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Enhancement of Low-Mass Dileptons in Heavy Ion Collisions
Open accessAbstract
Using a relativistic transport model for the expansion stage of S + Au collisions at 200 GeV/nucleon, we show that the recently observed enhancement of low-mass dileptons by the CERES Collaboration can be explained by the decrease of vector meson masses in hot and dense hadronic matter.
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Citations
Cited by
Dyson-Schwinger Equations: Density, Temperature and Continuum Strong QCD
Roberts, C. (2000) · Progress in Particle and Nuclear Physics · doi:10.1016/s0146-6410(00)00106-x · Cited by 632
Rho meson propagation and dilepton enhancement in hot hadronic matter
Rapp, R., Chanfray, G., & Wambach, J. (1997) · Nuclear Physics A · doi:10.1016/s0375-9474(97)00137-1 · Cited by 305
Signatures of quark-gluon plasma formation in high energy heavy-ion collisions: a critical review
Bass, S. A., Gyulassy, M., Stöcker, H., & Greiner, W. (1999) · Journal of Physics G: Nuclear and Particle Physics · doi:10.1088/0954-3899/25/3/013 · Cited by 269
Metadata
- Authors
- Li, G. Q., Ko, C. M., & Brown, G. E.
- Venue
- Physical Review Letters
- Publisher
- American Physical Society (APS)
- Published
- 1995-11-27
- Volume
- 75
- Issue
- 22
- Pages
- 4007-4010
- ISSN
- 0031-9007 (ISSN-L)
- 1079-7114
- OpenAlex
- W2088208700
- Cited by
- 291
- References
- 0
- FWCI
- 32.54
- Type
- journal article
- Language
- en
- Open access
- green
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- CoChat. (2026). Citation check: Enhancement of Low-Mass Dileptons in Heavy Ion Collisions. https://app.cochat.ai/papers/10.1103/physrevlett.75.4007
- The paper
- Li, G. Q., Ko, C. M., & Brown, G. E. (1995). Enhancement of Low-Mass Dileptons in Heavy Ion Collisions. Physical Review Letters. https://doi.org/10.1103/physrevlett.75.4007
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Bibliographic data: Semantic Scholar, OpenAlex, Crossref.
Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.
