TY - JOUR
T1 - Theoretical and experimental constraints for the equation of state of dense and hot matter
AU - Kumar, Rajesh
AU - Dexheimer, Veronica
AU - Jahan, Johannes
AU - Noronha, Jorge
AU - Noronha-Hostler, Jacquelyn
AU - Ratti, Claudia
AU - Yunes, Nico
AU - Nava Acuna, Angel Rodrigo
AU - Alford, Mark
AU - Anik, Mahmudul Hasan
AU - Chatterjee, Debarati
AU - Chatziioannou, Katerina
AU - Chen, Hsin Yu
AU - Clevinger, Alexander
AU - Conde, Carlos
AU - Cruz-Camacho, Nikolas
AU - Dore, Travis
AU - Drischler, Christian
AU - Elfner, Hannah
AU - Essick, Reed
AU - Friedenberg, David
AU - Ghosh, Suprovo
AU - Grefa, Joaquin
AU - Haas, Roland
AU - Haber, Alexander
AU - Hammelmann, Jan
AU - Harris, Steven
AU - Haster, Carl Johan
AU - Hatsuda, Tetsuo
AU - Hippert, Mauricio
AU - Hirayama, Renan
AU - Holt, Jeremy W.
AU - Kahangirwe, Micheal
AU - Karthein, Jamie
AU - Kojo, Toru
AU - Landry, Philippe
AU - Lin, Zidu
AU - Luzum, Matthew
AU - Manning, Timothy Andrew
AU - Salinas San Martin, Jordi
AU - Miller, Cole
AU - Most, Elias Roland
AU - Mroczek, Debora
AU - Muronga, Azwinndini
AU - Patino, Nicolas
AU - Peterson, Jeffrey
AU - Plumberg, Christopher
AU - Price, Damien
AU - Providencia, Constanca
AU - Rougemont, Romulo
AU - Roy, Satyajit
AU - Shah, Hitansh
AU - Shapiro, Stuart
AU - Steiner, Andrew W.
AU - Strickland, Michael
AU - Tan, Hung
AU - Togashi, Hajime
AU - Portillo Vazquez, Israel
AU - Wen, Pengsheng
AU - Zhang, Ziyuan
N1 - The authors would like to thank Niseem Abdelrahman, Wei Li, Tetyana Galatyuk, and You Zhou for providing comments and assistance in finding the experimental references in this work. The MUSES collaboration is supported by NSF under OAC-2103680. Additional support for the collaboration members includes: DM is supported NSF Graduate Research Fellowship Program under Grant No. DGE - 1746047. JSSM is supported by Consejo Nacional de Ciencia y Tecnologia (CONACYT) under SNI Fellowship I1200/16/2020. CR is supported by NSF under Grants No. PHY-1654219, PHY-2208724, PHY-2116686. MGA is partly supported by DOE, Office of Science, Office of Nuclear Physics under Award No. DE-FG02-05ER41375. VD is supported by NSF under Grants PHY1748621 and NP3M PHY-2116686. MS is supported by DOE, Office of Science No DE-SC0013470. MCM is supported in part by NASA ADAP Grant 80NSSC21K0649. ML thanks the S\u00E3o Paulo Research Foundation (FAPESP) for support under Grants 2021/08465-9, 2018/24720-6, and 2017/05685-2, as well as the support of the Brazilian National Council for Scientific and Technological Development (CNPq). ERM acknowledges support as the John Archibald Wheeler Fellow at Princeton University (PCTS), and from the Institute for Advanced Study. SPH is supported by DOE Grant DE-FG02-00ER41132. PL is supported by the Natural Sciences & Engineering Research Council of Canada (NSERC). CP is supported by FCT (Funda\u00E7\u00E3o para a Ci\u00EAncia e a Tecnologia, I.P, Portugal) under Projects No. UIDP/-04564/-2020, No. UIDB/-04564/-2020 and 2022.06460.PTDC. SLS is supported by NSF Grant PHY-2006066 and NASA Grant 80NSSC17K0070, both to UIUC.
PY - 2024/12
Y1 - 2024/12
N2 - This review aims at providing an extensive discussion of modern constraints relevant for dense and hot strongly interacting matter. It includes theoretical first-principle results from lattice and perturbative QCD, as well as chiral effective field theory results. From the experimental side, it includes heavy-ion collision and low-energy nuclear physics results, as well as observations from neutron stars and their mergers. The validity of different constraints, concerning specific conditions and ranges of applicability, is also provided.
AB - This review aims at providing an extensive discussion of modern constraints relevant for dense and hot strongly interacting matter. It includes theoretical first-principle results from lattice and perturbative QCD, as well as chiral effective field theory results. From the experimental side, it includes heavy-ion collision and low-energy nuclear physics results, as well as observations from neutron stars and their mergers. The validity of different constraints, concerning specific conditions and ranges of applicability, is also provided.
KW - Dense matter
KW - Heavy-ion collisions
KW - Multi-messenger physics
KW - Neutron star
UR - http://www.scopus.com/inward/record.url?scp=85195465919&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=85195465919&partnerID=8YFLogxK
U2 - 10.1007/s41114-024-00049-6
DO - 10.1007/s41114-024-00049-6
M3 - Review article
AN - SCOPUS:85195465919
SN - 2367-3613
VL - 27
JO - Living Reviews in Relativity
JF - Living Reviews in Relativity
IS - 1
M1 - 3
ER -