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Please use this identifier to cite or link to this item: http://dspace.bits-pilani.ac.in:8080/jspui/handle/123456789/20266
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dc.contributor.authorDas, Arpan-
dc.date.accessioned2025-11-28T10:17:53Z-
dc.date.available2025-11-28T10:17:53Z-
dc.date.issued2016-
dc.identifier.urihttps://inis.iaea.org/records/ss8kc-ze487-
dc.identifier.urihttp://dspace.bits-pilani.ac.in:8080/jspui/handle/123456789/20266-
dc.description.abstractHigh 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.isoenen_US
dc.publisherIndia International Centreen_US
dc.subjectPhysicsen_US
dc.subjectColor superconductivityen_US
dc.subjectNeutron superfluid vorticesen_US
dc.subjectHeavy-ion collisionsen_US
dc.subjectFlow fluctuation power spectrumen_US
dc.titleProbing color superconducting phases and neutron superfluidity via hydrodynamic evolution at FAIR and NICAen_US
dc.typeArticleen_US
Appears in Collections:Department of Physics

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