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Raman scattering in high-radio-brightness astrophysical systems: application to active galactic nuclei

Levinson, Amir and Blandford, Roger (1995) Raman scattering in high-radio-brightness astrophysical systems: application to active galactic nuclei. Monthly Notices of the Royal Astronomical Society, 274 (3). pp. 717-729. ISSN 0035-8711. https://resolver.caltech.edu/CaltechAUTHORS:20190523-125439785

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Abstract

Under conditions of high brightness temperature, stimulated Raman scattering of incident radio waves by Langmuir waves can occur. This process is analysed for a broad-band radio spectrum, and analytic and numerical models for special cases are presented. Two cases are identified. In strong Raman scattering, the radio brightness temperature is so large that the intensity of the Langmuir waves responsible for the scattering grows to non-linear strength and the radio waves are quickly scattered. In weak Raman scattering, the electrostatic wave intensity is determined by a balance between parametric growth and ion-electron collisional damping. In either case, back-scattering will only occur if the electron density, n, is high enough to allow Langmuir waves of short enough wavelength to propagate without Landau damping; at lower density, the radio waves will be scattered through an angle ∼0.2(n/10^6 cm^(−3))^(1/2)(T/10^6 K)^(−1/2)(v/1 GHz)^(−1⁠). In the weak, back-scattering regime, the reflection length is roughly 3 × 10^(11)(T/10^6 K)^(−3/2)(v/1 GHz)^(−2)(T_B/10^(15) K)^(−2)(T_B/10^(15) K)^(−2) cm⁠, independent of density, where TB is the brightness temperature. It is argued that intraday variability in compact extragalactic radio sources is probably not caused by a coherent emission mechanism with brightness temperature ∼10^(18) K, because the plasma density within and around the source would then have to be unreasonably low. Implications for space very long baseline interferometry (VLBI) and for tracing accretion flows in active galactic nuclei are also briefly discussed. By contrast, source models where the brightness temperature ≳ 10^(14) K are not seriously constrained by Raman scattering.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1093/mnras/274.3.717DOIArticle
http://adsabs.harvard.edu/abs/1995MNRAS.274..717LADSArticle
ORCID:
AuthorORCID
Blandford, Roger0000-0002-1854-5506
Additional Information:© 1995 Royal Astronomical Society. Provided by the NASA Astrophysics Data System. Accepted 1994 December 20. Received 1994 November 25; in original form 1994 June 30. We thank D. L. Meier for information concerning Space VLBI. This work was supported by NASA grants NAGW 2816 and 2372.
Group:TAPIR
Funders:
Funding AgencyGrant Number
NASANAGW 2816
NASANAGW 2372
Subject Keywords:plasmas, scattering, waves, galaxies: active, galaxies: nuclei, radio continuum: galaxies
Issue or Number:3
Record Number:CaltechAUTHORS:20190523-125439785
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20190523-125439785
Official Citation:Amir Levinson, Roger Blandford, Raman scattering in high-radio-brightness astrophysical systems: application to active galactic nuclei, Monthly Notices of the Royal Astronomical Society, Volume 274, Issue 3, 1 June 1995, Pages 717–729, https://doi.org/10.1093/mnras/274.3.717
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:95759
Collection:CaltechAUTHORS
Deposited By: George Porter
Deposited On:23 May 2019 20:35
Last Modified:03 Oct 2019 21:16

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