Built on

M. Bastero-Gil, A. Berera, and R. O. Ramos, JCAP 1109
Original
1929
Earlier work this paper cites.
A. Maleknejad and M. M. Sheikh-Jabbari, Phys. Rev. D84
Original
1932
Earlier work this paper cites.
A. Berera and L.-Z. Fang, Phys. Rev. Lett. 74
1995
Earlier work this paper cites.
A. Berera, Phys. Rev. Lett. 75
1995
Earlier work this paper cites.
J. Yokoyama and A. D. Linde, Phys. Rev. D60
1999
Earlier work this paper cites.
M. Schmaltz and D. Tucker-Smith, Ann. Rev. Nucl. Part. Sci. 55
2005
Earlier work this paper cites.
A. Berera, I. G. Moss, and R. O. Ramos, Rept. Prog. Phys. 72
Original
2009
Earlier work this paper cites.
M. Bastero-Gil and A. Berera, Int. J. Mod. Phys. A24
Original
2009
Earlier work this paper cites.

Similar

There are two methods for covering isotropic symmetry for gauge fields Golovnev et al. 2008 : The first one is introducing a collective mode A i a = ϕ ⁡ ( t ) δ i a A^{a}_{i}=\phi(t)\delta^{a}_{i} with a delta function between internal index and space index Adshead and Wyman 2012 ; Maleknejad and Sheikh-Jabbari 2011 . The second one is considering a configuration of quantized random direction fields at various positions in the space. With averaging of these fields the space part of the gauge field is integrated out and also the isotropic symmetry recovered. In our model, we have used the second one
2011
Cited alongside, same era.
M. M. Sheikh-Jabbari, Phys. Lett. B717
Original
2012
Cited alongside, same era.
P. Adshead and M. Wyman, Phys. Rev. Lett. 108
Original
2012
Cited alongside, same era.
M. Bastero-Gil, A. Berera, R. O. Ramos, and J. G. Rosa, JCAP 1301

Then

X.-M. Zhang, H.-Y. Ma, P.-C. Chu, J.-T. Liu, and J.-Y. Zhu, JCAP 1603
Original
2016
Later among the works it cites.
Y. Akrami et al. (Planck), (2018), arXiv:1807.06211 [astro-ph.CO]
Original
2018
Later among the works it cites.
P. Agrawal, G. Obied, P. J. Steinhardt, and C. Vafa, Phys. Lett. B784
Original
2018
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M. Motaharfar, V. Kamali, and R. O. Ramos, (2018), arXiv:1810.02816 [astro-ph.CO]
Original
2018
Later among the works it cites.
M. Bastero-Gil, A. Berera, R. Hernández-Jiménez, and J. G. Rosa, (2018), arXiv:1812.07296 [hep-ph]
Original

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2019

Warm (Pseudo)Scalar Inflation

Kamali, Vahid.

Understand

In this note, we will introduce an action for warm inflation model with direct coupling between the pseudoscalar field and mass-less $SU(2)$ gauge fields.

The potential of inflaton is protected against the thermal corrections in a thermal bath of gauge fields even with strong direct interaction between inflaton and light fields.
The dissipation parameter of this model is approximately constant in the high-dissipative regime.
In this regime, the model is compatible with observational data and non-Gaussianity is in order of Hubble slow-roll parameter $\frac{\epsilon_{\phi}}{1+Q}$ even in $f<M_p$ limit.

Built on

M. Bastero-Gil, A. Berera, and R. O. Ramos, JCAP 1109
Original
1929
Earlier work this paper cites.
A. Maleknejad and M. M. Sheikh-Jabbari, Phys. Rev. D84
Original
1932
Earlier work this paper cites.
A. Berera and L.-Z. Fang, Phys. Rev. Lett. 74
1995
Earlier work this paper cites.
A. Berera, Phys. Rev. Lett. 75
1995
Earlier work this paper cites.
J. Yokoyama and A. D. Linde, Phys. Rev. D60
1999
Earlier work this paper cites.
M. Schmaltz and D. Tucker-Smith, Ann. Rev. Nucl. Part. Sci. 55
2005
Earlier work this paper cites.
A. Berera, I. G. Moss, and R. O. Ramos, Rept. Prog. Phys. 72
Original
2009
Earlier work this paper cites.
M. Bastero-Gil and A. Berera, Int. J. Mod. Phys. A24
Original
2009
Earlier work this paper cites.

Similar

There are two methods for covering isotropic symmetry for gauge fields Golovnev et al. 2008 : The first one is introducing a collective mode A i a = ϕ ⁡ ( t ) δ i a A^{a}_{i}=\phi(t)\delta^{a}_{i} with a delta function between internal index and space index Adshead and Wyman 2012 ; Maleknejad and Sheikh-Jabbari 2011 . The second one is considering a configuration of quantized random direction fields at various positions in the space. With averaging of these fields the space part of the gauge field is integrated out and also the isotropic symmetry recovered. In our model, we have used the second one
2011
Cited alongside, same era.
M. M. Sheikh-Jabbari, Phys. Lett. B717
Original
2012
Cited alongside, same era.
P. Adshead and M. Wyman, Phys. Rev. Lett. 108
Original
2012
Cited alongside, same era.
M. Bastero-Gil, A. Berera, R. O. Ramos, and J. G. Rosa, JCAP 1301