Speaker
Mr
Longhui Ru
Description
The 511 keV gamma rays and below emitted by novae are mainly produced by 18F, the flux may be detected by satellite detectors. We can effectively constrain the novae model by comparing the theory and observation results. As the main consumed reaction of 18F, 18F(p,α)15O, its reaction rate is extremely important and has been invested for decades. This poster is mainly to introduce the gamma rays from novae and progress in studying the 18F(p,α)15O reaction rate at nova temperature.
Primary author
Mr
Longhui Ru
