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Your query: Author Sysno = "^umb_un_auth 0258764^"
  1. TitleOn cooling of neutron stars with a stiff equation of state including hyperons
    Author infoHovik Grigorian, Evgeni E. Kolomeitsev ... [et al.]
    Author Grigorian Hovik (25%)
    Co-authors Kolomeitsev Evgeni E. 1970- (25%) UMBFP06 - Katedra fyziky
    Maslov Konstantin A. (25%)
    Voskresensky Dmitri (25%)
    Source document Universe. Vol. 4, no. 2 (2018), pp. 1-6. - Basel : Multidisciplinary Digital Publishing Institute, 2018
    Keywords equation of state   neutron stars   neutrína - neutrinos  
    LanguageEnglish
    CountrySwitzerland
    systematics 53
    AnnotationExploiting a stiff equation of state of the relativistic mean-field model MKVORHf with sigma-scaled hadron effective masses and couplings, including hyperons, we demonstrate that the existing neutron-star cooling data can be appropriately described within “the nuclear medium cooling scenario” under the assumption that different sources have different masses
    URLLink na zdrojový dokument
    Public work category ADM
    No. of Archival Copy43911
    Catal.org.BB301 - Univerzitná knižnica Univerzity Mateja Bela v Banskej Bystrici
    Databasexpca - PUBLIKAČNÁ ČINNOSŤ
    ReferencesPERIODIKÁ-Súborný záznam periodika
    unrecognised

    unrecognised

  2. TitleCharged rho meson condensate in neutron stars within RMF models
    Author infoKonstantin A. Maslov, Evgeni E. Kolomeitsev, Dmitry N. Voskresensky
    Author Maslov Konstantin A. (34%)
    Co-authors Kolomeitsev Evgeni E. 1970- (33%) UMBFP06 - Katedra fyziky
    Voskresensky Dmitri (33%)
    Source document Universe. Vol. 4, no. 1 (2018), pp. 1-8. - Basel : Multidisciplinary Digital Publishing Institute, 2018 ; Compact stars in the QCD Phase Diagram medzinárodná konferencia
    Keywords neutron stars   equation of state   rho meson condensation   maximum mass   Delta resonances  
    LanguageEnglish
    CountrySwitzerland
    systematics 53
    AnnotationKnowledge of the equation of state (EoS) of cold and dense baryonic matter is essential for the description of properties of neutron stars (NSs). With an increase of the density, new baryon species can appear in NS matter, as well as various meson condensates. In previous works, we developed relativistic mean-field (RMF) models with hyperons and Δ -isobars, which passed the majority of known experimental constraints, including the existence of a 2 M ⊙ neutron star. In this contribution, we present results of the inclusion of ρ − -meson condensation into these models. We have shown that, in one class of the models (so-called KVOR-based models, in which the additional stiffening procedure is introduced in the isoscalar sector), the condensation gives only a small contribution to the EoS. In another class of the models (MKVOR-based models with additional stiffening in isovector sector), the condensation can lead to a first-order phase transition and a substantial decrease of the NS mass. Nevertheless, in all resulting models, the condensation does not spoil the description of the experimental constraints
    URLhttps://www.mdpi.com/2218-1997/4/1/1
    Public work category AFC
    No. of Archival Copy43907
    Catal.org.BB301 - Univerzitná knižnica Univerzity Mateja Bela v Banskej Bystrici
    Databasexpca - PUBLIKAČNÁ ČINNOSŤ
    ReferencesPERIODIKÁ-Súborný záznam periodika
    unrecognised

    unrecognised

  3. TitleThe effect of inclusion of delta resonances in relativistic mean-field model with scaled hadron masses and coupling constants
    Author infoK. A. Maslov, E. E. Kolomeitsev, D. N. Voskresensky
    Author Maslov Konstantin A. (1%)
    Co-authors Kolomeitsev Evgeni E. 1970- (98%) UMBFP06 - Katedra fyziky
    Voskresensky Dmitri (1%)
    Source document Journal of Physics: Conference Series. Vol. 798 (2017), pp. 1-5. - Bristol : IOP Publishing, 2017 ; International conference on particle physics and astrophysics ICPPA 2017 medzinárodná konferencia
    Keywords astrofyzika - astrophysics   neutron stars   relativita - relativity  
    LanguageEnglish
    CountryGreat Britian
    systematics 53
    Annotation© Published under licence by IOP Publishing Ltd.Knowledge of the equation of state of the baryon matter plays a decisive role in the description of neutron stars. With an increase of the baryon density the filling of Fermi seas of hyperons and Δ isobars becomes possible. Their inclusion into standard relativistic mean-field models results in a strong softening of the equation of state and a lowering of the maximum neutron star mass below the measured values. We extend a relativistic mean-field model with scaled hadron masses and coupling constants developed in our previous works and take into account now not only hyperons but also the Δ isobars. We analyze available empirical information to put constraints on coupling constants of Δs to mesonic mean fields. We show that the resulting equation of state satisfies majority of presently known experimental constraints.
    Public work category AFC
    No. of Archival Copy39068
    Catal.org.BB301 - Univerzitná knižnica Univerzity Mateja Bela v Banskej Bystrici
    Databasexpca - PUBLIKAČNÁ ČINNOSŤ
    ReferencesPERIODIKÁ-Súborný záznam periodika
    unrecognised

    unrecognised

  4. TitleDelta isobars in relativistic mean-field models with sigma-scaled hadron masses and couplings
    Author infoE. E. Kolomeitsev, K. A. Maslov, D. N. Voskresensky
    Author Kolomeitsev Evgeni E. 1970- (98%) UMBFP06 - Katedra fyziky
    Co-authors Maslov Konstantin A. (1%)
    Voskresensky Dmitri (1%)
    Source document Nuclear Physics A. Vol. 961 (2017), pp. 106-141. - Amsterdam : Elsevier B.V., 2017
    Keywords neutron stars   equation of state   heavy ion collisions  
    LanguageEnglish
    CountryNetherlands
    systematics 53
    AnnotationWe extend the relativistic mean-field models with hadron masses and meson-baryon coupling constants dependent on the scalar sigma field, studied previously to incorporate Delta(1232) baryons. Available empirical information is analyzed to put constraints on the couplings of Delta s with meson fields. Conditions for the appearance of Delta s are studied. We demonstrate that with inclusion of the Delta s our equations of state continue to fulfill majority of known empirical constraints including the pressure-density constraint from heavy-ion collisions, the constraint on the maximum mass of the neutron stars, the direct Urea and the gravitational baryon mass ratio constraints. (C) 2017 Elsevier B.V. All rights reserved.
    Public work category ADC
    No. of Archival Copy39909
    Catal.org.BB301 - Univerzitná knižnica Univerzity Mateja Bela v Banskej Bystrici
    Databasexpca - PUBLIKAČNÁ ČINNOSŤ
    ReferencesPERIODIKÁ-Súborný záznam periodika
    unrecognised

    unrecognised



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