English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Tools annual

Global: Zendy Free Plan

Global: Zendy Tools monthly

Global: Zendy Plus monthly

We extend the virial equation of state to include 3H and 3He nuclei, andpredict significant mass-three fractions near the neutrinosphere in supernovae.While alpha particles are often more abundant, we demonstrate that energytransfer cross-sections for muon and tau neutrinos at low densities aredominated by breakup of the loosely-bound 3H and 3He nuclei. The virialcoefficients involving A=3 nuclei are calculated directly from thecorresponding nucleon-3H and nucleon-3He scattering phase shifts. For theneutral-current inelastic cross-sections and the energy transfer crosssections, we perform ab-initio calculations based on microscopic two- andthree-nucleon interactions and meson-exchange currents.Comment: 6 pages, 2 figures, minor additions, to appear in Phys. Rev.

physical review. c. nuclear physics/physical review. c, nuclear physics

Neutrino breakup of<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>A</mml:mi><mml:mo>=</mml:mo><mml:mn>3</mml:mn></mml:mrow></mml:math>nuclei in supernovae

Neutrino breakup ofA=3nuclei in supernovae