activity
20142024
most citedCMB-S4 Science Case, Reference Design, and Project Plan

443 citations · 1.7k across the 35 of their papers we have counts for

collaborators

35 papers

astro-ph.CO2024★ 5 cited

Cosmic Neutrino Decoupling and its Observable Imprints: Insights from Entropic-Dual Transport

J. Richard Bond, George M. Fuller, Evan Grohs +2

Very different processes characterize the decoupling of neutrinos to form the cosmic neutrino background (CB) and the much later decoupling of photons from thermal equilibrium t…

astro-ph.HE2024★ 2 cited

Neutrino flavor transformation with moments: application to fast flavor instabilities in neutron star mergers

Julien Froustey, Sherwood Richers, Evan Grohs +4

Neutrino evolution, of great importance in environments such as neutron star mergers (NSMs) because of their impact on explosive nucleosynthesis, is still poorly understood due to…

astro-ph.HE2023★ 34 cited

Neutrino fast flavor oscillations with moments: linear stability analysis and application to neutron star mergers

Julien Froustey, Sherwood Richers, Evan Grohs +4

Providing an accurate modeling of neutrino physics in dense astrophysical environments such as binary neutron star mergers presents a challenge for hydrodynamic simulations. Nevert…

astro-ph.HE2023★ 27 cited

Two-Moment Neutrino Flavor Transformation with applications to the Fast Flavor Instability in Neutron Star Mergers

Evan Grohs, Sherwood Richers, Sean M. Couch +4

Multi-messenger astrophysics has produced a wealth of data with much more to come in the future. This enormous data set will reveal new insights into the physics of core collapse s…

hep-ph2023★ 9 cited

Implications on Cosmology from Dirac Neutrino Magnetic Moments

E. Grohs, A. B. Balantekin

The mechanism for generating neutrino masses remains a puzzle in particle physics. If neutrino masses follow from a Dirac mass term, then neutrino states exist with opposite chiral…

astro-ph.CO2023★ 2 cited

Big Bang Nucleosynthesis

Evan Grohs, George M. Fuller

As the early universe expands and cools the rates of the weak interactions that keep neutrinos in thermal equilibrium with the matter and the related rates of the reactions that in…