在天体物理能量下偏振光子的氘核光分解

IF 3.2 2区 物理与天体物理 Q2 PHYSICS, NUCLEAR
G. Ramachandran, Y. Y. Oo, S. Shilpashree
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引用次数: 4

摘要

在杜克大学自由电子激光实验室进行了精确的实验研究之后,我们使用一种独立于模型的理论方法,同时将M1和E1振幅结合在一起,讨论了具有100%线极化光子的氘核的光衰变。同标量M1{下标s}的贡献也被精确地考虑在内。从现有的双极化热中子捕获实验测量中可以看出,等标量M1{sub s}的贡献可能与实验测量的与大爆炸核合成(BBN)相关能量的截面具有相同的数量级。因此,建议对氘核光分解进行适当的测量,以经验性地确定天体物理能量的M1{sub s}贡献。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Deuteron photodisintegration with polarized photons at astrophysical energies
Following precise experimental studies at the Duke Free-Electron Laser Laboratory, we discuss the photodisintegration of deuterons with 100% linearly polarized photons using a model independent theoretical approach taking together M1 and E1 amplitudes simultaneously. The isoscalar M1{sub s} contribution is also taken exactly into account. From the existing experimental measurement on doubly polarized thermal neutron capture, it is seen that the isoscalar M1{sub s} contribution could be of the same order of magnitude as the experimentally measured cross sections at energies relevant to Big Bang Nucleosynthesis (BBN). Therefore appropriate measurements on deuteron photodisintegration are suggested to empirically determine the M1{sub s} contribution at astrophysical energies.
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来源期刊
Physical Review C
Physical Review C PHYSICS, NUCLEAR-
CiteScore
5.80
自引率
35.50%
发文量
863
期刊介绍: Physical Review C (PRC) is a leading journal in theoretical and experimental nuclear physics, publishing more than two-thirds of the research literature in the field. PRC covers experimental and theoretical results in all aspects of nuclear physics, including: Nucleon-nucleon interaction, few-body systems Nuclear structure Nuclear reactions Relativistic nuclear collisions Hadronic physics and QCD Electroweak interaction, symmetries Nuclear astrophysics
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