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Numerical Modeling of Electromagnetic Radiation from AGN Jets Based on -ray emission and spectral evolution of pair plasmas in AGN jets Bottcher et al. Astronomy and Astrophysics Vol. 324 1997 Giridhar Nandikotkur

Numerical Modeling of Electromagnetic Radiation from AGN Jets

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Numerical Modeling of Electromagnetic Radiation from AGN Jets. Based on. -ray emission and spectral evolution of pair plasmas in AGN jets Bottcher et al. Astronomy and Astrophysics Vol. 324 1997. Giridhar Nandikotkur. Numerical Modeling of Electromagnetic Radiation from AGN Jets. - PowerPoint PPT Presentation

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Page 1: Numerical Modeling of Electromagnetic Radiation from AGN Jets

Numerical Modeling of Electromagnetic Radiation from AGN Jets

Based on

-ray emission and spectral evolution of pair plasmas in AGN jets

Bottcher et al. Astronomy and Astrophysics Vol. 324 1997

Giridhar Nandikotkur

Page 2: Numerical Modeling of Electromagnetic Radiation from AGN Jets

Numerical Modeling of Electromagnetic Radiation from AGN Jets

• What are Active Galactic Nuclei (AGN)? Structure Historical Existence

• Physical Processes Experiment leading to theory

a chronological journey Current Status of theoretical methods

• First step- a small one

Page 3: Numerical Modeling of Electromagnetic Radiation from AGN Jets

What are Active Galactic Nuclei (AGNs)?

• Historical Existence Extra-galactic

measured redshifts Extremely bright and violent

presence of jets at all wavelengths

Estimated energy more than of order of 10^60 ergs!

Something gravitational in nature Sharp rise in Luminosity towards the center

Massive object at the center-black hole?

Page 4: Numerical Modeling of Electromagnetic Radiation from AGN Jets

What are Active Galactic Nuclei (AGNs)?

• Structure Black hole at the center Accretion disc Jet Clouds at some distance Ordered magnetic filed lines emanating from BH

Page 5: Numerical Modeling of Electromagnetic Radiation from AGN Jets

Physical Processes• Synchrotron Radiation

suggested by polarization measurements

Experimentally observation: Power law energy spectrum

can be produced by power law distribution of electrons

Page 6: Numerical Modeling of Electromagnetic Radiation from AGN Jets

Physical Processes Photon Scattering by Inverse Comton

emission

Thompson scattering - non-relativistic

Compton Scattering - relativistic: Klein-Nishina

Page 7: Numerical Modeling of Electromagnetic Radiation from AGN Jets

Physical Processes• Broadband Spectrum

Synchrotron radiation has a peak and (dF/dlog) = F vs. will show a peak. Peak around optical-UVfalls towards UV, Xrays

• Compton Gamma Ray Observatory Launch 1991 Detection of sources with high energy gamma ray emission Bulk of their luminosity in Gamma rays A second peak in the broad band spectrum

Explanation by Inverse Compton emission

Page 8: Numerical Modeling of Electromagnetic Radiation from AGN Jets

Torus

BLR

Ac. Disk B. Hole

Electrons

Photons

SED for FSRQ

Peak 1: Synchrotron Radiation

Peak 2. Accretion Disk Black Body

Peak 3. Self Synchrotron Emission (SSC)

Peak 4. External Comption Disk (ECD)

Peak 5. External Compton clouds (ECC)

Page 9: Numerical Modeling of Electromagnetic Radiation from AGN Jets

Theoretical ApproachesNumerical Model.

Assume an injected leptonic (e+ e-)

plasma blob with power law distribution.

Evolution of photon and electron distributions using emission and absorption processes.

Page 10: Numerical Modeling of Electromagnetic Radiation from AGN Jets

Power Law: N()d = C -s dC: Normalization constant N()d = No

Energy Losses

(d /dt)synchrotron ; (d /dt)SSC ; Numerical Integration

(d /dt)ECD ; (d /dt)ECC ;

Change in particle distribution

t = 0 + t * (d /dt)ECD Forward Euler

Photon Spectrum at each time step

Page 11: Numerical Modeling of Electromagnetic Radiation from AGN Jets

Power Law distribution. Log-Log Plot

-1.50

-1.00

-0.50

0.00

0.50

0.0 2.0 4.0 6.0 8.0

Log(Gamma)

Lo

g(N

)

Power Law Distribution

0.0

2.0

4.0

6.0

0 5000 10000 15000 20000 25000

Gamma: Lorentz factor

N(G

am

ma

)

Page 12: Numerical Modeling of Electromagnetic Radiation from AGN Jets

Simulation of ECD process

Scattering of accretion disk photons of electrons

mathematica postscript

Page 13: Numerical Modeling of Electromagnetic Radiation from AGN Jets

Convergence of Trapezoidal Rule

-20

-15

-10

-5

0

5

10

0 2000 4000 6000 8000 10000 12000

Number of steps

Lo

g (

Dif

fere

nce

)

Cos(x) (0-Pi/2)

Cos(x) (0,Pi)

2x + 3x^2 +5x^4

Power Law

Page 14: Numerical Modeling of Electromagnetic Radiation from AGN Jets

Energy Loss Rate from Compton Scattering of Disk Radiation

-1

0

1

2

3

4

5

6

3 3.5 4 4.5 5 5.5 6 6.5

Lorentz factor of electrons

En

erg

y L

oss

Ra

te

ELR

Has to match exactly with the paper.If not, find the parameter that is differentin the initialization

Page 15: Numerical Modeling of Electromagnetic Radiation from AGN Jets

Future Work

• Include other processes.

• Generate Photon Spectrum

• Explore Gaussian Quadrature to Numerically integrate.

• Ambitious Target: 3 months!