We re-examine the very stringent limits on the axion mass based on the strength and duration of the neutrino signal from SN 1987A, in the light of new measurements of the axial-vector coupling strength of nucleons, possible suppression of axion emission due to many-body effects, and additional emission processes involving pions. The suppression of axion emission due to nucleon spin fluctuations induced by many-body effects degrades previous limits by a factor of about 2. Emission processes involving thermal pions can strengthen the limits by a factor of 3-4 within a perturbative treatment that neglects saturation of nucleon spin fluctuations. Inclusion of saturation effects, however, tends to make the limits less dependent on pion abundance...
Direct Chandra observations of a surface temperature of isolated neutron star in Cassiopeia A (Cas A...
We study the impact of axion emission in simulations of massive star explosions, as an additional so...
The most efficient axion production mechanism in a supernova (SN) core is the nucleon-nucleon bremss...
We re-examine the very stringent limits on the axion mass based on the strength and duration of the ...
The effect of free-streaming axion emission on numerical models for the cooling of the newly born ne...
Observations of the cosmological large-scale structure provide well-established neutrino mass limits...
Supernovae provide fascinating opportunities to study various particles and their interactions. Amon...
Nucleon-nucleon, axion bremsstrahlung is the primary mechanism for axion emission from the nascent n...
If an axion of mass between about 10(exp -3) and 10 eV exists, axion emission would have significant...
Axion emission by hot and dense plasmas is a new energy-loss channel for stars. Observational conseq...
Relic thermal axions could play the role of an extra hot dark matter component in cosmological struc...
An axion with a mass greater than 1 eV should be detectable through its decay into two photons. The ...
There are a number of observational hints from astrophysics which point to the existence of stellar ...
We study the impact of axion emission in simulations of massive star explosions, as an additional so...
A review of the status of axions and axion-like particles is given. Special attention is devoted to ...
Direct Chandra observations of a surface temperature of isolated neutron star in Cassiopeia A (Cas A...
We study the impact of axion emission in simulations of massive star explosions, as an additional so...
The most efficient axion production mechanism in a supernova (SN) core is the nucleon-nucleon bremss...
We re-examine the very stringent limits on the axion mass based on the strength and duration of the ...
The effect of free-streaming axion emission on numerical models for the cooling of the newly born ne...
Observations of the cosmological large-scale structure provide well-established neutrino mass limits...
Supernovae provide fascinating opportunities to study various particles and their interactions. Amon...
Nucleon-nucleon, axion bremsstrahlung is the primary mechanism for axion emission from the nascent n...
If an axion of mass between about 10(exp -3) and 10 eV exists, axion emission would have significant...
Axion emission by hot and dense plasmas is a new energy-loss channel for stars. Observational conseq...
Relic thermal axions could play the role of an extra hot dark matter component in cosmological struc...
An axion with a mass greater than 1 eV should be detectable through its decay into two photons. The ...
There are a number of observational hints from astrophysics which point to the existence of stellar ...
We study the impact of axion emission in simulations of massive star explosions, as an additional so...
A review of the status of axions and axion-like particles is given. Special attention is devoted to ...
Direct Chandra observations of a surface temperature of isolated neutron star in Cassiopeia A (Cas A...
We study the impact of axion emission in simulations of massive star explosions, as an additional so...
The most efficient axion production mechanism in a supernova (SN) core is the nucleon-nucleon bremss...