2.3k citations
- Russian Academy of SciencesRU90 papers
- Centre National de la Recherche ScientifiqueFR42 papers
- Ioffe InstituteRU36 papers
- University of OsloNO36 papers
- Petersburg Nuclear Physics InstituteRU31 papers
- University of AveiroPT29 papers
- Karlsruhe Institute of TechnologyDE21 papers
- Argonne National LaboratoryUS19 papers
- Peter the Great St. Petersburg Polytechnic UniversityRU19 papers
- University of RegensburgDE19 papers
- Hebrew University of JerusalemIL15 papers
- St Petersburg UniversityRU14 papers
14 papers · 2 filters
Magnetic Hydrogen Atmosphere Models and the Neutron Star RX J1856.5-3754
Wynn C. G. Ho, David L. Kaplan, Philip Chang +2
RX J1856.5-3754 is one of the brightest nearby isolated neutron stars, and considerable observational resources have been devoted to it. However, current models are unable to satis…
Two-Photon 2s<->1s Transitions during Recombination of Hydrogen in the Universe
E. E. Kholupenko, A. V. Ivanchik
Based on the standard cosmological model, we calculate the correction to the rate of two-photon 2s<->1s transitions in the hydrogen atom under primordial hydrogen plasma recombinat…
Heat blanketing envelopes and thermal radiation of strongly magnetized neutron stars
A. Y. Potekhin, G. Chabrier, D. G. Yakovlev
Strong (B >> 10^9 G) and superstrong (B > 10^{14} G) magnetic fields profoundly affect many thermodynamic and kinetic characteristics of dense plasmas in neutron star envelopes. In…
Fusion reactions in multicomponent dense matter
D. G. Yakovlev, L. R. Gasques, M. Beard +2
We analyze thermonuclear and pycnonuclear fusion reactions in dense matter containing atomic nuclei of different types. We extend a phenomenological expression for the reaction rat…
Study of the spring and autumn daemon-flux maxima at the Baksan Neutrino Observatory
E. M. Drobyshevski, M. E. Drobyshevski
Detection of daemons in low-background conditions in September 2005 and March 2006 has provided evidence for the expected to occur at that times maxima in the flux of daemons with…
Rotochemical Heating of Neutron Stars: Rigorous Formalism with Electrostatic Potential Perturbations
Andreas Reisenegger, Paula Jofre, Rodrigo Fernandez +1
The electrostatic potential that keeps approximate charge neutrality in neutron star matter is self-consistently introduced into the formalism for rotochemical heating presented in…