Results 11 to 20 of about 80,732 (246)
Different to the core: the pre-supernova structures of massive single and binary-stripped stars [PDF]
The majority of massive stars live in binary or multiple systems and will interact during their lifetimes, which helps to explain the observed diversity of core-collapse supernovae.
E. Laplace+6 more
semanticscholar +1 more source
Muonic Boson Limits: Supernova Redux [PDF]
We derive supernova (SN) bounds on muon-philic bosons, taking advantage of the recent emergence of muonic SN models. Our main innovations are to consider scalars $\phi$ in addition to pseudoscalars $a$ and to include systematically the generic two-photon
A. Caputo, G. Raffelt, E. Vitagliano
semanticscholar +1 more source
Supernovae and their scientific secrets
Supernovae are the most gorgeous fireworks that people can observe in the universe. Their explosion can produce a maximum luminosity 10 billion times that of the Sun, helping scientists see farther.
LI Zhihong+8 more
doaj +1 more source
SNEWS 2.0: a next-generation supernova early warning system for multi-messenger astronomy [PDF]
The next core-collapse supernova in the Milky Way or its satellites will represent a once-in-a-generation opportunity to obtain detailed information about the explosion of a star and provide significant scientific insight for a variety of fields because ...
S. A. Kharusi+70 more
semanticscholar +1 more source
Swope Supernova Survey 2017a (SSS17a), the optical counterpart to a gravitational wave source [PDF]
Photons from a gravitational wave event Two neutron stars merging together generate a gravitational wave signal and have also been predicted to emit electromagnetic radiation. When the gravitational wave event GW170817 was detected, astronomers rushed to
D. Coulter+20 more
semanticscholar +1 more source
Improved axion emissivity from a supernova via nucleon-nucleon bremsstrahlung [PDF]
The most efficient axion production mechanism in a supernova (SN) core is the nucleon-nucleon bremsstrahlung. This process has been often modeled at the level of the vacuum one-pion exchange (OPE) approximation. Starting from this naive recipe, we revise
Pierluca Carenza+5 more
semanticscholar +1 more source
The electron-capture origin of supernova 2018zd [PDF]
In the transitional mass range (~8–10 solar masses) between white dwarf formation and iron core-collapse supernovae, stars are expected to produce an electron-capture supernova.
D. Hiramatsu+29 more
semanticscholar +1 more source
We analyze the expected arrival time spectrum of supernova neutrinos using simulated luminosity and compute the expected number of events in future detectors such as the DUNE Far Detector and Hyper-Kamiokande.
Celio A. Moura+2 more
doaj +1 more source
Improved cosmological constraints from a joint analysis of the SDSS-II and SNLS supernova samples [PDF]
Aims. We present cosmological constraints from a joint analysis of type Ia supernova (SN Ia) observations obtained by the SDSS-II and SNLS collaborations.
M. Betoule+71 more
semanticscholar +1 more source
A revised catalogue of 294 Galactic supernova remnants [PDF]
A revised catalogue of Galactic supernova remnants (SNRs) is presented, along with some simple statistics of their properties. Six new SNRs have been added to the catalogue since the previous published version from 2014, and six entries have been removed,
D. Green
semanticscholar +1 more source