Graciela B. Gelmini

TL;DR: In this article, the authors compute upper bounds to the expected amplitude of daily modulation due to channeling using channeling fractions that were obtained with analytic models in prior work and show that even the largest daily modulation amplitudes (of the order of 10% in some instances) would not be observable for WIMPs in the standard halo in the 13 years of data taken by the DAMA Collaboration.

TL;DR: In this article, the mechanism of the production of WIMPs in the early universe has been studied both in standard and non-standard pre-Big Bang Nucleosynthesis cosmologies.

TL;DR: In this article, the neutralino direct detection rate in nonstandard cosmological scenarios where neutralinos account for the dark matter of the Universe is computed. But the main feature is the presence of additional light (m Χ ≤ 40 GeV) and heavy (m ≥ 600 GeV), with detection rates within the sensitivity of future dark matter experiments.

TL;DR: In this article, the authors investigated the allowed range of reheating temperature values in light of the Planck 2015 results and the recent joint analysis of Cosmic Microwave Background (CMB) data from the BICEP2/Keck Array and Planck experiments, using monomial and binomial inflationary potentials.

TL;DR: In this paper, the authors compared direct dark matter (DM) detection data for light WIMPs with exothermic scattering with nuclei (exoDM), both assuming the Standard Halo Model (SHM) and in a halo-independent manner.