The strongest upper bounds on the axion mass come from astrophysical observations like the neutrino burst duration of SN1987A, which depends on the ax......
Bjorkeroth, F; Di Luzio, L; Mescia, F; Nardi, E; Panci, P; Ziegler, R
Bjorkeroth, F; Nardi, E (corresponding author), Ist Nazl Fis Nucl, Lab Nazl Frascati, CP 13, I-100044 Frascati, Italy.; Di Luzio, L (corresponding author), Deutsch Elektronen Synchrotron DESY, Notkestr 85, D-22607 Hamburg, Germany.; Di Luzio, L; Panci, P (corresponding author), Univ Pisa, Dipartimento Fis, Largo B Pontecorvo 3, I-56127 Pisa, Italy.; Di Luzio, L; Panci, P (corresponding author), Ist Nazl Fis Nucl, Sez Pisa, Largo B Pontecorvo 3, I-56127 Pisa, Italy.; Mescia, F (corresponding author), Univ Barcelona, Inst Ciencies Cosmos ICCUB, Dept Fis Quant & Astrofis, Marti Franques 1, E-08028 Barcelona, Spain.; Ziegler, R (corresponding author), CERN, Theoret Phys Dept, CH-1211 Geneva 23, Switzerland.; Panci, P (corresponding author), Lab Nazl Gran Sasso, Via G Acitelli 22, I-67100 Assergi, AQ, Italy.
PHYSICAL REVIEW D, 2020; 101 (3):