Published February 23, 2024 | Version v1
Journal article Open

Observation of the Electromagnetic Field Effect via Charge-Dependent Directed Flow in Heavy-Ion Collisions at the Relativistic Heavy Ion Collider

  • 1. American University in Cairo, New Cairo 11835, Egypt
  • 2. Texas A&M University, College Station, Texas 77843
  • 3. Czech Technical University in Prague, FNSPE, Prague 115 19, Czech Republic
  • 4. The Ohio State University, Columbus, Ohio 43210
  • 5. Joint Institute for Nuclear Research, Dubna 141 980
  • 6. Panjab University, Chandigarh 160014, India
  • 7. Variable Energy Cyclotron Centre, Kolkata 700064, India
  • 8. Alikhanov Institute for Theoretical and Experimental Physics NRC "Kurchatov Institute," Moscow 117218
  • 9. National Research Nuclear University MEPhI, Moscow 115409

Description

The deconfined quark-gluon plasma (QGP) created in relativistic heavy-ion collisions enables the exploration of the fundamental properties of matter under extreme conditions. Noncentral collisions can produce strong magnetic fields on the order of 1018G, which offers a probe into the electrical conductivity of the QGP. In particular, quarks and antiquarks carry opposite charges and receive contrary electromagnetic forces that alter their momenta. This phenomenon can be manifested in the collective motion of final-state particles, specifically in the rapidity-odd directed flow, denoted as v1(y). Here, we present the charge-dependent measurements of dv1/dy near midrapidities for π±, K±, and p(p¯) in Au+Au and isobar (Ru4496+Ru4496 and Zr4096+Zr4096) collisions at sNN=200GeV, and in Au+Au collisions at 27 GeV, recorded by the STAR detector at the Relativistic Heavy Ion Collider. The combined dependence of the v1 signal on collision system, particle species, and collision centrality can be qualitatively and semiquantitatively understood as several effects on constituent quarks. While the results in central events can be explained by the u and d quarks transported from initial-state nuclei, those in peripheral events reveal the impacts of the electromagnetic field on the QGP. Our data put valuable constraints on the electrical conductivity of the QGP in theoretical calculations.

Files

10.1103_PhysRevX.14.011028.pdf

Files (1.6 MB)

Name Size Download all
md5:d2f9806c31867c31f3cb7ff9600f0de5
1.6 MB Preview Download

Additional details

Identifiers

DOI
10.1103/PhysRevX.14.011028;
arXiv
arXiv:2304.03430;
Crossref Funder ID
10.13039/100001416; 10.13039/100006231; 10.13039/100017223; 10.13039/100006235; 10.13039/100006209; 10.13039/100006132; 10.13039/100000001; 10.13039/501100001809; 10.13039/501100002367; 10.13039/501100018537; 10.13039/501100007750; 10.13039/501100003725; 10.13039/501100001824; 10.13039/501100001823; 10.13039/501100018818; 10.13039/501100005881; 10.13039/501100001502; 10.13039/501100004281; 10.13039/100015526; 10.13039/501100010571; 10.13039/501100001656; 10.13039/501100001700; 10.13039/501100001691; 10.13039/501100020884;

Publishing Information

Journal Title
Physical Review X
Journal Volume
14
Journal Issue
1
Journal Page Range
12 pgs.
ISSN
2160-3308