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Using CMBR analysis tools for flow anisotropies in relativistic heavy-ion collisions |
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Content: |
Recently we have shown that there are crucial similarities in the physics of cosmic microwave background radiation (CMBR) anisotropies and the flow anisotropies in relativistic heavy-ion collision experiments (RHICE). Here we demonstrate how following the analysis techniques used in CMBR can give important information about the initial state and evolution of the plasma formed in heavy ion collisions. |
Id: |
133 |
Place: |
Room: Main Auditorium |
Starting date: |
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Duration: |
00' |
Primary Authors: |
Ms. PANDIAT, Saumia (Institute of Physics, Bubaneswar) |
Co-Authors: |
Mr. MISHRA, Ananta (Institute of Mathematical Sciences, Chennai) Mrs. MOHAPATRA, Ranjita (Institute of Physics, Bhubaneswar) Prof. SRIVASTAVA, Ajit (Institute of Physics, Bhubaneswar) |
Presenters: |
Ms. PANDIAT, Saumia |
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