2020
DOI: 10.1134/s1063772920020031
|View full text |Cite
|
Sign up to set email alerts
|

3D Simulation of Anisotropic Heat Transfer in Outer Layers of Magnetized Neutron Stars

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
1
1
1

Citation Types

0
7
0

Year Published

2020
2020
2020
2020

Publication Types

Select...
2
1

Relationship

0
3

Authors

Journals

citations
Cited by 3 publications
(7 citation statements)
references
References 28 publications
0
7
0
Order By: Relevance
“…where T s is the local surface temperature, K = K(B, θ B , T, ρ) is the effective opacity, θ B is the magnetic field inclination angle to a normal to the surface, g s = GM NS /(R 2 NS 1 − r g /R NS ) is the surface gravity acceleration, where G is the gravitational constant, and r g is the gravitational radius of the NS. For the effective opacity we assume the electron heat transfer (2.3) and radiative one for free-free and bound-free transitions and electron Thomson scattering with taking into account the degeneracy of the electrons [19]. Due to additivity of the thermal conductivity coefficient for electron and radiative processes the exact effective opacity reads as follows (e.g.…”
Section: Thermal Structure Of An Outer Envelopementioning
confidence: 99%
See 3 more Smart Citations
“…where T s is the local surface temperature, K = K(B, θ B , T, ρ) is the effective opacity, θ B is the magnetic field inclination angle to a normal to the surface, g s = GM NS /(R 2 NS 1 − r g /R NS ) is the surface gravity acceleration, where G is the gravitational constant, and r g is the gravitational radius of the NS. For the effective opacity we assume the electron heat transfer (2.3) and radiative one for free-free and bound-free transitions and electron Thomson scattering with taking into account the degeneracy of the electrons [19]. Due to additivity of the thermal conductivity coefficient for electron and radiative processes the exact effective opacity reads as follows (e.g.…”
Section: Thermal Structure Of An Outer Envelopementioning
confidence: 99%
“…Solving equation (2.10) numerically for different magnetic fields, inclination angles and surface temperatures leads to a so-called T s − T b -relationship, tabulated or analytically approximated function, which relates the surface temperature T s with the temperature at the boundary between the crust and the envelope T b . Results of several calculations are presented on Table 1, more results and a detailed discussion can be found in [19]. We use the tabulated T s − T b -relationship as a boundary condition for the heat transfer equation in the crust (see next section).…”
Section: Thermal Structure Of An Outer Envelopementioning
confidence: 99%
See 2 more Smart Citations
“…Heat transfer processes in the outer layers of the NS with the coaxial dipolar and quadrupolar fields were considered earlier in the paper Kondratyev et al (2020), hereinafter referred as Paper I, where the model of the magnetized envelope and used numerical technique are described in details. In this paper we obtain stationary temperature distribution in outer layers of NSs in the presence of dipole and quadrupole fields, whose axes are not aligned.…”
Section: Introductionmentioning
confidence: 99%