Results 1 to 10 of about 188,615 (124)

Detailed Geant4 simulations of the ANITA and ANITA-CUP neutron facilities [PDF]

open access: yes, 2015
Simulations of the ANITA spallation neutron source at The Svedberg Laboratory (TSL) are described. Neutron radiation calculations show close agreement with measurements at both standard and close user positions.
Hong, Q.   +3 more
core   +1 more source

THERMAL RADIATION FROM COOLING NEUTRON STARS [PDF]

open access: yesTexas in Tuscany, 2003
To be published in the Proceedings of the XXI Texas Symposium on Relativistic ...
Pavlov, G., Zavlin, V.
openaire   +3 more sources

Polarization of Thermal X-rays from Isolated Neutron Stars [PDF]

open access: yes, 1999
Since the opacity of a magnetized plasma depends on polarization of radiation, the radiation emergent from atmospheres of neutron stars with strong magnetic fields is expected to be strongly polarized. The degree of linear polarization, typically ~10-30%,
Becker W.   +17 more
core   +3 more sources

Effects of Neutron Irradiations in Various Crystal Samples of Large Size for Future Crystal Calorimeter [PDF]

open access: yes, 2010
In this paper, we report an investigation on the radiation damage effects induced by neutrons in large size crystal scintillator: BGO, CeF_3, LYSO:Ce and PWO. The irradiations were carried out by using fast neutrons from one ^(241)Am-Be and two ^(252)
Mao, Rihua, Zhang, Liyuan, Zhu, Ren-Yuan
core   +1 more source

Radiation of Neutron Stars Produced by Superfluid Core [PDF]

open access: yes, 2002
We find that neutron star interior is transparent for collisionless electron sound, the same way as it is transparent for neutrinos. In the presence of magnetic field the electron sound is coupled with electromagnetic radiation and form the fast ...
Amundsen L.   +17 more
core   +2 more sources

Gravitational Radiation Instability in Hot Young Neutron Stars [PDF]

open access: yes, 1998
We show that gravitational radiation drives an instability in hot young rapidly rotating neutron stars. This instability occurs primarily in the l=2 r-mode and will carry away most of the angular momentum of a rapidly rotating star by gravitational ...
Benjamin J. Owen   +12 more
core   +2 more sources

Coalescing Binary Neutron Stars [PDF]

open access: yes, 1999
Coalescing compact binaries with neutron star or black hole components provide the most promising sources of gravitational radiation for detection by the LIGO/VIRGO/GEO/TAMA laser interferometers now under construction.
Abramovici M   +87 more
core   +2 more sources

Gravitational Waves from Low-Mass X-ray Binaries: a Status Report [PDF]

open access: yes, 2000
We summarize the observations of the spin periods of rapidly accreting neutron stars. If gravitational radiation is responsible for balancing the accretion torque at the observed spin frequencies of ~300 Hz, then the brightest of these systems make ...
Bildsten, Lars   +2 more
core   +3 more sources

Mutagenic effects of tumorigenic neutron radiation [PDF]

open access: yesInternational Journal of Cancer, 1996
A fraction of thymic lymphomas induced by high LET neutron radiation contains activating mutations (single-base substitutions) in the ras genes. To determine whether such mutations are the result of the interaction of high LET radiation with cellular DNA, we have utilized an in vitro model system to screen and isolate neutron-radiation-induced mutants.
A, Garcia-Espana   +3 more
openaire   +2 more sources

Collective neutrino-pair emission due to Cooper pairing of protons in superconducting neutron stars [PDF]

open access: yes, 2000
The neutrino emission due to formation and breaking of Cooper pairs of protons in superconducting cores of neutron stars is considered with taking into account the electromagnetic coupling of protons to ambient electrons.
Amundsen   +24 more
core   +4 more sources

Home - About - Disclaimer - Privacy