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Relic neutrino decoupling including flavour oscillations

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Properties and performance of the prototype instrument for the Pierre Auger Observatory

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Primordial nucleosynthesis: From precision cosmology to fundamental physics

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Correlation of the highest-energy cosmic rays with nearby extragalactic objects.

Using data collected at the Pierre Auger Observatory during the past 3.7 years, we demonstrated a correlation between the arrival directions of cosmic rays with energy above 6 x 10(19) electron volts…
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Bounds on very low reheating scenarios after Planck

We consider the case of very low reheating scenarios [${T}_{\mathrm{RH}}\ensuremath{\sim}\mathcal{O}(\mathrm{MeV})$] with a better calculation of the production of the relic neutrino background (with…
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PArthENoPE: Public algorithm evaluating the nucleosynthesis of primordial elements

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Observation of the suppression of the flux of cosmic rays above 4 x 10 (19) eV.

The energy spectrum of cosmic rays above 2.5 x 10;{18} eV, derived from 20,000 events recorded at the Pierre Auger Observatory, is described and the hypothesis of a single power law is rejected with a significance greater than 6 standard deviations.
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Correlation of the highest-energy cosmic rays with the positions of nearby active galactic nuclei

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Nuclear reaction network for primordial nucleosynthesis: a detailed analysis of rates, uncertainties and light nuclei yields

We analyse in detail the standard primordial nucleosynthesis scenario. In particular, we discuss the key theoretical issues which are involved in a detailed prediction of light nuclide abundances,…
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The baryon density of the Universe from an improved rate of deuterium burning.

Improved cross-sections of the deuterium burning D(p,γ)3He reaction lead to BBN estimates of the baryon density at the 1.6 percent level, in excellent agreement with a recent analysis of the cosmic microwave background.
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