Results 161 to 170 of about 200,313 (264)

THE HE-RICH CORE-COLLAPSE SUPERNOVA 2007Y: OBSERVATIONS FROM X-RAY TO RADIO WAVELENGTHS [PDF]

open access: bronze, 2009
Maximilian Stritzinger   +47 more
openalex   +1 more source

Simulations of Electron Capture and Low-Mass Iron Core Supernovae

open access: yes, 2017
The evolutionary pathways of core-collapse supernova progenitors at the low-mass end of the spectrum are beset with major uncertainties. In recent years, a variety of evolutionary channels has been discovered in addition to the classical electron capture
Gay, D.   +5 more
core  

BLUE SUPERGIANT MODEL FOR ULTRA-LONG GAMMA-RAY BURST WITH SUPERLUMINOUS-SUPERNOVA-LIKE BUMP [PDF]

open access: bronze, 2013
Daisuke Nakauchi   +7 more
openalex   +1 more source

Supernova Relic Electron Neutrinos and anti-Neutrinos in future Large-scale Observatories

open access: yes, 2007
We investigate the signal from supernova relic neutrinos in future large scale observatories, such as MEMPHYS (UNO, Hyper-K), LENA and GLACIER, at present under study.
Volpe, C., Welzel, J.
core   +1 more source

Dips in the diffuse supernova neutrino background [PDF]

open access: hybrid, 2014
Yasaman Farzan   +3 more
openalex   +1 more source

New effects of non-standard self-interactions of neutrinos in a supernova [PDF]

open access: green, 2017
Anirban Das   +5 more
openalex   +1 more source

LAMOST J1010+2358 is not a Pair-Instability Supernova Relic

open access: yesThe Open Journal of Astrophysics
The discovery of a star formed out of pair-instability supernova ejecta would have massive implications for the Population III star initial mass function and the existence of stars over 100 Msun, but none have yet been found.
Pierre Thibodeaux   +4 more
doaj   +1 more source

COSMIC-RAY STREAMING FROM SUPERNOVA REMNANTS AND GAMMA-RAY EMISSION FROM NEARBY MOLECULAR CLOUDS [PDF]

open access: bronze, 2012
Huirong Yan   +5 more
openalex   +1 more source

Shedding light on the Δm212 tension with supernova neutrinos

open access: yesPhysics Letters B
One long-standing tension in the determination of neutrino parameters is the mismatched value of the solar mass square difference, Δm212, measured by different experiments: the reactor antineutrino experiment KamLAND finds a best fit larger than the one ...
Rasmi Hajjar   +2 more
doaj   +1 more source

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