title: ÐÐ»Ð¸ÑÐ½Ð¸Ðµ Ð¸ÑÐºÑÐ¸Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿ÑÐ¾ÑÑÑÐ°Ð½ÑÑÐ²Ð° Ð½Ð° Ð¼Ð¾Ð¼ÐµÐ½Ñ Ð¸Ð½ÐµÑÑÐ¸Ð¸ Ð½ÐµÐ¾ÑÐµÑÐ¸Ð¼Ð¼ÐµÑÑÐ¸ÑÐ½Ð¾Ð³Ð¾ Ð²Ð½ÐµÑÐ½ÐµÐ³Ð¾ Ð¼Ð°Ð³Ð½Ð¸ÑÐ½Ð¾Ð³Ð¾ Ð¿Ð¾Ð»Ñ Ð¿ÑÐ»ÑÑÐ°ÑÐ°
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¼Ð°Ð³Ð¸ÑÑÑÐ°
titleType: Subtitle
title: The effect of the curvature of space on the moment of inertia of the non-axisymmetric external magnetic field of the pulsar
Creators: name: ÐÐ°ÑÐµÐ²Ð¾ÑÑÐ½, ÐÑÐ°Ð¼
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2024
Subjects: ÐÑÐ»ÑÑÐ°ÑÑ
ÐÐ²ÐµÐ·Ð´Ñ Ð½ÐµÐ¹ÑÑÐ¾Ð½Ð½ÑÐµ
ÐÐ°Ð³Ð½Ð¸ÑÐ½Ð¾Ðµ Ð¿Ð¾Ð»Ðµ
ÐÑÐµÐ¼Ð¸ÑÐ½Ð¾Ðµ ÑÑÐ³Ð¾ÑÐµÐ½Ð¸Ðµ
Ð¿ÑÐµÑÐµÑÑÐ¸Ñ
Ð¼Ð¾Ð¼ÐµÐ½Ñ Ð¸Ð½ÐµÑÑÐ¸Ð¸
Ð¼ÐµÑÑÐ¸ÐºÐ° Ð¨Ð²Ð°ÑÑÑÐ¸Ð»ÑÐ´Ð°
Ð¸Ð½Ð´ÐµÐºÑ ÑÐ¾ÑÐ¼Ð¾Ð¶ÐµÐ½Ð¸Ñ
precession
moment of inertia
Schwarzschild metric
deceleration index

description: ÐÐ°Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð¸Ñ, ÐºÐ°ÐºÐ¾Ðµ Ð²Ð»Ð¸ÑÐ½Ð¸Ðµ Ð¾ÐºÐ°Ð·ÑÐ²Ð°ÐµÑ ÑÑÐµÑ Ð¸ÑÐºÑÐ¸Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿ÑÐ¾ÑÑÑÐ°Ð½ÑÑÐ²Ð° Ð² Ð¼ÐµÑÑÐ¸ÐºÐµ Ð¨Ð²Ð°ÑÑÑÐ¸Ð»ÑÐ´Ð° Ð½Ð° Ð²ÐºÐ»Ð°Ð´ Ð¼Ð°Ð³Ð½Ð¸ÑÐ½Ð¾Ð³Ð¾ Ð¿Ð¾Ð»Ñ Ð²Ð½Ðµ Ð½ÐµÐ¹ÑÑÐ¾Ð½Ð½Ð¾Ð¹ Ð·Ð²ÐµÐ·Ð´Ñ Ð² Ð¼Ð¾Ð¼ÐµÐ½Ñ Ð¸Ð½ÐµÑÑÐ¸Ð¸ ÑÐ°Ð´Ð¸Ð¾Ð¿ÑÐ»ÑÑÐ°ÑÐ°. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÑÑ Ð·Ð°Ð²Ð¸ÑÐ¸Ð¼Ð¾ÑÑÑ ÑÑÐ¾Ð³Ð¾ Ð²ÐºÐ»Ð°Ð´Ð° ÐºÐ°Ðº Ð¸ Ð¾Ñ ÑÐ¾Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ñ r_g /r_ns , Ð³Ð´Ðµ r_ns â ÑÐ°Ð´Ð¸ÑÑ Ð½ÐµÐ¹ÑÑÐ¾Ð½Ð½Ð¾Ð¹ Ð·Ð²ÐµÐ·Ð´Ñ, Ð° r_g â ÐµÑ Ð³ÑÐ°Ð²Ð¸ÑÐ°ÑÐ¸Ð¾Ð½Ð½ÑÐ¹ ÑÐ°Ð´Ð¸ÑÑ, ÑÐ°Ðº Ð¸ Ð¾Ñ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÐ° Ð¼ÑÐ»ÑÑÐ¸Ð¿Ð¾Ð»ÑÐ½Ð¾ÑÑÐ¸ l. ÐÐ¾ÐºÐ°Ð·Ð°Ð½Ð¾, ÑÑÐ¾ Ð²Ð»Ð¸ÑÐ½Ð¸Ðµ Ð¸ÑÐºÑÐ¸Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿ÑÐ¾ÑÑÑÐ°Ð½ÑÑÐ²Ð° ÑÐ¼ÐµÐ½ÑÑÐ°ÐµÑ Ð²ÐºÐ»Ð°Ð´ Ð²Ð½ÐµÑÐ½ÐµÐ³Ð¾ Ð¼Ð°Ð³Ð½Ð¸ÑÐ½Ð¾Ð³Ð¾ Ð¿Ð¾Ð»Ñ Ð² Ð¾ÑÐ»Ð¸ÑÐ¸Ðµ ÑÐµÐ½Ð·Ð¾ÑÐ° Ð¸Ð½ÐµÑÑÐ¸Ð¸ Ð¾Ñ ÑÑÐµÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ»ÑÑÐ°Ñ Ð² Ð½ÐµÑÐºÐ¾Ð»ÑÐºÐ¾ ÑÐ°Ð· Ð¿ÑÐ¸ ÑÐ¸ÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð¼ Ð¼Ð°Ð³Ð½Ð¸ÑÐ½Ð¾Ð¼ Ð¿Ð¾Ð»Ñ Ð½Ð° Ð¿Ð¾Ð²ÐµÑÑÐ½Ð¾ÑÑÐ¸ Ð·Ð²ÐµÐ·Ð´Ñ. ÐÐ¾Ð¼Ð¸Ð¼Ð¾ ÑÑÐ¾Ð³Ð¾ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÐµÑÑÑ, ÐºÐ°ÐºÐ¾Ðµ Ð²Ð»Ð¸ÑÐ½Ð¸Ðµ Ð¾ÐºÐ°Ð·ÑÐ²Ð°ÐµÑ Ð¸ÑÐºÑÐ¸Ð²Ð»ÐµÐ½Ð¸Ðµ Ð¿ÑÐ¾ÑÑÑÐ°Ð½ÑÑÐ²Ð° Ð½Ð° Ð¾ÑÐµÐ½ÐºÑ Ð¼Ð°ÐºÑÐ¸Ð¼Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð·Ð½Ð°ÑÐµÐ½Ð¸Ñ Ð¸Ð½Ð´ÐµÐºÑÐ° ÑÐ¾ÑÐ¼Ð¾Ð¶ÐµÐ½Ð¸Ñ. ÐÐ¾ÐºÐ°Ð·Ð°Ð½Ð° Ð·Ð°Ð²Ð¸ÑÐ¸Ð¼Ð¾ÑÑÑ ÑÑÐ¾Ð³Ð¾ Ð²Ð»Ð¸ÑÐ½Ð¸Ñ Ð¾Ñ ÑÐ¾Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ñ r_g /r_ns , Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÐ° l Ð¸ m.
description: The given work is devoted to consideration what effect accounting for the curvature of space in the Schwarzschild metric has on the contribution of the magnetic field outside the neutron star at the moment of inertia of theradio pulsar. The simplest configuration of the magnetic field was used for consideration - its description by only one harmonic. Consider the dependence of this contribution both on the ratio r_g /r_ns , where r_ns is the radius of a neutron star, and r_g is its gravitational radius, and on the multipole parameter l. It is shown that the effect of space curvature reduces the contribution of the external magnetic field in contrast to the inertia tensor from the spherical case by several times with a fixed magnetic field on the surface of the star. In addition, it is considered what effect the curvature of space has on the assessment of the maximum value of the braking index. The dependence of this effect on the ratio r_g /r_ns , the parameter l and m is shown.