Search results

Records found: 3  
Your query: Author Sysno/Doc.kind = "^umb_un_auth 0205463 xpca^"
  1. TitleHybrid model with viscous relativistic hydrodynamics: a role of constraints on the shear-stress tensor
    Author infoA. S. Khvorostukhin ... [et al.]
    Author Khvorostukhin A. S. (34%)
    Co-authors Kolomeitsev Evgeni E. 1970- (33%) UMBFP06 - Katedra fyziky
    Toneev V. D. (33%)
    Source document The European Physical Journal A : Hadrons and Nuclei. Vol. 57, no. 10 (2021), pp. 294-1-294-25. - New York : Springer Nature, 2021
    Keywords relativistic hydrodynamics   heavy ion collisions   viscosity  
    Form. Descr.články - journal articles
    LanguageEnglish
    CountryGermany
    AnnotationWe present the hybrid model connecting the parton–hadron–string dynamic model (PHSD) and a hydrodynamic model taking into account shear viscosity within the Israel–Stewart approach. The numerical scheme, initialization, and particlization procedure are discussed in detail. The performance of the code is tested on the pion and proton rapidity and transverse mass distributions calculated for Au + Au and Pb+Pb collisions at AGS–SPS energies. The influence of the switch time from transport to hydro models, the viscous parameter, and freeze-out time are discussed. Since the applicability of the Israel–Stewart hydrodynamics assumes the perturbative character of the viscous stress tensor, πμν, which should not exceed the ideal energy–momentum tensor, T μν id , hydrodynamical codes usually rescale the shear stress tensor if the inequality πμν T μν id is not fulfilled in some sense. There are several conditions used in the literature and we analyze in detail the influence of different conditions and values of the cut-off parameter on observables.We show that the form of the corresponding condition plays an important role in the sensitivity of hydrodynamic calculations to the viscous parameter – a ratio of the shear viscosity to the entropy density, η/s. It is shown that the constraints used in the vHLLE and MUSIC models give the same results for the observables.With these constraints, the rapidity distributions and transverse momentum spectra are most sensitive to a change of the η/s ratio. We demonstrate that these constraints do not guarantee that each element of the πμν tensor is smaller than the corresponding element T μν id . As an alternative, a strict condition is used. When applied it reduces the sensitivity of the proton and pion momentum distributions to the viscosity parameter. We performed global fits of the rapidity and transverse mass distributions of pion and protons. It was also found that η/s as a function of the collision energy monotonically increases from Elab = 6 AGeV up to Elab = 40 AGeV and saturates for higher SPS energies. We observe that it is difficult to reproduce simultaneously pion and proton rapidity distribution within our model with the present choice of the equation of state without a phase transition.
    URLLink na plný text
    Public work category ADC
    No. of Archival Copy50708
    Catal.org.BB301 - Univerzitná knižnica Univerzity Mateja Bela v Banskej Bystrici
    Databasexpca - PUBLIKAČNÁ ČINNOSŤ
    ReferencesPERIODIKÁ-Súborný záznam periodika
  2. TitleMechanism of r-mode stability in young rapidly rotating pulsars
    Author infoE. E. Kolomeitsev, D. N. Voskresensky
    Author Kolomeitsev Evgeni E. 1970- (50%) UMBFP06 - Katedra fyziky
    Co-authors Voskresensky Dmitri (50%)
    Source document The European Physical Journal A : Hadrons and Nuclei. Vol. 50, no. 12 (2014), pp. [1-5]. - Berlin : Springer, 2014
    Keywords r-modes   viscosity   neutron stars   young pulsars  
    LanguageEnglish
    CountryGermany
    systematics 53
    AnnotationWe demonstrate that stability of r-modes in young rapidly rotating pulsars might be explained if one takes into account strong medium modifications of the nucleon-nucleon interaction because of the softening of pionic degrees of freedom in dense nucleon matter. Presence of the efficient direct Urca processes is not required. Within our model the most rapidly rotating observed young pulsar PSR J0537-6910 should have the mass > 1.8M_sol
    Public work category ADC
    No. of Archival Copy31379
    Catal.org.BB301 - Univerzitná knižnica Univerzity Mateja Bela v Banskej Bystrici
    Databasexpca - PUBLIKAČNÁ ČINNOSŤ
    ReferencesPERIODIKÁ-Súborný záznam periodika
    unrecognised

    unrecognised

  3. TitleThe hydrodynamic oscillator and its use in the investigation of chemical oscillators
    Par.titleHydrodynamický oscilátor a jeho využitie v štúdiu chemických oscilátorov
    Author infoĽubica Adamčíková, Zuzana Melichová
    Author Adamčíková Ľubica (50%)
    Co-authors Melichová Zuzana 1966- (50%) UMBFP08 - Katedra chémie
    Source document Collection of Czechoslovak Chemical Communications. Vol. 57, no. 8 (1992), pp. 1621-1628. - Prague : The Czech Academy of Sciences, 1992
    Keywords hydrodynamické oscilátory   hydrodynamic oscillators   oscilácie   kmitanie - oscillation   viskozita   viscosity  
    LanguageEnglish
    Country-CS
    systematics 54
    Public work category ADF
    No. of Archival Copy22425
    Repercussion categoryORLIK, Marek. Reakcje oscylacyjne : porządek i chaos. Warszawa : Wydawnictwa naukowo-techniczne, 1996. [343] s. ISBN 83-204-1970-0.
    KLEČKOVÁ, Marta - BLAŽKOVÁ, Radmila. Hydrodynamický oscilátor ve školním experimentu. In 50. sjezd chemických společností, Zlín, 8. - 11. záři 1997. Olomouc : Univerzita Palackého, 1997. ISBN 80-7067-745-7, s. 155.
    Catal.org.BB301 - Univerzitná knižnica Univerzity Mateja Bela v Banskej Bystrici
    Databasexpca - PUBLIKAČNÁ ČINNOSŤ
    ReferencesPERIODIKÁ-Súborný záznam periodika
    unrecognised

    unrecognised



  This site uses cookies to make them easier to browse. Learn more about how we use cookies.