1.2k citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Russian Academy of SciencesRU133 papers
- Lomonosov Moscow State UniversityRU72 papers
- National Research Tomsk State UniversityRU34 papers
- Institute of Solar-Terrestrial PhysicsRU32 papers
- Universitat de ValènciaES27 papers
- Troitsk Institute for Innovation and Fusion ResearchRU23 papers
- Universidade de São PauloBR21 papers
- Chinese Academy of SciencesCN20 papers
- Instituto de Física CorpuscularES19 papers
- Institute for High Energy PhysicsES18 papers
- National Astronomical ObservatoriesCN18 papers
- Kurchatov InstituteRU17 papers
11 papers · 1 filter
Plasma effects in neutrino-pair emission due to Cooper pairing of protons in superconducting neutron stars
L. B. Leinson
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…
Direct Urca processes in superdense cores of neutron stars
L. B. Leinson
We use the field theoretical model to perform relativistic calculations of neutrino energy losses caused by the direct Urca processes on nucleons in the degenerate baryon matter. B…
Large mixing angle oscillations as a probe of the deep solar interior
C. Burgess, N. S. Dzhalilov, M. Maltoni +4
We re-examine the sensitivity of solar neutrino oscillations to noise in the solar interior using the best current estimates of neutrino properties. Our results show that the measu…
Confronting Spin Flavor Solutions of the Solar Neutrino Problem with current and future solar neutrino data
J. Barranco, O. G. Miranda, T. I. Rashba +2
We show that spin flavor precession solutions to the solar neutrino problem, although preferred by the latest solar data, are ruled out by the first results from the KamLAND reacto…
Direct Urca processes on nucleons in cooling neutron stars
L. B. Leinson
We use the field theoretical model to perform relativistic calculations of neutrino energy losses caused by the direct Urca processes on nucleons in the degenerate baryon matter. B…
Weak magnetism effects in the direct Urca processes in cooling neutron stars
L. B. Leinson
In the mean field approximation, we study the effects of weak magnetism and pseudoscalar interaction in the neutrino energy losses caused by the direct Urca processes on relativist…
Generation of Flows in the Solar Chromosphere Due to Magnetofluid Coupling
Swadesh M. Mahajan, Komunela I. Nikol'skaya, Nana L. Shatashvili +1
It is shown that a generalized magneto-Bernoulli mechanism can effectively generate high velocity flows in the Solar chromosphere by transforming the plasma pressure energy into ki…
On the Influence of Einstein-Podolsky-Rosen Effect on the Domain Wall Formation during the Cosmological Phase Transitions
Yu. V. Dumin
Search for the mechanisms suppressing formation of Higgs field defects (e.g. domain walls) during the cosmological phase transitions is one of key problems in explanation of the ob…
On a probable manifestation of Hubble expansion at the local scales, as inferred from LLR data
Yu. V. Dumin
Processing the data of lunar laser ranging (LLR), whose accuracy now reaches a few millimeters, points to the effect of anomalous increase in the lunar semimajor axis (with an exce…
Eigenoscillations of the differentially rotating Sun: II. Generalization of Laplace's tidal equation
N. S. Dzhalilov, J. Staude
The general PDE governing linear, adiabatic, nonraradial oscillations in a spherical, differentially and slowly rotating non-magnetic star is derived. This equation describes mainl…
Eigenoscillations of the Differentially Rotating Sun: I. 22-year, 4000-year, and quasi-biennial modes
N. S. Dzhalilov, J. Staude, V. N. Oraevsky
Retrograde waves with frequencies much lower than the rotation frequency become trapped in the solar radiative interior. The eigenfunctions of the compressible, nonadiabatic, Rossb…