–234 [2014-04-02]. ISBN 0201328402. （原始内容存档于2014-04-05）.

cam.ac.uk

damtp.cam.ac.uk

Shellard, Paul. The Four Pillars of the Standard Cosmology. Cambridge Cosmology: Hot Big Bang. University of Cambridge. [May 28, 2014]. （原始内容存档于2014-03-17）.

doi.org

這是因為暴脹勢可以寫作φ/m_Pl的泰勒級數，其中φ為暴脹場，m_Pl為普朗克質量。對於單單一個項，比如質量項m_φ⁴(φ/m_Pl)²，慢滾條件在φ比m_Pl大很多的情況下得到滿足。有效場論就是這種情況，高階項會使暴脹的條件不再得到滿足。這些高階項不存在，也可以看做是一種微調。見：Alabidi, Laila; Lyth, David H. Inflation models and observation. JCAP. 2006, 0605 (5): 016. Bibcode:2006JCAP...05..016A. arXiv:astro-ph/0510441 . doi:10.1088/1475-7516/2006/05/016.
Ade, P.A.R. et al (BICEP2 Collaboration). Detection of B-Mode Polarization at Degree Angular Scales by BICEP2. Physical Review Letters. 19 June 2014, 112: 241101. arXiv:1403.3985 . doi:10.1103/PhysRevLett.112.241101.
Kofman, Lev; Linde, Andrei; Starobinsky, Alexei. Reheating after inflation. Physical Review Letters. 1994, 73 (5): 3195–3198. Bibcode:1986CQGra...3..811K. arXiv:hep-th/9405187 . doi:10.1088/0264-9381/3/5/011.
Misner, Charles W.; Coley, A A; Ellis, G F R; Hancock, M. The isotropy of the universe. Astrophysical Journal. 1968, 151 (2): 431. Bibcode:1998CQGra..15..331W. doi:10.1088/0264-9381/15/2/008.
Misner, Charles W.; Leach, P G L. Mixmaster universe. Physical Review Letters. 1969, 22 (15): 1071–74. Bibcode:2008JPhA...41o5201A. doi:10.1088/1751-8113/41/15/155201.
't Hooft, Gerard. Magnetic monopoles in Unified Gauge Theories. Nuclear Physics B. 1974, 79 (2): 276–84. Bibcode:1974NuPhB..79..276T. doi:10.1016/0550-3213(74)90486-6.
Guth, Alan; Tye, S. Phase Transitions and Magnetic Monopole Production in the Very Early Universe. Physical Review Letters. 1980, 44 (10): 631–635; Erratum ibid.,44:963, 1980. Bibcode:1980PhRvL..44..631G. doi:10.1103/PhysRevLett.44.631.
Einhorn, Martin B; Stein, D. L.; Toussaint, Doug. Are Grand Unified Theories Compatible with Standard Cosmology?. Physical Review D. 1980, 21 (12): 3295–3298. Bibcode:1980PhRvD..21.3295E. doi:10.1103/PhysRevD.21.3295.
Zel'dovich, Ya.; Khlopov; M. Yu. Khlopov. On the concentration of relic monopoles in the universe. Physics Letters B. 1978, 79 (3): 239–41. Bibcode:1978PhLB...79..239Z. doi:10.1016/0370-2693(78)90232-0.
Preskill, John. Cosmological production of superheavy magnetic monopoles. Physical Review Letters. 1979, 43 (19): 1365. Bibcode:1979PhRvL..43.1365P. doi:10.1103/PhysRevLett.43.1365.
See, e.g. Yao, W.–M.; Amsler, C.; Asner, D.; Barnett, R. M.; Beringer, J.; Burchat, P. R.; Carone, C. D.; Caso, C.; Dahl, O.; d'Ambrosio, G.; De Gouvea, A.; Doser, M.; Eidelman, S.; Feng, J. L.; Gherghetta, T.; Goodman, M.; Grab, C.; Groom, D. E.; Gurtu, A.; Hagiwara, K.; Hayes, K. G.; Hernández-Rey, J. J.; Hikasa, K.; Jawahery, H.; Kolda, C.; Kwon, Y.; Mangano, M. L.; Manohar, A. V.; Masoni, A.; et al. Review of Particle Physics. J. Phys. G. 2006, 33 (1): 1 [2014-06-03]. Bibcode:2006JPhG...33....1Y. arXiv:astro-ph/0601168 . doi:10.1088/0954-3899/33/1/001. （原始内容存档于2017-09-07）.
