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Based on a hydrodynamical model, we compare 130 GeV/$A$ Au+Au collisions atRHIC and 17 GeV/$A$ Pb+Pb collisions at SPS. The model well reproduces thesingle-particle distributions of both RHIC and SPS.  The numerical solution indicates that huge amount of collision energy in RHICis mainly used to produce a large extent of hot fluid rather than to make ahigh temperature matter; longitudinal extent of the hot fluid in RHIC is muchlarger than that of SPS and initial energy density of the fluid is only 5%higher than the one in SPS. The solution well describes the HBT radii at SPSenergy but shows some deviations from the ones at RHIC.Comment: 28 pages, 21 figures, REVTeX4, one figure is added and some figures  are replace

physical review. c. nuclear physics/physical review. c, nuclear physics

Comparison of space-time evolutions of hot, dense matter in<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msqrt><mml:mrow><mml:mrow><mml:msub><mml:mrow><mml:mi>s</mml:mi></mml:mrow><mml:mrow><mml:mi>NN</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:mrow></mml:msqrt></mml:mrow><mml:mrow><mml:mrow><mml:mrow /></mml:mrow></mml:mrow><mml:mo>=</mml:mo><mml:mn>17</mml:mn><mml:mn /></mml:math>and 130 GeV relativistic heavy ion collisions based on a …

Comparison of space-time evolutions of hot, dense matter insNN=17and 130 GeV relativistic heavy ion collisions based on a …