activity
20242026
most citedFifty shades of grayness: parametrizations of spectral distortions and applications in cosmology

1 citations · 2 across the 6 of their papers we have counts for

collaborators

18 papers

astro-ph.CO2026

Primordial Asymmetries, Primordial Equation of State & Primordial Black Holes

Maël Gonin, Julien Froustey, Albert Escrivà +3

We study the thermal history of the primordial Universe in presence of non-zero lepton and baryon asymmetries. Considering different scenarios, we determine the equation of state (…

astro-ph.CO2026

What could an emerging Big Bang Nucleosynthesis discrepancy be hinting at?

Vivian Poulin, Julien Froustey, Cyril Pitrou +1

The latest measurement of the primordial deuterium abundance is in tension with several state-of-the-art predictions of standard Big Bang nucleosynthesis (BBN), when usi…

hep-ph2026

Neutrino helicity oscillations in astrophysical environments: a many-body approach

Yiheng Xu, Julien Froustey, George M. Fuller +2

Neutrino rest mass enables left-handed states to "flip" to right-handed states and vice versa. In-medium effects can enhance the probability for such spin-flip. We demonstrate that…

astro-ph.HE2026

Neutrino transport and flavor instabilities in a post-merger disk

Erick Urquilla, Swapnil Shankar, Debraj Kundu +6

Neutron star mergers are multimessenger sources whose dynamics and signals depend critically on neutrinos and their flavor transformations. We investigate whether fast and collisio…

hep-ph20261 cited

Fifty shades of grayness: parametrizations of spectral distortions and applications in cosmology

Gabriela Barenboim, Julien Froustey, Cyril Pitrou +1

Thermal distribution functions can only be of the Fermi-Dirac or Bose-Einstein types, whereas distorted spectra encompass any possible deviations from these shapes. It is fruitful…

astro-ph.HE20261 cited

Neutrino flavor instabilities in neutron star mergers with moment transport: Slow, fast, and collisional modes

Julien Froustey, Francois Foucart, Christian Hall +5

Determining where, when, and how neutrino flavor oscillations must be included in large-scale simulations of hot and dense astrophysical environments is an enduring challenge that…