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Supernova Remnants: Types and Evolution
Although only a small fraction of stars end their lives as supernovae, all supernovae leave behind a supernova remnant (SNR), an expanding shock wave... -
Diffuse Supernova Neutrino Background
Neutrinos are the second most ubiquitous Standard Model particles in the universe. On the other hand, they are also the ones least likely to... -
Revisiting progenitor-age dependence of type Ia supernova luminosity standardization process
Much of the research in supernova cosmology is based on an assumption that the peak luminosity of type Ia supernovae (SNe Ia), after a...
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Oscillations of Majorana Neutrinos in Supernova and CP Vviolation
AbstractLeptonic CP violation is one of the most important topics in neutrino physics. CP violation in the neutrino sector is strongly related to the...
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A superluminous supernova lightened by collisions with pulsational pair-instability shells
Superluminous supernovae are among the most energetic stellar explosions in the Universe, but their energy sources remain an open question. Here we...
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Cosmogenic Isotopes in Lunar Soil: Solar Activity and the Exploding of Nearby Supernova
AbstractLunar soil is a natural detector of cosmic rays (CRs) of different origins (solar and Galactic). Analysis of the depth profiles of cosmogenic...
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Theoretical Implications of the Gamma-Ray Burst-Supernova Connection
Although observations of circumstellar shock interactions around supernovae are generally consistent with a... -
Thermal Processes in Supernova Remnants
This chapter provides a theoretical overview of thermal processes in supernova remnants (SNRs), which can be understood as a series of energy... -
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Magnetorotational Supernova Neutrino Emission Spectra and Prospects for Observations by Large-Size Underwater Telescopes
AbstractWe analyze neutrino fluxes near the surface of a protoneutron star in type II supernova explosions. For magnetorotational explosion mechanism...
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Comparative Modeling of the 2012b Outburst of Supernova 2009ip
AbstractThe September 2012 outburst of the type IIn supernova 2009ip was simulated using two independent codes, STELLA and FRONT. The
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The Jet and the Supernova in GRB 990712
We show that the polarization measurements of GRB 990712 can be interpreted as originating in a modestly spreading jet. For that interpretation to be... -
Supernova Neutrino Spectra and Observations by Large Volume Telescopes
AbstractThe energy spectra of neutrinos of type II supernovae under various explosion mechanisms are considered. For dynamo active supernovae it is...
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A precursor interpretation for the Crab supernova 1054 A.D. very early light curve
In spite that the Crab supernova in 1054 A.D. was studied over the years, it is still not clear what type of event produced the explosion. The most...
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Supernova Dynamo Effect in Neutrino Spectra and Perspective of Observations by Large Volume Telescopes
AbstractNeutrino fluxes near the surface of a protoneutron star in type II supernovae are studied. For dynamoactive supernovae it is shown that...
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Diffuse Supernova Neutrino Background
Neutrinos are the second most ubiquitous Standard Model particles in the universe. On the other hand, they are also the ones least likely to... -
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Supernova 2009ip Outbursts in 2012: From Scenario to Model
AbstractSpherical and aspherical models are presented for two outbursts in 2012 of supernova 2009ip. Models are based on a scenario which suggests...
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Thermal Processes in Supernova Remnants
This chapter provides a theoretical overview of thermal processes in supernova remnants (SNRs), which can be understood as a series of energy...