text: 487,139,1350064428348297216,1349798626483187713,Ivan Esteban,"Paper out! In <LINK>, Jordi Salvado & myself ask ourselves: why do we always assume ideal gases in cosmology? We study how long-range interactions change the energy density and equation of state (eos). And, what happens if neutrinos self-interact? <LINK> This plot shows eos as a function of temperature for an interacting system: 1) It is ultrarelativistic (w=1/3) for temperatures well below the particle mass. For neutrinos, this means they would be relativistic longer! 2) Notice the dramatic difference wrt ideal gas [dashed]! <LINK> When applied to self-interacting neutrinos, 1) There is *no* relevant cosmological neutrino mass bound. #KATRIN could detect something soon! 2) Future surveys as EUCLID could fail to detect neutrino masses. We have also made our cosmo code public! <LINK>",https://arxiv.org/abs/2101.05804,"Cosmology is well suited to study the effects of long range interactions due to the large densities in the early Universe. In this article, we explore how the energy density and equation of state of a fermion system diverge from the commonly assumed ideal gas form under the presence of scalar long range interactions with a range much smaller than cosmological scales. In this scenario, ""small""-scale physics can impact our largest-scale observations. As a benchmark, we apply the formalism to self-interacting neutrinos, performing an analysis to present and future cosmological data. Our results show that the current cosmological neutrino mass bound is fully avoided in the presence of a long range interaction, opening the possibility for a laboratory neutrino mass detection in the near future. We also demonstrate an interesting complementarity between neutrino laboratory experiments and the future EUCLID survey. ",Long Range Interactions in Cosmology: Implications for Neutrinos,3,"['Paper out!\nIn <LINK>, Jordi Salvado &amp; myself ask ourselves: why do we always assume ideal gases in cosmology? \nWe study how long-range interactions change the energy density and equation of state (eos). And, what happens if neutrinos self-interact? <LINK>', 'This plot shows eos as a function of temperature for an interacting system:\n1) It is ultrarelativistic (w=1/3) for temperatures well below the particle mass. For neutrinos, this means they would be relativistic longer!\n2) Notice the dramatic difference wrt ideal gas [dashed]! https://t.co/THqijhjsxX', 'When applied to self-interacting neutrinos,\n1) There is *no* relevant cosmological neutrino mass bound. #KATRIN could detect something soon!\n2) Future surveys as EUCLID could fail to detect neutrino masses.\n\nWe have also made our cosmo code public! https://t.co/Oi9oVsApuj']",21,01,793