Shedding Light to the Dark Sides of the Universe: Cosmology from Strong Interactions

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F61389005%3A_____%2F22%3A00563494" target="_blank" >RIV/61389005:_____/22:00563494 - isvavai.cz</a>

Výsledek na webu

<a href="https://doi.org/10.3390/universe8100545" target="_blank" >https://doi.org/10.3390/universe8100545</a>

DOI - Digital Object Identifier

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Jazyk výsledku

angličtina

Název v původním jazyce

Shedding Light to the Dark Sides of the Universe: Cosmology from Strong Interactions

Popis výsledku v původním jazyce

The basic aim of this Special Issue was to reflect upon the modern status of research on strong interactions and their implications in Cosmology. In addtion to a few important original research articles, our Special Issue comprises a collection of reviews on existing implications of the physics of strongly coupled and non-perturbative phenomena such as those in Quantum Chromodynamics (QCD) to the universe evolution in different epochs. Such implications concern, in particular, cosmological aspects of quark–gluon plasma and phase transition dynamics, the physics of neutron stars, QCD equations of state (EoS), as well as the origins of Dark Matter (DM) and Dark Energy (DE) from both dark sectors and QCD, inflationary cosmology, etc.

Název v anglickém jazyce

Shedding Light to the Dark Sides of the Universe: Cosmology from Strong Interactions

Popis výsledku anglicky

The basic aim of this Special Issue was to reflect upon the modern status of research on strong interactions and their implications in Cosmology. In addtion to a few important original research articles, our Special Issue comprises a collection of reviews on existing implications of the physics of strongly coupled and non-perturbative phenomena such as those in Quantum Chromodynamics (QCD) to the universe evolution in different epochs. Such implications concern, in particular, cosmological aspects of quark–gluon plasma and phase transition dynamics, the physics of neutron stars, QCD equations of state (EoS), as well as the origins of Dark Matter (DM) and Dark Energy (DE) from both dark sectors and QCD, inflationary cosmology, etc.

Druh

O - Ostatní výsledky

CEP obor

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OECD FORD obor

10308 - Astronomy (including astrophysics,space science)

Projekt

Výsledek vznikl pri realizaci vícero projektů. Více informací v záložce Projekty.

Návaznosti

I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Rok uplatnění

2022

Kód důvěrnosti údajů

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů