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Properties of QCD matter at high baryon density

紀錄類型:	書目-電子資源 : Monograph/item
正題名/作者:	Properties of QCD matter at high baryon densityedited by Xiaofeng Luo ... [et al.].
其他作者:	Luo, Xiaofeng.
出版者:	Singapore :Springer Nature Singapore :2022.
面頁冊數:	xi, 287 p. :ill., digital ;24 cm.
Contained By:	Springer Nature eBook
標題:	Quantum chromodynamics.
電子資源:	https://doi.org/10.1007/978-981-19-4441-3
ISBN:	9789811944413$q(electronic bk.)

Properties of QCD matter at high baryon density
Properties of QCD matter at high baryon density[electronic resource] /edited by Xiaofeng Luo ... [et al.]. - Singapore :Springer Nature Singapore :2022. - xi, 287 p. :ill., digital ;24 cm.

Introduction -- QCD phase structure at finite baryon density -- Nuclear matter under extreme external fields : rotation and magnetic fields -- Dynamical evolution of non-equilibrium and transport -- Nuclear matter at high density and EOS -- Summary and outlook.

This book highlights the discussions by renown researchers on questions emerged during transition from the relativistic heavy-ion collider (RHIC) to the future electron ion collider (EIC) Over the past two decades, the RHIC has provided a vast amount of data over a wide range of the center of mass energies. What are the scientific priorities, after RHIC is shut down and turned to the future EIC? What should be the future focuses of the high-energy nuclear collisions? What are thermodynamic properties of quantum chromodynamics (QCD) at large baryon density? Where is the phase boundary between quark-gluon-plasma and hadronic matter at high baryon density? How does one make connections from thermodynamics learned in high-energy nuclear collisions to astrophysical topics, to name few, the inner structure of compact stars, and perhaps more interestingly, the dynamical processes of the merging of neutron stars? While most particle physicists are interested in Dark Matter, we should focus on the issues of Visible Matter! Multiple heavy-ion accelerator complexes are under construction: NICA at JINR (4 ~ 11 GeV), FAIR at GSI (2 ~ 4.9 GeV SIS100), HIAF at IMP (2 ~ 4 GeV) In addition, the heavy-ion collision has been actively discussed at the J-PARC. The book is a collective work of top researchers from the field where some of the above-mentioned basic questions will be addressed. We believe that answering those questions will certainly advance our understanding of the phase transition in early universe as well as its evolution that leads to today's world of nature.

ISBN: 9789811944413$q(electronic bk.)

Standard No.: 10.1007/978-981-19-4441-3doiSubjects--Topical Terms:

228107
Quantum chromodynamics.

LC Class. No.: QC793.3.Q35

Dewey Class. No.: 539.7548

Properties of QCD matter at high baryon density
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520 $a This book highlights the discussions by renown researchers on questions emerged during transition from the relativistic heavy-ion collider (RHIC) to the future electron ion collider (EIC) Over the past two decades, the RHIC has provided a vast amount of data over a wide range of the center of mass energies. What are the scientific priorities, after RHIC is shut down and turned to the future EIC? What should be the future focuses of the high-energy nuclear collisions? What are thermodynamic properties of quantum chromodynamics (QCD) at large baryon density? Where is the phase boundary between quark-gluon-plasma and hadronic matter at high baryon density? How does one make connections from thermodynamics learned in high-energy nuclear collisions to astrophysical topics, to name few, the inner structure of compact stars, and perhaps more interestingly, the dynamical processes of the merging of neutron stars? While most particle physicists are interested in Dark Matter, we should focus on the issues of Visible Matter! Multiple heavy-ion accelerator complexes are under construction: NICA at JINR (4 ~ 11 GeV), FAIR at GSI (2 ~ 4.9 GeV SIS100), HIAF at IMP (2 ~ 4 GeV) In addition, the heavy-ion collision has been actively discussed at the J-PARC. The book is a collective work of top researchers from the field where some of the above-mentioned basic questions will be addressed. We believe that answering those questions will certainly advance our understanding of the phase transition in early universe as well as its evolution that leads to today's world of nature.
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