- Abstract:
-
Many neutron star features can be accurately modeled only if one assumes that a significant portion of the neutron star interior is in a superfluid state and if relativitic effects are considered, and possible solutions to the underlying mathematical models include vortex solutions. It was recently shown that vorticity in relativistic superfluids can be studied under the framework of a nonlinear Klein-Gordon (NLKG) model in general curvilinear coordinates where the phase dynamics of solutions...
Expand abstract - Publication status:
- Published
- Peer review status:
- Peer reviewed
- Version:
- Accepted manuscript
- Files:
-
-
(pdf, 354.4KB)
-
- Publisher copy:
- 10.1088/1402-4896/aa86fa
-
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- Publisher:
- Institute of Physics Publisher's website
- Journal:
- Physica Scripta Journal website
- Volume:
- 92
- Pages:
- 105001
- Publication date:
- 2017-09-18
- Acceptance date:
- 2017-08-18
- DOI:
- EISSN:
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1402-4896
- ISSN:
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0031-8949
- Pubs id:
-
pubs:724272
- URN:
-
uri:4d761cdd-571e-45fb-88dc-9d0762fd73fe
- UUID:
-
uuid:4d761cdd-571e-45fb-88dc-9d0762fd73fe
- Local pid:
- pubs:724272
- Copyright holder:
- Royal Swedish Academy of Sciences
- Copyright date:
- 2017
- Notes:
- © 2017 The Royal Swedish Academy of Sciences. This is the accepted manuscript version of the article. The final version is available online from Institute of Physics at: https://doi.org/10.1088/1402-4896/aa86fa
Journal article
A nonlinear Klein-Gordon equation for relativistic superfluidity
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