Abstract
A system of equations and inequalities that allows one to determine the constraints on central density ρ c and the chemical composition, which is governed by parameter μ e , of the white dwarf RX J0648.0- 4418 with a record short period of rotation T = 13.18s and mass m = (1.28 ± 0.05)m⊙, has been derived. The analysis of numerical solutions of this system reveal a complex dependence of μ e on ρ c . The intervals of variation of μ e and ρ c are as follows: 1.09 ≤ μ e ≤ 1.21 and 9.04 ≤ μ e /ρ0 ≤ 103 (ρ0 = 0.98 × 106 g/cm3). This range of μ e values suggests that the white dwarf RX J0648.0-4418 is not made of pure hydrogen and should contain 9–21% of heavy elements. Calculations have been performed with the equation of state of an ideal degenerate electron gas. Approximate analytic expressions (with an accuracy of 10-3) for the minimum period T min and mass m of the white dwarf are obtained. It is demonstrated that the white-dwarf mass is almost doubled (compared to the case of no rotation at a fixed central density) as period T approaches T min.
Similar content being viewed by others
References
S. Mereghetti, “RXJ0648.0-4418: the fastest-spinning white dwarf,” in Proceedings of 13th Marcel Grossman Meeting MG13, Stockholm, Sweden, July 1–7, 2012, arXiv:1302.4634v1 [astro-ph.HE] (2013), pp. 1–3.
A. Scholz and J. Eislöffel, “Rotation and variability of very low mass stars and brown dwarfs near γ Ori,” Astron. Astrophys. 429, 1007–1023 (2005); arXiv:astro-ph/0410101v1 (2004), pp. 1–17.
S. L. Shapiro and S. Teukolsky, Black Holes, White Dwarfs, and Neutron Stars: Physics of Compact Objects (Wiley, New York, 1983).
V. E. Fortov, Thermodynamics and Equations of State for Matter. From Ideal Gas to Quark-Gluon Plasma (Fizmatlit, Moscow, 2012; World Scientific, Singapore, 2016).
S. A. Mikheev and V. P. Tsvetkov, “Polynomial and polytropic approximations in equation of equilibrium post-newtonian rotating configurations of degenerate neutron gas,” Phys. Part. Nucl. Lett. 7, 1 (2010).
E. V. Bespal’ko, S. A. Mikheev, I. V. Puzynin, and V. P. Tsvetkov, “A gravitating rapidly rotating superdense configuration with relativistic state equations,” Mat. Model. 18 (3), 103 (2006).
S. A. Mikheev and V. P. Tsvetkov, “Critical points and points of the bifurcaton of the rotating magnetized newtonian polytropes with a index,” Phys. Part. Nucl. Lett. 10, 234–242 (2013).
J.-L. Tassoul, Theory of Rotating Stars (Princeton Univ. Press, Princeton, 1978).
S. A. Mikheev and V. P. Tsvetkov, “Mathematical model of equilibrium rotating Newton configurations of degenerate fermi-gas,” Vestn. Tver. Univ., Ser. Prikl. Mat., No. 2, 15–22 (2009).
V. P. Tsvetkov and V. V. Masyukov, “The Buermann- Lagrange series method in the problem of analytical representation of the newtonian potential of perturbed ellipsoidal configurations,” Dokl. Akad. Nauk SSSR 3, 1099–1102 (1990).
V. V. Ermakov and N. N. Kalitkin, “The optimal step and regularization for Newton’s method,” Zh. Vychisl. Mat. Mat. Fiz. 21, 491–497 (1981).
S. A. Mikheev and V. P. Tsvetkov, “Critical points of density distribution of rapidly rotating superdense newtonian polytropes,” Phys. Part. Nucl. Lett. 7, 384–390 (2010).
Upasana Das and Banibrata Mukhopadhyay, “New mass limit for white dwarfs: super-Chandrasekhar type is supernova as a new standard candle,” Phys. Rev. Lett. 110, 071102 (2013); arXiv:1301.5965v1 [astro-ph.SR] (2013), pp. 1–7.
Author information
Authors and Affiliations
Corresponding author
Additional information
Original Russian Text © S.A. Mikheev, V.P. Tsvetkov, 2016, published in Pis’ma v Zhurnal Fizika Elementarnykh Chastits i Atomnogo Yadra, 2016.
Rights and permissions
About this article
Cite this article
Mikheev, S.A., Tsvetkov, V.P. Constraints on the central density and chemical composition of the white dwarf RX J0648.0-4418 with a record period of rotation in a model with the equation of state of an ideal degenerate electron gas. Phys. Part. Nuclei Lett. 13, 442–450 (2016). https://doi.org/10.1134/S1547477116040099
Received:
Published:
Issue Date:
DOI: https://doi.org/10.1134/S1547477116040099