Advancement of Photospheric Radius Expansion and Clocked Type-I X-Ray Burst Models with the New Mg22(α,p)Al25 Reaction Rate Determined at the Gamow Energy-Reference-Cited by-同舟云学术

Advancement of Photospheric Radius Expansion and Clocked Type-I X-Ray Burst Models with the New Mg22(α,p)Al25 Reaction Rate Determined at the Gamow Energy

Published:2021-10-19 Issue:17 Volume:127 Page:
ISSN:0031-9007
Container-title:Physical Review Letters
language:en
Short-container-title:Phys. Rev. Lett.

Author:

Hu J.^ORCID,Yamaguchi H.^ORCID,Lam Y. H.^ORCID,Heger A.^ORCID,Kahl D.^ORCID,Jacobs A. M.,Johnston Z.^ORCID,Xu S. W.,Zhang N. T.,Ma S. B.,Ru L. H.,Liu E. Q.,Liu T.^ORCID,Hayakawa S.^ORCID,Yang L.^ORCID,Shimizu H.,Hamill C. B.,Murphy A. St J.,Su J.^ORCID,Fang X.,Chae K. Y.,Kwag M. S.,Cha S. M.,Duy N. N.^ORCID,Uyen N. K.,Kim D. H.,Pizzone R. G.^ORCID,La Cognata M.^ORCID,Cherubini S.,Romano S.^ORCID,Tumino A.,Liang J.,Psaltis A.,Sferrazza M.,Kim D.,Li Y. Y.,Kubono S.

Funder

Major State Basic Research Development Program of China

Chinese Academy of Sciences

Japan Society for the Promotion of Science

Ministry of Education, Culture, Sports, Science and Technology

National Natural Science Foundation of China

Science and Technology Facilities Council

Australian Research Council

ARC Centre of Excellence for All-Sky Astrophysics

National Science Foundation

National Research Foundation of Korea

Fonds De La Recherche Scientifique - FNRS