Guth, Alan H. Inflationary universe: A possible solution to the horizon and flatness problems (PDF). Physical Review D. 1981, 23 (2): 347–356 [2014-06-03]. Bibcode:1981PhRvD..23..347G. doi:10.1103/PhysRevD.23.347. （原始内容 (PDF)存档于2013-08-10）.
Starobinsky, Alexei A. A new type of isotropic cosmological models without singularity. Physics Letters B. 1980, 91: 99–102. Bibcode:1980PhLB...91...99S. doi:10.1016/0370-2693(80)90670-X.
Kazanas, D. Dynamics of the universe and spontaneous symmetry breaking. Astrophysical Journal. 1980, 241: L59–63. Bibcode:1980ApJ...241L..59K. doi:10.1086/183361.
Sato, K. Cosmological baryon number domain structure and the first order phase transition of a vacuum. Physics Letters B. 1981, 33: 66–70. Bibcode:1981PhLB...99...66S. doi:10.1016/0370-2693(81)90805-4.
Einhorn, Martin B; Sato, Katsuhiko. Monopole Production In The Very Early Universe In A First Order Phase Transition. Nuclear Physics B. 1981, 180 (3): 385–404. Bibcode:1981NuPhB.180..385E. doi:10.1016/0550-3213(81)90057-2.
Linde, A. A new inflationary universe scenario: A possible solution of the horizon, flatness, homogeneity, isotropy and primordial monopole problems. Physics Letters B. 1982, 108 (6): 389–393. Bibcode:1982PhLB..108..389L. doi:10.1016/0370-2693(82)91219-9.
Albrecht, Andreas; Steinhardt, Paul. Cosmology for Grand Unified Theories with Radiatively Induced Symmetry Breaking (PDF). Physical Review Letters. 1982, 48 (17): 1220–1223 [2014-06-03]. Bibcode:1982PhRvL..48.1220A. doi:10.1103/PhysRevLett.48.1220. （原始内容 (PDF)存档于2012-01-30）.
Hawking, S.W. The development of irregularities in a single bubble inflationary universe. Physics Letters B. 1982, 115 (4): 295. Bibcode:1982PhLB..115..295H. doi:10.1016/0370-2693(82)90373-2.
Starobinsky, Alexei A. Dynamics of phase transition in the new inflationary universe scenario and generation of perturbations. Physics Letters B. 1982, 117 (3–4): 175–8. Bibcode:1982PhLB..117..175S. doi:10.1016/0370-2693(82)90541-X.
Guth, A.H. Fluctuations in the new inflationary universe. Physical Review Letters. 1982, 49 (15): 1110–3. Bibcode:1982PhRvL..49.1110G. doi:10.1103/PhysRevLett.49.1110.
Bardeen, James M.; Steinhardt, Paul J.; Turner, Michael S. Spontaneous creation Of almost scale-free density perturbations in an inflationary universe. Physical Review D. 1983, 28 (4): 679. Bibcode:1983PhRvD..28..679B. doi:10.1103/PhysRevD.28.679.
Tegmark, M.; et al. Cosmological constraints from the SDSS luminous red galaxies. Physical Review D. August 2006, 74 (12): 123507. Bibcode:2006PhRvD..74l3507T. arXiv:astro-ph/0608632 . doi:10.1103/PhysRevD.74.123507.
Steinhardt, Paul J. Cosmological perturbations: Myths and facts. Modern Physics Letters A. 2004, 19 (13 & 16): 967–82. Bibcode:2004MPLA...19..967S. doi:10.1142/S0217732304014252.
Boyle, Latham A.; Steinhardt, PJ; Turok, N. Inflationary predictions for scalar and tensor fluctuations reconsidered. Physical Review Letters. 2006, 96 (11): 111301. Bibcode:2006PhRvL..96k1301B. PMID 16605810. arXiv:astro-ph/0507455 . doi:10.1103/PhysRevLett.96.111301.
Tegmark, Max. What does inflation really predict?. JCAP. 2005, 0504 (4): 001. Bibcode:2005JCAP...04..001T. arXiv:astro-ph/0410281 . doi:10.1088/1475-7516/2005/04/001.
