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Warm λ4ϕ4 inflationary universe model in light of Planck 2015 results
DOI: 10.1140/epjc/s10052-015-3764-3 Bibcode: 2015EPJC...75..525P

Videla, Nelson; Panotopoulos, Grigorios

In the present work we show that warm chaotic inflation characterized by a simple λ4ϕ4 self-interaction potent…

2015 European Physical Journal C
Planck 38
Warm intermediate inflation in the Randall–Sundrum II model in the light of Planck 2015 and BICEP2 results: a general dissipative coefficient
DOI: 10.1140/epjc/s10052-015-3433-6 Bibcode: 2015EPJC...75..205H

Videla, Nelson; Herrera, Ramón; Olivares, Marco

A warm inflationary Universe in the Randall–Sundrum II model during intermediate inflation is studied. For this purpose, we consider the general form for the dissipative coefficient Γ(T,<…

2015 European Physical Journal C
Planck 34
X-ray lines and self-interacting dark matter
DOI: 10.1140/epjc/s10052-015-3788-8 Bibcode: 2015EPJC...75..570M

Mambrini, Yann; Toma, Takashi

We study the correlation between a monochromatic signal from annihilating dark matter and its self-interacting cross section. We apply our argument to a complex scalar dark sector, where the pseudo-scalar plays the role of a warm dark matter candidate while the scalar mediates its interaction with the Standard Model. We combine the recent observat…

2015 European Physical Journal C
INTEGRAL 14
Nearly scale-invariant power spectrum and quantum cosmological perturbations in the gravity's rainbow scenario
DOI: 10.1140/epjc/s10052-015-3457-y Bibcode: 2015EPJC...75..259W

Wang, Sai; Chang, Zhe

We propose the gravity's rainbow scenario as a possible alternative of the inflation paradigm to account for the flatness and horizon problems. We focus on studying the cosmological scalar perturbations which are seeded by the quantum fluctuations in the very early universe. The scalar power spectrum is expected to be nearly scale-invariant. We es…

2015 European Physical Journal C
Planck 11