The Experts below are selected from a list of 270 Experts worldwide ranked by ideXlab platform
Dimitrios Psaltis - One of the best experts on this subject based on the ideXlab platform.
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model independent inference of neutron star radii from Moment of Inertia measurements
Physical Review C, 2016Co-Authors: Carolyn A Raithel, Feryal Ozel, Dimitrios PsaltisAbstract:A precise Moment of Inertia measurement for PSR J0737-3039A in the double pulsar system is expected within the next five years. We present here a new method of mapping the anticipated measurement of the Moment of Inertia directly into the neutron star structure. We determine the maximum and minimum values possible for the Moment of Inertia of a neutron star of a given radius based on physical stability arguments, assuming knowledge of the equation of state only at densities below the nuclear saturation density. If the equation of state is trusted up to the nuclear saturation density, we find that a measurement of the Moment of Inertia will place absolute bounds on the radius of PSR J0737-3039A to within $\ifmmode\pm\else\textpm\fi{}1$ km. The resulting combination of Moment of Inertia, mass, and radius measurements for a single source will allow for new, stringent constraints on the dense-matter equation of state.
X. Viñas - One of the best experts on this subject based on the ideXlab platform.
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Moment of Inertia of a trapped superfluid gas of Fermions
arXiv: Superconductivity, 2000Co-Authors: M. Farine, Peter Schuck, X. ViñasAbstract:The Moment of Inertia Q of a trapped superfluid gas of atomic Fermions (6Li) is calculated as a function of the temperature. At zero temperature the Moment of Inertia takes on the irrotational flow value. Only for T very close to Tc rigid rotation is attained. It is proposed that future measurements of the rotational energy will unambiguously reveal whether the system is in a superfluid state or not.
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Moment of Inertia of a trapped superfluid gas of atomic fermions
Physical Review A, 2000Co-Authors: M. Farine, Peter Schuck, X. ViñasAbstract:The Moment of Inertia of a trapped superfluid gas of atomic fermions (6Li) is calculated as a function of the temperature. At zero temperature the Moment of Inertia takes on the irrotational flow value. Only for T very close to Tc is rigid rotation attained. It is proposed that future measurements of the rotational energy will unambiguously reveal whether the system is in a superfluid state or not.
Carolyn A Raithel - One of the best experts on this subject based on the ideXlab platform.
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model independent inference of neutron star radii from Moment of Inertia measurements
Physical Review C, 2016Co-Authors: Carolyn A Raithel, Feryal Ozel, Dimitrios PsaltisAbstract:A precise Moment of Inertia measurement for PSR J0737-3039A in the double pulsar system is expected within the next five years. We present here a new method of mapping the anticipated measurement of the Moment of Inertia directly into the neutron star structure. We determine the maximum and minimum values possible for the Moment of Inertia of a neutron star of a given radius based on physical stability arguments, assuming knowledge of the equation of state only at densities below the nuclear saturation density. If the equation of state is trusted up to the nuclear saturation density, we find that a measurement of the Moment of Inertia will place absolute bounds on the radius of PSR J0737-3039A to within $\ifmmode\pm\else\textpm\fi{}1$ km. The resulting combination of Moment of Inertia, mass, and radius measurements for a single source will allow for new, stringent constraints on the dense-matter equation of state.
M. Farine - One of the best experts on this subject based on the ideXlab platform.
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Moment of Inertia of a trapped superfluid gas of Fermions
arXiv: Superconductivity, 2000Co-Authors: M. Farine, Peter Schuck, X. ViñasAbstract:The Moment of Inertia Q of a trapped superfluid gas of atomic Fermions (6Li) is calculated as a function of the temperature. At zero temperature the Moment of Inertia takes on the irrotational flow value. Only for T very close to Tc rigid rotation is attained. It is proposed that future measurements of the rotational energy will unambiguously reveal whether the system is in a superfluid state or not.
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Moment of Inertia of a trapped superfluid gas of atomic fermions
Physical Review A, 2000Co-Authors: M. Farine, Peter Schuck, X. ViñasAbstract:The Moment of Inertia of a trapped superfluid gas of atomic fermions (6Li) is calculated as a function of the temperature. At zero temperature the Moment of Inertia takes on the irrotational flow value. Only for T very close to Tc is rigid rotation attained. It is proposed that future measurements of the rotational energy will unambiguously reveal whether the system is in a superfluid state or not.
Feryal Ozel - One of the best experts on this subject based on the ideXlab platform.
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model independent inference of neutron star radii from Moment of Inertia measurements
Physical Review C, 2016Co-Authors: Carolyn A Raithel, Feryal Ozel, Dimitrios PsaltisAbstract:A precise Moment of Inertia measurement for PSR J0737-3039A in the double pulsar system is expected within the next five years. We present here a new method of mapping the anticipated measurement of the Moment of Inertia directly into the neutron star structure. We determine the maximum and minimum values possible for the Moment of Inertia of a neutron star of a given radius based on physical stability arguments, assuming knowledge of the equation of state only at densities below the nuclear saturation density. If the equation of state is trusted up to the nuclear saturation density, we find that a measurement of the Moment of Inertia will place absolute bounds on the radius of PSR J0737-3039A to within $\ifmmode\pm\else\textpm\fi{}1$ km. The resulting combination of Moment of Inertia, mass, and radius measurements for a single source will allow for new, stringent constraints on the dense-matter equation of state.
