Model Spectra of Neutron Star Surface Thermal Emission Department of Physics National Tsing Hua...

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Model Spectra of Neutron Model Spectra of Neutron Star Surface Thermal Star Surface Thermal Emission Emission Department of Physics National Tsing Hua Univ ersity Lun-Wen Yeh 2004.5.6
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Transcript of Model Spectra of Neutron Star Surface Thermal Emission Department of Physics National Tsing Hua...

Page 1: Model Spectra of Neutron Star Surface Thermal Emission Department of Physics National Tsing Hua University Lun-Wen Yeh 2004.5.6.

Model Spectra of Neutron Model Spectra of Neutron Star Surface Thermal Star Surface Thermal EmissionEmission

Department of Physics

National Tsing Hua University

Lun-Wen Yeh 2004.5.6

Page 2: Model Spectra of Neutron Star Surface Thermal Emission Department of Physics National Tsing Hua University Lun-Wen Yeh 2004.5.6.

Structure of neutron star

Radiation transfer equation

Temperature correction

Flux ≠const

Flux = constSpectrum

P(τ) ρ(τ) T(τ)

Page 3: Model Spectra of Neutron Star Surface Thermal Emission Department of Physics National Tsing Hua University Lun-Wen Yeh 2004.5.6.

AssumptionsAssumptions Plane-parallel atmosphere( local model)Plane-parallel atmosphere( local model)

Radiative equilibrium( energy transported solely by radiation ) Radiative equilibrium( energy transported solely by radiation )

Equation of state is ideal gas( ionized H) Equation of state is ideal gas( ionized H)

Neglect conduction and convectionNeglect conduction and convection

HydrostaticsHydrostatics

No magnetic fieldNo magnetic field

The physical properties independent of timeThe physical properties independent of time

Page 4: Model Spectra of Neutron Star Surface Thermal Emission Department of Physics National Tsing Hua University Lun-Wen Yeh 2004.5.6.

Structure of NSStructure of NS

Gray atmosphere Gray atmosphere

Equation of stateEquation of state

Oppenheimer-VolkoffOppenheimer-VolkoffkT

mP p

2

Page 5: Model Spectra of Neutron Star Surface Thermal Emission Department of Physics National Tsing Hua University Lun-Wen Yeh 2004.5.6.
Page 6: Model Spectra of Neutron Star Surface Thermal Emission Department of Physics National Tsing Hua University Lun-Wen Yeh 2004.5.6.

Structure of NSStructure of NS

Rosseland meanRosseland mean

Page 7: Model Spectra of Neutron Star Surface Thermal Emission Department of Physics National Tsing Hua University Lun-Wen Yeh 2004.5.6.

Radiation transfer equationRadiation transfer equationAbsorption Spontaneous emission Induced emission

Scattering

Page 8: Model Spectra of Neutron Star Surface Thermal Emission Department of Physics National Tsing Hua University Lun-Wen Yeh 2004.5.6.

Radiation transfer Radiation transfer equationequation

Diffusion approimation

Page 9: Model Spectra of Neutron Star Surface Thermal Emission Department of Physics National Tsing Hua University Lun-Wen Yeh 2004.5.6.

Feautrier methodFeautrier methodMean intensity like

Flux like

1

0

2

1

2

i1

2

j

2

ij

R

SCi

ii

1

0

2

1

2

i1

2

j

2

ij

R

SCi

ii

j

j

),(g)(P),(g)(P2163

S)(Id

)(dI

),(g)(P),(g)(P2163

S)(Id

)(dI

Page 10: Model Spectra of Neutron Star Surface Thermal Emission Department of Physics National Tsing Hua University Lun-Wen Yeh 2004.5.6.

Feautrier methodFeautrier method

Surface normal n

Page 11: Model Spectra of Neutron Star Surface Thermal Emission Department of Physics National Tsing Hua University Lun-Wen Yeh 2004.5.6.

Feautrier methodFeautrier method

ddddddd SPAPBPC 11

Page 12: Model Spectra of Neutron Star Surface Thermal Emission Department of Physics National Tsing Hua University Lun-Wen Yeh 2004.5.6.

Feautrier methodFeautrier method

ddddddd SPAPBPC 11

d=2,3,……,D-2,D-1

μ=1,2,……M

Page 13: Model Spectra of Neutron Star Surface Thermal Emission Department of Physics National Tsing Hua University Lun-Wen Yeh 2004.5.6.

Feautrier methodFeautrier method

I1

I2

I3

..

..

..

I1

I2

I3

..

..

..

I1

I2

I3

..

..

..

d=1 d=2 d=3…..

Page 14: Model Spectra of Neutron Star Surface Thermal Emission Department of Physics National Tsing Hua University Lun-Wen Yeh 2004.5.6.

Test Feautrier methodTest Feautrier method

Scattering

Page 15: Model Spectra of Neutron Star Surface Thermal Emission Department of Physics National Tsing Hua University Lun-Wen Yeh 2004.5.6.
Page 16: Model Spectra of Neutron Star Surface Thermal Emission Department of Physics National Tsing Hua University Lun-Wen Yeh 2004.5.6.
Page 17: Model Spectra of Neutron Star Surface Thermal Emission Department of Physics National Tsing Hua University Lun-Wen Yeh 2004.5.6.

Test Feautrier methodTest Feautrier method

Scattering and free-free absorption

Page 18: Model Spectra of Neutron Star Surface Thermal Emission Department of Physics National Tsing Hua University Lun-Wen Yeh 2004.5.6.

46~91 4.9%

91~901 4.1%

901~9001 0.39%

Page 19: Model Spectra of Neutron Star Surface Thermal Emission Department of Physics National Tsing Hua University Lun-Wen Yeh 2004.5.6.

46~91 0.29%

91~901 0.17%

901~9001 0.0079%

Page 20: Model Spectra of Neutron Star Surface Thermal Emission Department of Physics National Tsing Hua University Lun-Wen Yeh 2004.5.6.

46~91 0.19%

91~901 0.065%

901~9001 0.0058%

Page 21: Model Spectra of Neutron Star Surface Thermal Emission Department of Physics National Tsing Hua University Lun-Wen Yeh 2004.5.6.
Page 22: Model Spectra of Neutron Star Surface Thermal Emission Department of Physics National Tsing Hua University Lun-Wen Yeh 2004.5.6.
Page 23: Model Spectra of Neutron Star Surface Thermal Emission Department of Physics National Tsing Hua University Lun-Wen Yeh 2004.5.6.
Page 24: Model Spectra of Neutron Star Surface Thermal Emission Department of Physics National Tsing Hua University Lun-Wen Yeh 2004.5.6.

46~91 4.2%

91~901 3.6%

901~9001 0.30%

Page 25: Model Spectra of Neutron Star Surface Thermal Emission Department of Physics National Tsing Hua University Lun-Wen Yeh 2004.5.6.

Future workFuture work

Run my program with many directions , Run my program with many directions , and carry out temperature-correction.and carry out temperature-correction.

Add magnetic filed in local model Add magnetic filed in local model