activity
20002015
most citedCooling of Neutron Stars. Hadronic Model

119 citations · 215 across the 6 of their papers we have counts for

collaborators

6 papers

nucl-th2015★ 6 cited

Hyperon puzzle and the RMF model with scaled hadron masses and coupling constants

E. E. Kolomeitsev, K. A. Maslov, D. N. Voskresensky

The equation of state of cold baryonic matter is studied within a relativistic mean-field model with hadron masses and coupling constants depending on a scalar field. We demonstrat…

astro-ph.HE2015★ 61 cited

Relativistic Mean-Field Models with Scaled Hadron Masses and Couplings: Hyperons and Maximum Neutron Star Mass

K. A. Maslov, E. E. Kolomeitsev, D. N. Voskresensky

An equation of state of cold nuclear matter with an arbitrary isotopic composition is studied within a relativistic mean-field approach with hadron masses and coupling constants de…

astro-ph2005★ 3 cited

Cooling of Neutron Stars and 3P_2 neutron gap

H. Grigorian, D. N. Voskresensky

We study the dependence of the cooling of isolated neutron stars on the magnitude of the neutron gap. It is demonstrated that our ``Nuclear medium cooling scenario'' is in f…

astro-ph2004★ 119 cited

Cooling of Neutron Stars. Hadronic Model

D. Blaschke, H. Grigorian, D. N. Voskresensky

We study the cooling of isolated neutron stars. The main cooling regulators are introduced: EoS, thermal transport, heat capacity, neutrino and photon emissivity, superfluid nucleo…

nucl-th2002★ 3 cited

Resonance states below pion-nucleon threshold and their consequences for nuclear systems

E. E. Kolomeitsev, D. N. Voskresensky

Regular sequences of narrow peaks have been observed in the missing mass spectra in the reactions pp --> p pi^+ X and pd --> ppX_1 below pion-production threshold. They are interpr…

astro-ph2000★ 23 cited

Rearrangement of the Fermi Surface of Dense Neutron Matter and Direct Urca Cooling of Neutron Stars

D. N. Voskresensky, V. A. Khodel, M. V. Zverev +1

It is proposed that a rearrangement of single-particle degrees of freedom may occur in a portion of the quantum fluid interior of a neutron star. Such a rearrangement is associated…