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Volumn 66, Issue 5, 2002, Pages 549041-5490410

Comparison of space-time evolutions of hot, dense matter in √sNN=17 and 130 GeV relativistic heavy ion collisions based on a hydrodynamical model

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EID: 0036876513     PISSN: 05562813     EISSN: None     Source Type: Journal    
DOI: 10.1103/PhysRevC.66.054904     Document Type: Article
Times cited : (59)

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    • In this paper, we used a simpler hydrodynamical model than the present paper; we did not take account of baryon number nor particle productions through the resonances. The EoS is also different.
    • K. Morita, S. Muroya, H. Nakamura, and C. Nonaka, Phys. Rev. C 61, 034904 (2000). In this paper, we used a simpler hydrodynamical model than the present paper; we did not take account of baryon number nor particle productions through the resonances. The EoS is also different.
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* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.