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

High energy solar neutrinos can come from the hep reaction ^3He(p,\nue^+)^4Hewith a large end point energy of 18.8 MeV. Understanding the hep reaction maybe important for interpreting solar neutrino spectra. We calculate thecontribution of the axial charge transition $^3P_0\to ^1S_0$ to the hepthermonuclear S factor using a one-body reaction model involving a nucleonmoving in optical potentials. Our result is comparable to or larger thanprevious calculations of the s-wave Gamow Teller contribution. This indicatesthat the hep reaction may have p-wave strength leading to an enhancement of theS factor.Comment: 4 pages, 1 ps figure, very minor changes, Phys. Rev. C in pres

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

High energy solar neutrinos and<i>p</i>-wave contributions to<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msup><mml:mrow /><mml:mrow><mml:mn>3</mml:mn></mml:mrow></mml:msup></mml:mrow><mml:mi mathvariant="normal">He</mml:mi><mml:mo>(</mml:mo><mml:mi>p</mml:mi><mml:mo>,</mml:mo><mml:mi>ν</mml:mi><mml:mrow><mml:msup><mml:mrow><mml:mi>e</mml:mi></mml:mrow><mml:mrow><mml:mo>+</mml:mo></mml:mrow></mml:msup></mml:mrow><mml:mrow><mml:msup><mml:mrow><mml:mo…

High energy solar neutrinos andp-wave contributions to3He(p,νe+