brane inflation
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2021 ◽  
Vol 104 (12) ◽  
Author(s):  
Abolhassan Mohammadi ◽  
Tayeb Golanbari ◽  
Jamil Enayati
Keyword(s):  

2021 ◽  
Vol 136 (1) ◽  
Author(s):  
S. Santos da Costa ◽  
M. Benetti ◽  
R. M. P. Neves ◽  
F. A. Brito ◽  
R. Silva ◽  
...  

2020 ◽  
Vol 810 ◽  
pp. 135813
Author(s):  
R.M.P. Neves ◽  
F.F. Santos ◽  
F.A. Brito
Keyword(s):  

2020 ◽  
Vol 2020 (10) ◽  
Author(s):  
Manki Kim ◽  
Liam McAllister

Abstract In axion monodromy inflation, traversing N axion periods corresponds to discharging N units of a quantized charge. In certain models with moving D7-branes, such as Higgs-otic inflation, this monodromy charge is D3-brane charge induced on the D7-branes. The stress-energy of the induced charge affects the internal space, changing the inflaton potential and potentially limiting the field range. We compute the backreaction of induced D3-brane charge in Higgs-otic inflation. The effect on the nonperturbative superpotential is dramatic even for N = 1, and may preclude large-field inflation in this model in the absence of a mechanism to control the backreaction.


2020 ◽  
Vol 101 (12) ◽  
Author(s):  
Abolhassan Mohammadi ◽  
Tayeb Golanbari ◽  
Salah Nasri ◽  
Khaled Saaidi
Keyword(s):  

Author(s):  
Mudassar Sabir ◽  
Waqas Ahmed ◽  
Yungui Gong ◽  
Yizhou Lu

AbstractIn the large extra dimensional braneworld inflation, Friedmann equation is modified to include a quadratic term in energy density with an additional parameter $$\lambda $$λ called brane tension in addition to the usual linear term. The high energy brane corrections modify the slow-roll parameters and affect the behaviour of inflation. We analyse the superconformal inflation for E-models and find that there exist $$\alpha $$α-attractors in brane inflation. The predictions for the scalar spectral index $$n_s$$ns and the tensor-to-scalar ratio r are computed numerically, and approximate analytic formulas in the high energy limit have been given for the observable $$n_s$$ns and r. The constraints on the model parameters are obtained by using Planck 2018 and BICEP2 observational data.


2019 ◽  
Vol 2019 (09) ◽  
pp. 030-030 ◽  
Author(s):  
Renata Kallosh ◽  
Andrei Linde
Keyword(s):  

2019 ◽  
Vol 2019 (1) ◽  
Author(s):  
Renata Kallosh ◽  
Andrei Linde ◽  
Yusuke Yamada
Keyword(s):  

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