Helium Burning Reactions in Stars
Author(s) -
H. L. Duorah
Publication year - 1962
Publication title -
progress of theoretical physics
Language(s) - English
Resource type - Journals
eISSN - 1347-4081
pISSN - 0033-068X
DOI - 10.1143/ptp.28.585
Subject(s) - physics , helium , stars , range (aeronautics) , astrophysics , atmospheric temperature range , atomic physics , nuclear physics , production rate , ion , thermodynamics , industrial engineering , engineering , materials science , quantum mechanics , composite material
Helium burning reactlon rates are calculated with experimental information at temperatures in the ranges 1 to 2 x 10⁸ and 3 to 6 x 10⁸ deg K. A fresh supply of helium at the higher range of temperatures may come from certain heavy-ion reactions. At lower temperature ranges Ne²⁰ production rate is found to be too slow. (auth)
Accelerating Research
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom
Address
John Eccles HouseRobert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom