The shape of the neutrino pulse from the supernova SN1987a provides one of the most stringent constraints on the size of large, compact, "gravity-only" extra dimensions. Previously, calculations have been carrie
Work which discussed the physical situation involved in CEE was published before 1976 (Bisnovatyi-Kogan and Sunyaev 1971; Sparks et al. 1974; Refsdal et al. 1974), and interest in such cases helped to inspire the realization that CEE might be a formation mechanism for close binaries. None...