Precession of spheroids under Lorentz violation and observational consequences for neutron stars

نویسندگان

چکیده

The Standard-Model Extension (SME) is an effective-field-theoretic framework that catalogs all Lorentz-violating field operators. anisotropic correction from the minimal gravitational SME to Newtonian energy for spheroids studied, and rotation of rigid solved with perturbation method numerical approach. well-known forced precession solution given by Nordtvedt in parametrized post-Newtonian formalism recovered applied two observed solitary millisecond pulsars set bounds on coefficients Lorentz violation framework. A different solution, which describes otherwise free-precessing star presence violation, found, its consequences pulsar signals continuous waves emitted neutron stars (NSs) are investigated. study provides new possible tests once NSs firmly identified future.

برای دانلود باید عضویت طلایی داشته باشید

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

Precession of Isolated Neutron Stars

I summarize the evidence for precession of isolated neutron stars and theoretical effort to understand the observations. I discuss factors that might set the precession period, describe constraints on the material properties of the crust, and conclude with a brief discussion of possible sources of stress that would deform a neutron star to the extent required.

متن کامل

Observational Consequences of Topological Currents in Neutron Stars

We argue that topological vector currents may be the source of many phenomena in neutron stars: kicks, jets, toroidal fields and magnetic helicity. Topological vector currents exist because of the P-symmetry violation of the weak interaction. Kicks and helicity are both objects that transform as pseudovectors and thus require P-symmetry violation to manifest themselves. This symmetry argument i...

متن کامل

Geodetic Precession in Binary Neutron Stars

The discovery of pulsars in 1967 marked the beginning of a new era in astrophysics. Besides studying pulsars as fascinating astrophysical objects in their own right, these sources serve as invaluable tools in the research of a large variety of physical and astrophysical problems. Studied subjects range from plasma and solid-state physics under extreme conditions to investigations of the interst...

متن کامل

Parity Violation, the Neutron Radius of Lead, and Neutron Stars

The neutron radius of a heavy nucleus is a fundamental nuclear-structure observable that remains elusive. Progress in this arena has been limited by the exclusive use of hadronic probes that are hindered by large and controversial uncertainties in the reaction mechanism. The Parity Radius Experiment at the Jefferson Laboratory offers an attractive electro-weak alternative to the hadronic progra...

متن کامل

Tkachenko waves, glitches and precession in neutron stars

Here I discuss possible relations between free precession of neutron stars, Tkachenko waves inside them and glitches. I note that the proposed precession period of the isolated neutron star RX J0720.4-3125 (Haberl et al. 2006) is consistent with the period of Tkachenko waves for the spin period 8.4 s. Based on a possible observation of a glitch in RX J0720.4-3125 (van Kerkwijk et al. 2007), I p...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

ژورنال

عنوان ژورنال: Physical review

سال: 2021

ISSN: ['0556-2813', '1538-4497', '1089-490X']

DOI: https://doi.org/10.1103/physrevd.103.084028