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Description
  • Stavové rovnice relativistické asymetrické jaderné hmoty (EoS) lze získat z předpokládaného tvaru interakčního lagrangianu. Tvoří jeden z důležitých vstupů pro popis neutronových hvězd. Struktura neutronových hvězd, tj. hustota hmoty a tlak jako funkce radiální vzdálenosti, počínaje z jejich hodnot ve středu hvězdy, přímo závisí na EoS. Podobně lze odtud získat limitu na celkovou hmotnost neutronové hvězdy. EoS a ji determinující nukleonové interakce tedy mohou být testovány pomocí astronomických observací. (cs)
  • The equations of state (EoS) of relativistic asymmetric nuclear matter are obtainable from assumed form of the interaction Lagrangian. They are one of important inputs to describe the neutron stars. The structure of the neutron stars, i.e. the density of matter and the pressure as functions of radial distance starting from their values at the center of a star, is straightforwardly dependent on EoS. Similarly, a limitation on the total mass of the neutron star can be obtained therefrom. Thus, EoS and the underlying nucleon interactions can be tested also by the means of astronomical observations.
  • The equations of state (EoS) of relativistic asymmetric nuclear matter are obtainable from assumed form of the interaction Lagrangian. They are one of important inputs to describe the neutron stars. The structure of the neutron stars, i.e. the density of matter and the pressure as functions of radial distance starting from their values at the center of a star, is straightforwardly dependent on EoS. Similarly, a limitation on the total mass of the neutron star can be obtained therefrom. Thus, EoS and the underlying nucleon interactions can be tested also by the means of astronomical observations. (en)
Title
  • Nuclear matter equations of state and the neutron stars
  • Stavové rovnice jaderné hmoty a neutronové hvězdy (cs)
  • Nuclear matter equations of state and the neutron stars (en)
skos:prefLabel
  • Nuclear matter equations of state and the neutron stars
  • Stavové rovnice jaderné hmoty a neutronové hvězdy (cs)
  • Nuclear matter equations of state and the neutron stars (en)
skos:notation
  • RIV/47813059:19240/08:#0001929!RIV09-MSM-19240___
http://linked.open...avai/riv/aktivita
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  • P(LC06014), Z(MSM4781305903)
http://linked.open...vai/riv/dodaniDat
http://linked.open...aciTvurceVysledku
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  • 383400
http://linked.open...ai/riv/idVysledku
  • RIV/47813059:19240/08:#0001929
http://linked.open...riv/jazykVysledku
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  • asymmetric nuclear matter, neutron stars, quantum hadrodynamics, relativistic Brueckner-Haitree-Fock, equations of state (en)
http://linked.open.../riv/klicoveSlovo
http://linked.open...ontrolniKodProRIV
  • [B22FFF6DE67E]
http://linked.open...v/mistoKonaniAkce
  • Crete, GREECE
http://linked.open...i/riv/mistoVydani
  • GREECE
http://linked.open...i/riv/nazevZdroje
  • FRONTIERS IN NUCLEAR STRUCTURE, ASTROPHYSICS, AND REACTIONS - FINUSTAR 2
http://linked.open...in/vavai/riv/obor
http://linked.open...ichTvurcuVysledku
http://linked.open...cetTvurcuVysledku
http://linked.open...vavai/riv/projekt
http://linked.open...UplatneniVysledku
http://linked.open...iv/tvurceVysledku
  • Běták, Emil
  • Stuchlík, Zdeněk
  • Urbanec, Martin
http://linked.open...vavai/riv/typAkce
http://linked.open...ain/vavai/riv/wos
  • 000256223700054
http://linked.open.../riv/zahajeniAkce
http://linked.open...n/vavai/riv/zamer
issn
  • 0094-243X
number of pages
http://purl.org/ne...btex#hasPublisher
  • NCSR; Univ Jyvaskyla; Natl Tech Univ Athens; Greek Minist Educ
https://schema.org/isbn
  • 978-0-7354-0532-5
http://localhost/t...ganizacniJednotka
  • 19240
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