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  1. TitleCharged rho-meson condensation in neutron stars
    Author infoEvgeni E. Kolomeitsev, K. A. Maslov ... [et al.]
    Author Kolomeitsev Evgeni E. 1970- (34%) UMBFP06 - Katedra fyziky
    Co-authors Maslov K. A. (33%)
    Voskresensky Dmitri (33%)
    Source document Nuclear Physics A. Vol. 970, (2018), pp. 291-315. - Amsterdam : Elsevier B.V., 2018
    Keywords neutron stars   equation of state   condensation  
    LanguageEnglish
    CountryNetherlands
    systematics 53
    AnnotationWe extend relativistic mean-field models with hadron masses and meson–baryon coupling constants dependent on the scalar field σ, including hyperons and (1232)baryons, to incorporate a possibility of the charged ρmeson condensation in neutron star matter. The influence of the ρ−condensation on the equation of state proves to be strongly model dependent. In our models of one type (KVORcut-based ones) the ρ−condensation arises by a second-order phase transition above a critical density and the maximum value of the neutron star mass diminishes only slightly. The matter composition changes more significantly. In our models of other type (MKVOR*-based ones), if the system is considered at fixed density, the ρ−condensation arises by a second-order phase transition at the baryon density n =n(II)c,ρand at a slightly higher density n =n(I)c,ρthere occurs a first-order phase transition. In a neutron star matter starting with a density n <n(II)c,ρthere appears a region of a mixed phase, or the system is described by Maxwell construction, that results in a substantial decrease of the value of the maximum neutron star mass. Nevertheless in the models under consideration the observational constraint on the maximum neutron star mass is fulfilled. Besides, in MKVOR*-based models the appearance of the ρ−condensate is accompanied by a strong rearrangement of the matter composition. Dependence of the results on a choice of the ρmeson scaling functions for the effective ρmeson mass and coupling constants is also investigated
    URLLink na plný text
    Public work category ADC
    No. of Archival Copy43905
    Catal.org.BB301 - Univerzitná knižnica Univerzity Mateja Bela v Banskej Bystrici
    Databasexpca - PUBLIKAČNÁ ČINNOSŤ
    ReferencesPERIODIKÁ-Súborný záznam periodika
    unrecognised

    unrecognised

  2. TitleRelativistic mean-field models with scaled hadron masses and couplings
    Subtitlehyperons and maximum neutron star mass
    Author infoK. A. Maslov, E. E. Kolomeitsev, D. N. Voskresensky
    Author Maslov K. A. (1%)
    Co-authors Kolomeitsev Evgeni E. 1970- (98%) UMBFP06 - Katedra fyziky
    Voskresensky Dmitri (1%)
    Source document Nuclear Physics A. Vol. 950 (2016), pp. 64-109. - Amsterdam : Elsevier B.V., 2016
    Keywords stavová rovnica   equation of state   neutrónové hviezdy   neutron stars   fyzika - physics  
    LanguageEnglish
    CountryNetherlands
    systematics 53
    Public work category ADC
    No. of Archival Copy36997
    Catal.org.BB301 - Univerzitná knižnica Univerzity Mateja Bela v Banskej Bystrici
    Databasexpca - PUBLIKAČNÁ ČINNOSŤ
    ReferencesPERIODIKÁ-Súborný záznam periodika
    unrecognised

    unrecognised

  3. TitleHyperon puzzle and the RMF model with scaled hadron masses and coupling constants
    Author infoE. E. Kolomeitsev, K. A. Maslov, D. N. Voskresensky
    Author Kolomeitsev Evgeni E. 1970- (96%) UMBFP06 - Katedra fyziky
    Co-authors Maslov K. A. (2%)
    Voskresensky Dmitri (2%)
    Source document Journal of Physics: Conference Series. Vol. 668 (2016), pp. 1-6. - Bristol : IOP Publishing, 2016 ; SQM 2015 medzinárodná konferencia
    Keywords stavová rovnica   relativistický model stredného poľa   neutrónové hviezdy   equation of state   relativistic mean-field models   neutron stars  
    LanguageEnglish
    CountryGreat Britian
    systematics 533
    AnnotationThe 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 demonstrate that if the effective nucleon mass stops to decrease with a density increase at densities n > n > n0, where n0 is the nuclear saturation density, the equation of state stiffens for these densities and the limiting neutron star mass increases. The stabilization of the nucleon mass can be realised if in the equation of motion for the scalar mean-field there appear a term sharply varying in a narrow vicinity of the field value corresponding to the density n . We show several possible realizations of this mechanism getting sufficiently stiff equations of state. The appearance of hyperons in dense neutron star interiors is accounted for. The obtained equations of state remain sufficiently stiff if the reduction of the ϕ meson mass is incorporated. Thereby, the hyperon puzzle can be resolved
    Public work category AFC
    No. of Archival Copy35029
    Catal.org.BB301 - Univerzitná knižnica Univerzity Mateja Bela v Banskej Bystrici
    Databasexpca - PUBLIKAČNÁ ČINNOSŤ
    ReferencesPERIODIKÁ-Súborný záznam periodika
    unrecognised

    unrecognised

  4. TitleMaking a soft relativistic mean-field equation of state stiffer at high density
    Author infoK. A. Maslov, E. E. Kolomeitsev, D. N. Voskresensky
    Author Maslov K. A. (25%)
    Co-authors Kolomeitsev Evgeni E. 1970- (50%) UMBFP06 - Katedra fyziky
    Voskresensky Dmitri (25%)
    Source document Physical Review C : Nuclear Physics. Vol. 92, no. 5 (2015), pp. [1-5]. - Maryland : American Physical Society, 2015
    Keywords neutrónové hviezdy   stavová rovnica   relativistický model stredného poľa   neutron stars   equation of state   relativistic mean-field models  
    LanguageEnglish
    CountryUnited States of America
    systematics 531
    Public work category ADC
    No. of Archival Copy34334
    Catal.org.BB301 - Univerzitná knižnica Univerzity Mateja Bela v Banskej Bystrici
    Databasexpca - PUBLIKAČNÁ ČINNOSŤ
    ReferencesPERIODIKÁ-Súborný záznam periodika
    unrecognised

    unrecognised

  5. TitleSolution of the hyperon puzzle within a relativistic mean-field model
    Author infoK. A. Maslov, Evgeni E. Kolomeitsev, D. N. Voskresensky
    Author Maslov K. A. (34%)
    Co-authors Kolomeitsev Evgeni E. 1970- (33%) UMBFP06 - Katedra fyziky
    Voskresensky Dmitri (33%)
    Source document Physics Letters B. Vol. 748 (2015), pp. 369-375. - Amsterdam : Elsevier B.V., 2015
    Keywords neutrónové hviezdy   neutron stars   relativistic mean-field models   hyperons  
    LanguageEnglish
    CountryNetherlands
    Public work category ADC
    No. of Archival Copy33613
    Catal.org.BB301 - Univerzitná knižnica Univerzity Mateja Bela v Banskej Bystrici
    Databasexpca - PUBLIKAČNÁ ČINNOSŤ
    ReferencesPERIODIKÁ-Súborný záznam periodika
    unrecognised

    unrecognised



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