Komatsu, E.; Smith, K. M.; Dunkley, J.; Bennett, C. L.; Gold, B.; Hinshaw, G.; Jarosik, N.; Larson, D.; Nolta, M. R.; Page, L.; Spergel, D. N.; Halpern, M.; Hill, R. S.; Kogut, A.; Limon, M.; Meyer, S. S.; Odegard, N.; Tucker, G. S.; Weiland, J. L.; Wollack, E.; Wright, E. L. Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation. The Astrophysical Journal Supplement Series. January 2010, 192 (2): 18. Bibcode:2011ApJS..192...18K. arXiv:1001.4538 . doi:10.1088/0067-0049/192/2/18.
Spergel, D. N.; et al. First year Wilkinson Microwave Anisotropy Probe (WMAP) observations: determination of cosmological parameters. Astrophysical Journal Supplement Series. 2003, 148 (1): 175–194. Bibcode:2003ApJS..148..175S. arXiv:astro-ph/0302209 . doi:10.1086/377226.
Hanson, D.; et al. Detection of B-Mode Polarization in the Cosmic Microwave Background with Data from the South Pole Telescope. Physical Review Letters. 14. Sep 30, 2013, 111. doi:10.1103/PhysRevLett.111.141301.
Loeb, A.; Zaldarriaga, M. Measuring the small-scale power spectrum of cosmic density fluctuations through 21 cm tomography prior to the epoch of structure formation. Physical Review Letters. 2004, 92 (21): 211301. Bibcode:2004PhRvL..92u1301L. PMID 15245272. arXiv:astro-ph/0312134 . doi:10.1103/PhysRevLett.92.211301.
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見：Lyth, David H. What would we learn by detecting a gravitational wave signal in the cosmic microwave background anisotropy?. Physical Review Letters. 1997, 78 (10): 1861–3 [2020-10-06]. Bibcode:1997PhRvL..78.1861L. arXiv:hep-ph/9606387 . doi:10.1103/PhysRevLett.78.1861. （原始内容存档于2012-06-29）.
Vilenkin, Alexander. The birth of inflationary universes. Physical Review D. 1983, 27 (12): 2848. Bibcode:1983PhRvD..27.2848V. doi:10.1103/PhysRevD.27.2848.
A. Borde, A. Guth and A. Vilenkin. Inflationary space-times are incomplete in past directions. Physical Review Letters. 2003, 90 (15): 151301. Bibcode:2003PhRvL..90o1301B. PMID 12732026. arXiv:gr-qc/0110012 . doi:10.1103/PhysRevLett.90.151301.
A. Borde. Open and closed universes, initial singularities and inflation. Physical Review D. 1994, 50 (6): 3692–702. Bibcode:1994PhRvD..50.3692B. doi:10.1103/PhysRevD.50.3692.
A. Borde and A. Vilenkin. Eternal inflation and the initial singularity. Physical Review Letters. 1994, 72 (21): 3305–9. Bibcode:1994PhRvL..72.3305B. arXiv:gr-qc/9312022 . doi:10.1103/PhysRevLett.72.3305.
Carroll, Sean M.; Chen, Jennifer. Does inflation provide natural initial conditions for the universe?. Gen. Rel. Grav. 2005, 37 (10): 1671–4. Bibcode:2005GReGr..37.1671C. arXiv:gr-qc/0505037 . doi:10.1007/s10714-005-0148-2.
Aguirre, Anthony; Gratton, Steven. Inflation without a beginning: A null boundary proposal. Physical Review D. 2003, 67 (8): 083515. Bibcode:2003PhRvD..67h3515A. arXiv:gr-qc/0301042 . doi:10.1103/PhysRevD.67.083515.
Aguirre, Anthony; Gratton, Steven. Steady-State Eternal Inflation. Physical Review D. 2002, 65 (8): 083507. Bibcode:2002PhRvD..65h3507A. arXiv:astro-ph/0111191 . doi:10.1103/PhysRevD.65.083507.
