Results 31 to 40 of about 6,843,697 (359)
Bias Effects on g- and s-Factors in Westcott Convention
Applied Sciences, 2021 For accuracy improvement of neutron activation analysis and neutron capture cross sections, bias effects are investigated on g- and s-factors in the Westcott convention.
Hideo Harada
doaj +1 more source
Constraining the Neutron Star Mass–Radius Relation and Dense Matter Equation of State with NICER. I. The Millisecond Pulsar X-Ray Data Set [PDF]
Astrophysical Journal, 2019 We present the set of deep Neutron Star Interior Composition Explorer (NICER) X-ray timing observations of the nearby rotation-powered millisecond pulsars PSRs J0437−4715, J0030+0451, J1231−1411, and J2124−3358, selected as targets for constraining the ...
S. Bogdanov +31 more
semanticscholar +1 more source
Materials & Design, 2021 The effects of vacuum induction melting (VIM) vacuum (
Liang Zheng +6 more
doaj
Research on Neutronics Safety Parameters of the AP1000 Nuclear Reactor under Different Conditions
Energies, 2023 Changes in temperature during reactor operation may cause changes in physical parameters, leading to core overheating and accidents. It is essential to analyze and assess the safety parameters of the core under different operating conditions.
Xinyi Niu +4 more
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Radiation, 2023 Accelerated neutron tests on silicon (Si) and silicon carbide (SiC) power MOSFETs at different temperatures and drain bias voltages were performed at the ChipIr facility (Didcot, UK).
Fabio Principato +5 more
doaj +1 more source
Stellar neutron spectra at 28 keV thermal temperature [PDF]
EPJ Web of Conferences, 2023 To calculate the reaction rate in the neutron capture processes it is common to work with the Maxwellian Average Cross Section (MACS), defined as the reaction rate scaled by the most probable neutron velocity of the Maxwell-Boltzmann distribution.
Musacchio-González Elizabeth +2 more
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On the spreading layer emission in luminous accreting neutron stars [PDF]
, 2013 Emission of the neutron star surface potentially contains information about its size and thus of vital importance for high energy astrophysics. In spite of the wealth of data on the emission of luminous accreting neutron stars, the emission of their ...
Poutanen, Juri +2 more
core +4 more sources
Temperature Distribution in Magnetized Neutron Star Crusts [PDF]
Astronomy & Astrophysics, 2004 We investigate the influence of different magnetic field configurations on the temperature distribution in neutron star crusts. We consider axisymmetric dipolar fields which are either restricted to the stellar crust, ``crustal fields'', or allowed to penetrate the core, ``core fields''. By integrating the two-dimensional heat transport equation in the
Ulrich Geppert, Dany Page, M. Kueker
openaire +4 more sources
Peering into the Dark Side: Magnesium Lines Establish a Massive Neutron Star in PSR J2215+5135 [PDF]
, 2018 New millisecond pulsars (MSPs) in compact binaries provide a good opportunity to search for the most massive neutron stars. Their main-sequence companion stars are often strongly irradiated by the pulsar, displacing the effective center of light from ...
M. Linares, T. Shahbaz, J. Casares
semanticscholar +1 more source
Forecasting Neutron Star Temperatures: Predictability and Variability [PDF]
Physical Review Letters, 2013 5 pages, 3 figures. Submitted to Phys.
Dany Page, Sanjay Reddy
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