Question #55061

The synchrotron power P radiated by an ultrarelativistic (1) electron is extracted from its kinetic energy E mec2. The synchrotron lifetime of such an electron is:

Estimate the synchrotron lifetime of electrons responsible for the 1 GHz radiation from our Galaxy. You may make the approximation that Galactic synchrotron radiation at frequency v = 1 GHz is produced primarily by electrons whose critical frequency in the B = 5 × 10−6 G magnetic field of our Galaxy is vc = 1 GHz.
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Expert's answer

2015-10-19T00:00:46-0400

Answer on Question 55061, Physics / Astronomy | Astrophysics:

Question:

The synchrotron power P radiated by an ultrarelativistic (1) electron is extracted from its kinetic energy E mec2. The synchrotron lifetime of such an electron is?

Estimate the synchrotron lifetime of electrons responsible for the 1 GHz radiation from our Galaxy. You may make the approximation that Galactic synchrotron radiation at frequency v=1v = 1 GHz is produced primarily by electrons whose critical frequency in the B=5×106B = 5 \times 10^{-6} G magnetic field of our Galaxy is vc=1v_c = 1 GHz.

Solution:

Synchrotron power is given by:


P=43σTβ2γ2cUB, whereP = \frac {4}{3} \sigma_ {T} \beta^ {2} \gamma^ {2} c U _ {B}, \text{ where}UB=B28π, andU _ {B} = \frac {B ^ {2}}{8 \pi}, \text{ and}σT=8π3(e2mec2)2\sigma_ {T} = \frac {8 \pi}{3} \left(\frac {e ^ {2}}{m _ {e} c ^ {2}}\right) ^ {2}


Therefore:


P=438π3(e2mec2)β2γ2c×B28π=49ε4β2γ2B2me2c2P = \frac {4}{3} \frac {8 \pi}{3} \left(\frac {e ^ {2}}{m _ {e} c ^ {2}}\right) \beta^ {2} \gamma^ {2} c \times \frac {B ^ {2}}{8 \pi} = \frac {4}{9} \frac {\varepsilon^ {4} \beta^ {2} \gamma^ {2} B ^ {2}}{m _ {e} ^ {2} c ^ {2}}


The critical frequency is:


νc=32γ2νGsina=32γ2ωG2πsina=3γ24πeBmecsinaλ=4πmecνc3eBsina\nu_ {c} = \frac {3}{2} \gamma^ {2} \nu_ {G} \sin a = \frac {3}{2} \gamma^ {2} \frac {\omega_ {G}}{2 \pi} \sin a = \frac {3 \gamma^ {2}}{4 \pi} \frac {e B}{m _ {e} c} \sin a \Rightarrow \lambda = \sqrt {\frac {4 \pi m _ {e} c \nu_ {c}}{3 e B \sin a}}


Assume sin0.5\sin \sim 0.5. Then we get γ104\gamma \sim 10^4, and β1\beta \sim 1.


τEP=λmec249ε4β2γ2B2me2c2=3×1015sec\tau \approx \frac {E}{P} = \frac {\lambda m _ {e} c ^ {2}}{\frac {4}{9} \frac {\varepsilon^ {4} \beta^ {2} \gamma^ {2} B ^ {2}}{m _ {e} ^ {2} c ^ {2}}} = 3 \times 10^{15} \text{sec}


Answer: t108t \sim 10^{8} years

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