 
 
 
 
 
   
When an electron is not at rest, but colliding with a soft photon,
the recoiling photon gains its energy by the transfer from the incoming
electrons. 
This process called Inverse Compton Scattering,
 , is a representative radiation in many astronomical
environments that produces high energy X-ray/
, is a representative radiation in many astronomical
environments that produces high energy X-ray/ -ray.
-ray.
The colliding energy between a photon and an electron
is often defined by the he Lorentz invariant
center of mass (CM) energy squared  as defined by
 as defined by
 and
 and 
 are 4-momentum of the  electron  and the photon respectively.
 
are 4-momentum of the  electron  and the photon respectively.
 can be rewritten in the different system:
 can be rewritten in the different system: 
 .
In this expression, the photon energy
.
In this expression, the photon energy 
 in the electron rest system in Eq. 25
is written by
in the electron rest system in Eq. 25
is written by
|  | (28) | 
 as a function of incoming electron energy
as a function of incoming electron energy  in the lab system as
 in the lab system as
 is the recoiling energy of
 is the recoiling energy of  -ray
in the Universe lab system. 
By using Eq. 29 
we can modify the Kline-Nishina
formula Eq. 25 
to derive the energy differential
cross section. We obtain
-ray
in the Universe lab system. 
By using Eq. 29 
we can modify the Kline-Nishina
formula Eq. 25 
to derive the energy differential
cross section. We obtain
 is the dimensionless energy of the electron
normalized by primary energy of incoming electron.
The electron transfer most of its
energy to the photon via the inverse Compton scattering
as you see the cross section becomes larger in
 is the dimensionless energy of the electron
normalized by primary energy of incoming electron.
The electron transfer most of its
energy to the photon via the inverse Compton scattering
as you see the cross section becomes larger in  regime
in Eq. 30.
Integrating
 regime
in Eq. 30.
Integrating  from
 from  to 1
(this range is given by Eq. 29
with
 to 1
(this range is given by Eq. 29
with 
 ), we obtain the total cross section:
), we obtain the total cross section:
|  |  |  | |
| ![$\displaystyle -{1\over \beta^2}(2-3\beta^2-\beta^3)\ln{1+\beta\over 1-\beta}],$](img121.png) | (31) | 
 is the velocity
of the outgoing electron in the CMS.
 is the velocity
of the outgoing electron in the CMS.
 
 
 
 
