scholarly journals Parameter-free effective field theory calculation for the solar proton-fusion and hep processes

2003 ◽  
Vol 67 (5) ◽  
Author(s):  
T.-S. Park ◽  
L. E. Marcucci ◽  
R. Schiavilla ◽  
M. Viviani ◽  
A. Kievsky ◽  
...  
2006 ◽  
Vol 643 (5) ◽  
pp. 263-267 ◽  
Author(s):  
H. Sadeghi ◽  
S. Bayegan ◽  
Harald W. Grießhammer

2013 ◽  
Vol 720 (4-5) ◽  
pp. 385-388 ◽  
Author(s):  
Jiunn-Wei Chen ◽  
C.-P. Liu ◽  
Shen-Hsi Yu

1984 ◽  
Vol 232 (1) ◽  
pp. 61-72 ◽  
Author(s):  
Andrew Cohen ◽  
Howard Georgi ◽  
Benjamin Grinstein

1999 ◽  
Vol 449 (1-2) ◽  
pp. 1-5 ◽  
Author(s):  
David B. Kaplan ◽  
Martin J. Savage ◽  
Roxanne P. Springer ◽  
Mark B. Wise

2007 ◽  
Vol 22 (25n28) ◽  
pp. 2143-2151 ◽  
Author(s):  
TAE-SUN PARK

A modern effective field theory is exploited to pin down accurately the flux S factors for the pp and hep processes in the Sun. The technique used is to combine the high accuracy established in few-nucleon systems of the "standard nuclear physics approach" (SNPA) and the systematic power counting of chiral perturbation theory (ChPT) into a consistent effective field theory framework. Using highly accurate wave functions obtained in the SNPA and working to N 3 LO in the chiral counting for the current, we make totally parameter-free and error-controlled predictions for the pp and hep processes in the Sun. We also discuss the convergence with respect to chiral expansion.


Sign in / Sign up

Export Citation Format

Share Document