Abstract:
Polarization of photons emitted in weak decays occuring at distant star allows to
determine
whether this star is made from antimatter. Even more promissing is the observation of
neutrinos (antineutrinos) produced at neutronization (antineutronization) reactions at the
beginning of SN (¯SN) explosion.
Citation:
A. D. Dolgov, V. A. Novikov, M. I. Vysotsky, “How to see an antistar”, Pis'ma v Zh. Èksper. Teoret. Fiz., 98:9 (2013), 587–590; JETP Letters, 98:9 (2013), 519–522
Dolgov A.D., 3Rd International Conference on New Frontiers in Physics, Epj Web of Conferences, 95, ed. Bravina L. Foka Y. Kabana S., E D P Sciences, 2015, 03007
A.D. Dolgov, L. Bravina, Y. Foka, S. Kabana, EPJ Web of Conferences, 95 (2015), 03007
Dolgov A.D., 2Nd International Conference on New Frontiers in Physics, Epj Web of Conferences, 71, eds. Bravina L., Foka Y., Kabana S., E D P Sciences, 2014, 00040