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20062023
most citedThe pre-inflationary dynamics of loop quantum cosmology: Confronting quantum gravity with observations

260 citations · 2.4k across the 63 of their papers we have counts for

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Showing 2010Show all

6 papers · 1 filter

astro-ph.CO2010★ 163 cited

Non-gaussianities and the Stimulated creation of quanta in the inflationary universe

Ivan Agullo, Leonard Parker

Cosmological inflation generates a spectrum of density perturbations that can seed the cosmic structures we observe today. These perturbations are usually computed as the result of…

gr-qc2010★ 8 cited

Acceleration radiation, transition probabilities, and trans-Planckian physics

I. Agullo, J. Navarro-Salas, G. J. Olmo +1

An important question in the derivation of the acceleration radiation, which also arises in Hawking's derivation of black hole radiance, is the need to invoke trans-Planckian physi…

hep-th2010★ 31 cited

Hawking radiation by Kerr black holes and conformal symmetry

Ivan Agullo, Jose Navarro-Salas, Gonzalo J. Olmo +1

The exponential blueshift associated with the event horizon of a black hole makes conformal symmetry play a fundamental role in accounting for its thermal properties. Using a deriv…

astro-ph.CO2010

Inflation, Quantum Field Renormalization, and CMB Anisotropies

Ivan Agullo, Jose Navarro-Salas, Gonzalo J. Olmo +1

We point out that if quantum field renormalization is taken into account the predictions of slow-roll inflation for both the scalar and tensorial power spectra change significantly…

gr-qc2010★ 2 cited

Reply to "Comment on 'Insensitivity of Hawking radiation to an invariant Planck-scale cutoff' "

Ivan Agullo, Jose Navarro-Salas, Gonzalo J. Olmo +1

We clarify the relationship between the conclusions of the previous Comment of A. Helfer [1] and that of our Brief Report [arXiv:0906.5315]

gr-qc2010★ 7 cited

Inflation, Renormalization, and CMB Anisotropies

I. Agullo, J. Navarro-Salas, Gonzalo J. Olmo +1

In single-field, slow-roll inflationary models, scalar and tensorial (Gaussian) perturbations are both characterized by a zero mean and a non-zero variance. In position space, the…