activity
20192026
most citedIncomplete neutrino decoupling effect on big bang nucleosynthesis

25 citations · 34 across the 12 of their papers we have counts for

collaborators

23 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 the presence of non-zero lepton and baryon asymmetries. Considering different scenarios, we determine the equation of sta…

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 usin…

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-ph2026

Impact of non-standard neutrino-electron interactions on Big Bang Nucleosynthesis

Julien Froustey, Stefano Gariazzo, Jaume Moncho +2

Neutrino non-standard interactions (NSI) with electrons, predicted in many extended theoretical models of particle physics, are known to alter the picture of neutrino decoupling fr…

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…