Why I-Love-Q: Explaining why universality emerges in compact objects
dc.contributor.author | Yagi, Kent | |
dc.contributor.author | Stein, Leo C. | |
dc.contributor.author | Pappas, George | |
dc.contributor.author | Yunes, Nicolás | |
dc.contributor.author | Apostolatos, Theocharis A. | |
dc.date.accessioned | 2014-12-02T20:41:47Z | |
dc.date.available | 2014-12-02T20:41:47Z | |
dc.date.issued | 2014 | |
dc.description.abstract | Black holes are said to have no hair because all of their multipole moments can be expressed in terms of just their mass, charge and spin angular momentum. The recent discovery of approximately equation-of-state-independent relations among certain multipole moments in neutron stars suggests that they are also approximately bald. We here explore the yet unknown origin for this universality. First, we investigate which region of the neutron star’s interior and of the equation of state is most responsible for the universality. We find that the universal relation between the moment of inertia and the quadrupole moment is dominated by the star’s outer core, a shell of width 50%–95% of the total radius, which corresponds to the density range 1014–1015 g/cm3. In this range, realistic neutron star equations of state are not sufficiently similar to each other to explain the universality observed. Second, we study the impact on the universality of approximating stellar isodensity contours as self-similar ellipsoids. An analytical calculation in the nonrelativistic limit reveals that the shape of the ellipsoids per se does not affect the universal relations much, but relaxing the self-similarity assumption can completely destroy it. Third, we investigate the eccentricity profiles of rotating relativistic stars and find that the stellar eccentricity is roughly constant, with variations of roughly 20%–30% in the region that matters to the universal relations. Fourth, we repeat the above analysis for differentially rotating, noncompact, regular stars and find that this time the eccentricity is not constant, with variations that easily exceed 100%, and moreover universality is lost. These findings suggest that universality arises as an emergent approximate symmetry: as one flows in the stellar-structure phase space from noncompact star region to the relativistic star region, the eccentricity variation inside stars decreases, leading to approximate self-similarity in their isodensity contours, which then leads to the universal behavior observed in their exterior multipole moments. | en_US |
dc.description.sponsorship | We would like to thank Ben Owen, Jan Steinhoff, Terence Delsate and Katerina Chatziioannou for useful comments and suggestions. N. Y. acknowledges support from NSF Grant No. PHY-1114374 and the NSF CAREER Award No. PHY-1250636, as well as support provided by the National Aeronautics and Space Administration from Grant No. NNX11AI49G, under sub-award 00001944. L. C. S. acknowledges that support for this work was provided by the National Aeronautics and Space Administration through Einstein Postdoctoral Fellowship Award No. PF2-130101 issued by the Chandra X-ray Observatory Center, which is operated by the Smithsonian Astrophysical Observatory for and on behalf of the National Aeronautics Space Administration under Contract No. NAS8-03060, and further acknowledges support from NSF Grant No. PHY-1068541. G. P. acknowledges financial support from the European Research Council under the European Union’s Seventh Framework Programme (FP7/2007-2013)/ERC Grant Agreement No. 306425 “Challenging General Relativity.” Some calculations used the computer algebra systems MAPLE, in combination with the GRTENSORII package. | en_US |
dc.identifier.citation | Yagi, Kent, Leo C. Stein, George Pappas, Nicolas Yunes, and Theocharis A. Apostolatos. "Why I-Love-Q: Explaining why universality emerges in compact objects." Physical Review D 90, no. 6 (2014): 063010. http://dx.doi.org/10.1103/PhysRevD.90.063010 | en_US |
dc.identifier.issn | 1550-7998 | |
dc.identifier.uri | http://dx.doi.org/10.1103/PhysRevD.90.063010 | |
dc.identifier.uri | https://scholarworks.montana.edu/handle/1/8737 | |
dc.publisher | American Physical Society | en_US |
dc.subject | Astrophysics | en_US |
dc.subject | Mechanics | en_US |
dc.title | Why I-Love-Q: Explaining why universality emerges in compact objects | en_US |
dc.type | Article | en_US |
mus.citation.extentfirstpage | 63010 | en_US |
mus.citation.issue | 6 | en_US |
mus.citation.journaltitle | Physical Review D | en_US |
mus.citation.volume | 90 | en_US |
mus.identifier.category | Physics & Mathematics | en_US |
mus.identifier.doi | 10.1103/PhysRevD.90.063010 | en_US |
mus.relation.college | College of Letters & Science | |
mus.relation.college | College of Letters & Sciences | en_US |
mus.relation.department | Physics. | en_US |
mus.relation.university | Montana State University - Bozeman | en_US |
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