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Probing color superconducting phases and neutron superfluidity via hydrodynamic evolution at FAIR and NICA

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dc.contributor.author Das, Arpan
dc.date.accessioned 2025-11-28T10:17:53Z
dc.date.available 2025-11-28T10:17:53Z
dc.date.issued 2016
dc.identifier.uri https://inis.iaea.org/records/ss8kc-ze487
dc.identifier.uri http://dspace.bits-pilani.ac.in:8080/jspui/handle/123456789/20266
dc.description.abstract High baryon density regions of the cores of neutron stars are expected to have exotic phases such as color superconducting phases. The symmetry breaking pattern of these phases allows for topological vortices. Even in the lower density region of neutron star, neutron superfluid and associated topological vortices play important role in the dynamics of neutron star, e.g. in pulsar timings and glitches. We consider the possibility of formation of these superfluid phases in heavy-ion collision experiments, e.g. at FAIR and NICA, by carrying out Hydrodynamic simulation. Our result shows that existence of superfluid phases can be detected by studying the effect of vortices on power spectrum of flow fluctuations. ( en_US
dc.language.iso en en_US
dc.publisher India International Centre en_US
dc.subject Physics en_US
dc.subject Color superconductivity en_US
dc.subject Neutron superfluid vortices en_US
dc.subject Heavy-ion collisions en_US
dc.subject Flow fluctuation power spectrum en_US
dc.title Probing color superconducting phases and neutron superfluidity via hydrodynamic evolution at FAIR and NICA en_US
dc.type Article en_US


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