Hartle, J.; Hawking, S. Wave function of the universe. Physical Review D. 1983, 28 (12): 2960. Bibcode:1983PhRvD..28.2960H. doi:10.1103/PhysRevD.28.2960. ; See also Hawking (1998).
Page, Don N. Inflation does not explain time asymmetry. Nature. 1983, 304 (5921): 39. Bibcode:1983Natur.304...39P. doi:10.1038/304039a0. ，見：The Road to Reality: A Complete Guide to the Laws of the Universe，羅傑·潘洛斯著。
Albrecht, Andreas; Sorbo, Lorenzo. Can the universe afford inflation?. Physical Review D. 2004, 70 (6): 063528. Bibcode:2004PhRvD..70f3528A. arXiv:hep-th/0405270 . doi:10.1103/PhysRevD.70.063528.
Martin, Jerome; Brandenberger, Robert. The trans-Planckian problem of inflationary cosmology. Physical Review D. 2001, 63 (12): 123501. Bibcode:2001PhRvD..63l3501M. arXiv:hep-th/0005209 . doi:10.1103/PhysRevD.63.123501.
Martin, Jerome; Ringeval, Christophe. Superimposed Oscillations in the WMAP Data?. Physical Review D. 2004, 69 (8): 083515. Bibcode:2004PhRvD..69h3515M. arXiv:astro-ph/0310382 . doi:10.1103/PhysRevD.69.083515.
Kachru, Shamit; Kallosh, Renata; Linde, Andrei; Maldacena, Juan; McAllister, Liam; Trivedi, Sandip P. Towards inflation in string theory. JCAP. 2003, 0310 (10): 013. Bibcode:2003JCAP...10..013K. arXiv:hep-th/0308055 . doi:10.1088/1475-7516/2003/10/013.
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Poplawski, N. Nonsingular, big-bounce cosmology from spinor-torsion coupling. Physical Review D. 2012, 85 (10): 107502. Bibcode:2012PhRvD..85j7502P. arXiv:1111.4595 . doi:10.1103/PhysRevD.85.107502.
Brandenberger, R; Vafa, C. Superstrings in the early universe. Nuclear Physics B. 1989, 316 (2): 391–410. Bibcode:1989NuPhB.316..391B. doi:10.1016/0550-3213(89)90037-0.
Battefeld, Thorsten; Watson, Scott. String Gas Cosmology. Reviews Modern Physics. 2006, 78 (2): 435–454. Bibcode:2006RvMP...78..435B. arXiv:hep-th/0510022 . doi:10.1103/RevModPhys.78.435.
Brandenberger, Robert H.; Nayeri, ALI; Patil, Subodh P.; Vafa, Cumrun. String Gas Cosmology and Structure Formation. International Journal of Modern Physics A. 2007, 22 (21): 3621–3642. Bibcode:2007IJMPA..22.3621B. arXiv:hep-th/0608121 . doi:10.1142/S0217751X07037159.
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harvard.edu

ui.adsabs.harvard.edu

這是因為暴脹勢可以寫作φ/m_Pl的泰勒級數，其中φ為暴脹場，m_Pl為普朗克質量。對於單單一個項，比如質量項m_φ⁴(φ/m_Pl)²，慢滾條件在φ比m_Pl大很多的情況下得到滿足。有效場論就是這種情況，高階項會使暴脹的條件不再得到滿足。這些高階項不存在，也可以看做是一種微調。見：Alabidi, Laila; Lyth, David H. Inflation models and observation. JCAP. 2006, 0605 (5): 016. Bibcode:2006JCAP...05..016A. arXiv:astro-ph/0510441 . doi:10.1088/1475-7516/2006/05/016.
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A. Borde. Open and closed universes, initial singularities and inflation. Physical Review D. 1994, 50 (6): 3692–702. Bibcode:1994PhRvD..50.3692B. doi:10.1103/PhysRevD.50.3692.
A. Borde and A. Vilenkin. Eternal inflation and the initial singularity. Physical Review Letters. 1994, 72 (21): 3305–9. Bibcode:1994PhRvL..72.3305B. arXiv:gr-qc/9312022 . doi:10.1103/PhysRevLett.72.3305.
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