Dense nuclear matter equation of state from heavy-ion collisions

Result code in IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F61389005%3A_____%2F24%3A00581780" target="_blank" >RIV/61389005:_____/24:00581780 - isvavai.cz</a>

Alternative codes found

RIV/68407700:21340/24:00371384

Result on the web

<a href="https://doi.org/10.1016/j.ppnp.2023.104080" target="_blank" >https://doi.org/10.1016/j.ppnp.2023.104080</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.1016/j.ppnp.2023.104080" target="_blank" >10.1016/j.ppnp.2023.104080</a>

Result language

angličtina

Original language name

Dense nuclear matter equation of state from heavy-ion collisions

Original language description

The nuclear equation of state (EOS) is at the center of numerous theoretical and experimental efforts in nuclear physics. With advances in microscopic theories for nuclear interactions, the availability of experiments probing nuclear matter under conditions not reached before, endeav-ors to develop sophisticated and reliable transport simulations to interpret these experiments, and the advent of multi-messenger astronomy, the next decade will bring new opportunities for determining the nuclear matter EOS, elucidating its dependence on density, temperature, and isospin asymmetry. Among controlled terrestrial experiments, collisions of heavy nuclei at inter -mediate beam energies (from a few tens of MeV/nucleon to about 25 GeV/nucleon in the fixed-target frame) probe the widest ranges of baryon density and temperature, enabling studies of nuclear matter from a few tenths to about 5 times the nuclear saturation density and for temper-atures from a few to well above a hundred MeV, respectively. Collisions of neutron-rich isotopes further bring the opportunity to probe effects due to the isospin asymmetry. However, capitaliz-ing on the enormous scientific effort aimed at uncovering the dense nuclear matter EOS, both at RHIC and at FRIB as well as at other international facilities, depends on the continued develop-ment of state-of-the-art hadronic transport simulations. This white paper highlights the essential role that heavy-ion collision experiments and hadronic transport simulations play in understand -ing strong interactions in dense nuclear matter, with an emphasis on how these efforts can be used together with microscopic approaches and neutron star studies to uncover the nuclear EOS.

Czech name

—

Czech description

—

Type

J_imp - Article in a specialist periodical, which is included in the Web of Science database

CEP classification

—

OECD FORD branch

10303 - Particles and field physics

Project

<a href="/en/project/GA22-25026S" target="_blank" >GA22-25026S: Matter in extreme conditions and relativistic heavy-ion collisions</a><br>

Continuities

I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year

2024

Confidentiality

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

Name of the periodical

Progress in Particle and Nuclear Physics

ISSN

0146-6410

e-ISSN

1873-2224

Volume of the periodical

134

Issue of the periodical within the volume

JAN

Country of publishing house

NL - THE KINGDOM OF THE NETHERLANDS

Number of pages

62

Pages from-to

104080

UT code for WoS article

001134736900001

EID of the result in the Scopus database

2-s2.0-85176272683