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20102026
most citedWarm inflation as a way out of the swampland

143 citations · 880 across the 47 of their papers we have counts for

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hep-th2022★ 10 cited

Unitarity Problems for an Effective Field Theory Description of Early Universe Cosmology

Robert Brandenberger, Vahid Kamali

In the context of Effective Field Theory, the Hilbert space of states increases in an expanding universe. Hence, the time evolution cannot be unitary. The formation of structure is…

hep-th2020★ 11 cited

Thermal, Trapped and Chromo-Natural Inflation in light of the Swampland Criteria and the Trans-Planckian Censorship Conjecture

Arjun Berera, Robert Brandenberger, Vahid Kamali +1

We consider thermal, trapped and chromo-natural inflation in light of the swampland criteria and the Trans-Planckian Censorship Conjecture (TCC). Since thermal inflation occurs at…

hep-th2020★ 12 cited

Creating Spatial Flatness by Combining String Gas Cosmology and Power Law Inflation

Vahid Kamali, Robert Brandenberger

We show that it is possible to combine an early phase of String Gas Cosmology which can explain the origin of the observed structures on cosmological scales with a short later peri…

hep-th2020

Strengthening the de Sitter swampland conjecture in warm inflation

Robert Brandenberger, Vahid Kamali, Rudnei O. Ramos

The "de Sitter constraint" on the space of effective scalar field theories consistent with superstring theory provides a lower bound on the slope of the potential of a scalar field…

hep-th2020★ 25 cited

Relaxing the TCC Bound on Inflationary Cosmology?

Vahid Kamali, Robert Brandenberger

We demonstrate that the strict upper bounds on the energy scale of inflation and on the tensor-to-scalar ratio can be somewhat relaxed if we assume that - after an initial period o…

hep-th2013★ 34 cited

Tachyon Warm-Logamediate Inflationary Universe Model in High Dissipative Regime

M. R. Setare, V. Kamali

In the present work, we study warm tachyon inflation model in the context of "logamediate inflation" where the cosmological scale factor expands as . The cha…