Fetching the paper…
Reading the bibliography…
Galileon inflation is a radiatively stable higher derivative model of inflation.
C. Burrage and D. Seery, (2010), arXiv:1005.1927 [astro-ph.CO]
1927
Earlier work this paper cites.
C. Deffayet, S. Deser, and G. Esposito-Farese, Phys. Rev., D80
1967
Earlier work this paper cites.
A. I. Vainshtein, Phys. Lett., B39
1972
Earlier work this paper cites.
G. ’t Hooft, NATO Adv. Study Inst. Ser. B Phys., 59
1980
Earlier work this paper cites.
E. D. Stewart and D. H. Lyth, Phys. Lett., B302
1993
Earlier work this paper cites.
J. F. Donoghue, Phys. Rev. Lett., 72
1994
Earlier work this paper cites.
J. F. Donoghue, Phys. Rev., D50
1994
Earlier work this paper cites.
A. A. Tseytlin, (1999), arXiv:hep-th/9908105
1999
Earlier work this paper cites.
C. Armendariz-Picon, T. Damour, and V. F. Mukhanov, Phys. Lett., B458
1999
Earlier work this paper cites.
J. Garriga and V. F. Mukhanov, Phys. Lett., B458
1999
Earlier work this paper cites.
G. R. Dvali, G. Gabadadze, and M. Porrati, Phys. Lett., B485
2000
Earlier work this paper cites.
E. Komatsu and D. N. Spergel, Phys. Rev., D63
2001
Earlier work this paper cites.
T. Okamoto and W. Hu, Phys. Rev., D66
2002
Earlier work this paper cites.
P. Creminelli, JCAP, 0310
2003
Earlier work this paper cites.
M. A. Luty, M. Porrati, and R. Rattazzi, JHEP, 09
2003
Earlier work this paper cites.
J. M. Maldacena, JHEP, 05
2003
Earlier work this paper cites.
E. Silverstein and D. Tong, Phys. Rev., D70
2004
Earlier work this paper cites.
M. Alishahiha, E. Silverstein, and D. Tong, Phys. Rev., D70
2004
Earlier work this paper cites.
M. Porrati and J. W. Rombouts, Phys. Rev., D69
2004
Earlier work this paper cites.
A. Nicolis and R. Rattazzi, JHEP, 06
2004
Earlier work this paper cites.
N. Arkani-Hamed, P. Creminelli, S. Mukohyama, and M. Zaldarriaga, JCAP, 0404
2004
Earlier work this paper cites.
D. Babich, P. Creminelli, and M. Zaldarriaga, JCAP, 0408
2004
Earlier work this paper cites.
P. Creminelli and M. Zaldarriaga, JCAP, 0410
2004
Earlier work this paper cites.
X. Chen, JHEP, 08
2005
Earlier work this paper cites.
D. Seery and J. E. Lidsey, JCAP, 0506
2005
Earlier work this paper cites.
S. Weinberg, Phys. Rev., D72
2005
Cited alongside, same era.
L. Boubekeur and D. H. Lyth, Phys. Rev., D73
2006
Cited alongside, same era.
M. Sasaki, J. Valiviita, and D. Wands, Phys. Rev., D74
2006
Cited alongside, same era.
X. Chen, M.-x. Huang, S. Kachru, and G. Shiu, JCAP, 0701
2007
Cited alongside, same era.
D. Seery, J. E. Lidsey, and M. S. Sloth, JCAP, 0701
2007
Cited alongside, same era.
J. E. Lidsey and D. Seery, Phys. Rev., D75
2007
Cited alongside, same era.
C. de Rham and G. Gabadadze, Phys. Rev., D82
2010
Closest in time.
T. Kobayashi, H. Tashiro, and D. Suzuki, Phys. Rev., D81
2010
Closest in time.
2010
Closest in time.
A. De Felice and S. Tsujikawa, (2010a), arXiv:1007.2700 [astro-ph.CO]
2010
Closest in time.
A. De Felice and S. Tsujikawa, (2010b), arXiv:1008.4236 [hep-th]
2010
Closest in time.
alphaXiv searches the wider corpus for related work and actual follow-ups.
alphaXiv is searching for related work…
These slow-roll combinations differ slightly from Eqs. (A.9)–(A.10) of Ref. Chen et al. 2007 , because we are expressing each Hankel function in terms of the combination − k c s τ -kc_{s}\tau , whereas the authors of Ref. Chen et al. 2007 used the combination k c s / a H kc_{s}/aH . These differ at first order in slow-roll parameters, but our expressions are equivalent
2007
Cited alongside, same era.
2007
Cited alongside, same era.
N. Barnaby and N. Kamran, JHEP, 02
2008
Cited alongside, same era.
2008
Cited alongside, same era.
C. de Rham, S. Hofmann, J. Khoury, and A. J. Tolley, JCAP, 0802
2008
Cited alongside, same era.
C. Cheung, P. Creminelli, A. L. Fitzpatrick, J. Kaplan, and L. Senatore, JHEP, 03
2008
Cited alongside, same era.
2010
Closest in time.
P. Creminelli, A. Nicolis, and E. Trincherini, (2010), arXiv:1007.0027 [hep-th]
2010
Closest in time.
T. Kobayashi, M. Yamaguchi, and J. Yokoyama, (2010b), arXiv:1008.0603 [hep-th]
2010
Closest in time.
S. Mizuno and K. Koyama, (2010), arXiv:1009.0677 [hep-th]
2010
Closest in time.
C. Deffayet, O. Pujolas, I. Sawicki, and A. Vikman, (2010a), arXiv:1008.0048 [hep-th]
2010
Closest in time.
S. Endlich, K. Hinterbichler, L. Hui, A. Nicolis, and J. Wang, (2010), arXiv:1002.4873 [hep-th]
2010
Closest in time.
K. Hinterbichler, M. Trodden, and D. Wesley, (2010), arXiv:1008.1305 [hep-th]
2010
Closest in time.
C. Deffayet, S. Deser, and G. Esposito-Farese, (2010b), arXiv:1007.5278 [gr-qc]
2010
Closest in time.
A. Padilla, P. M. Saffin, and S.-Y. Zhou, (2010a), arXiv:1007.5424 [hep-th]
2010
Closest in time.
A. Padilla, P. M. Saffin, and S.-Y. Zhou, (2010b), arXiv:1008.0745 [hep-th]
2010
Closest in time.
A. Padilla, P. M. Saffin, and S.-Y. Zhou, (2010c), arXiv:1008.3312 [hep-th]
2010
Closest in time.
L. Senatore, K. M. Smith, and M. Zaldarriaga, JCAP, 1001
2010
Closest in time.
N. Bartolo, M. Fasiello, S. Matarrese, and A. Riotto, JCAP, 1008
2010
Closest in time.
N. Bartolo, M. Fasiello, S. Matarrese, and A. Riotto, (2010b), arXiv:1006.5411 [astro-ph.CO]
2010
Closest in time.
E. Komatsu et al. , (2010), arXiv:1001.4538 [astro-ph.CO]
2010
Closest in time.
J. Smidt et al. , Phys. Rev., D81
2010
Closest in time.
A similar observation was made in the recent preprint Ref. Hinterbichler et al. 2010 , which appeared as this paper was in the final stages of preparation
2010
Closest in time.
N. Bartolo, E. Dimastrogiovanni, and A. Vallinotto, (2010c), arXiv:1006.0196 [astro-ph.CO]
2010
Closest in time.
C. de Rham et al. , Phys. Rev. Lett., 100
2072
Closest in time.