Neutron star in the presence of a torsion-dilaton field
Classical and Quantum Gravity, ISSN: 0264-9381, Vol: 16, Issue: 7, Page: 2359-2380
1999
- 16Citations
- 3Captures
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Article Description
We develop the general theory of stars in Saa's model of gravity with propagating torsion and study the basic stationary state of a neutron star. Our numerical results show that the torsion force decreases the role of the gravity in the star configuration, leading to significant changes in the neutron star masses depending on the equation of state of star matter. The inconsistency of Saa's model with Roll-Krotkov-Dicke and Braginsky-Panov experiments is discussed.
Bibliographic Details
http://www.scopus.com/inward/record.url?partnerID=HzOxMe3b&scp=0033243668&origin=inward; http://dx.doi.org/10.1088/0264-9381/16/7/314; https://iopscience.iop.org/article/10.1088/0264-9381/16/7/314; https://dx.doi.org/10.1088/0264-9381/16/7/314; https://validate.perfdrive.com/fb803c746e9148689b3984a31fccd902/?ssa=b8f4fa4a-b7d5-4237-abe0-90649c12ec8d&ssb=46323232052&ssc=https%3A%2F%2Fiopscience.iop.org%2Farticle%2F10.1088%2F0264-9381%2F16%2F7%2F314&ssi=5db5d91f-8427-40d3-bf93-111a64ae4bd7&ssk=support@shieldsquare.com&ssm=22526893835010327998747315081227212&ssn=4ec76e03425d34d7b9bef734d0455a2262bca842bdc0-9b7b-4e59-b26ec4&sso=b5f8c0fa-9e3578620ac479f2f60af112e752591d33cb1efde3c8dff7&ssp=25138959421719905843172028242964166&ssq=66648592534760332443941132186386358400212&ssr=NTIuMy4yMTcuMjU0&sst=com.plumanalytics&ssu=&ssv=&ssw=&ssx=eyJ1em14IjoiN2Y5MDAwZWQ3OGYyMmMtODkyYi00NTZhLWFmZTItMzg4OWE4YzkyNDE0NS0xNzE5OTQxMTMyNTY0Mjg0MjE1MzEyLTJiNzQ2NTkxZWRhYzZjOWQ5OTg2OCIsInJkIjoiaW9wLm9yZyIsIl9fdXptZiI6IjdmNjAwMGIzYTMwMWU3LWYyNWUtNGQzOS05NDRiLWFiOWE4ZjQ0OTBjNjE3MTk5NDExMzI1NjQyODQyMTUzMTItZDBiNWZjYzY3ZGNiZDdkOTk5ODY4In0=
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