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Radiant Pressure

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23 views1 page

Radiant Pressure

Uploaded by

f9876995
Copyright
© © All Rights Reserved
We take content rights seriously. If you suspect this is your content, claim it here.
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Intensity of photons/ Incoming Light

The energy of photons, striking normally per unit area per unit time is called intensity of
wave.
Let N photons striking on a area A in time t such that the
direction of velocity of photons and normal to the surface
are inclined at angle  then Acos
E0  h  Energy of each photon
E  Nh  Total energy of photons striking on the area A 
Nh nh 
I= = , where,
At cos  cos  A
  frequency of each photon
n  number of photons striking on a unit area per unit time.
Icos 
 h = = mc2 = pc
n
Icos 
 p = momentum of each photon =
nc
Calculation of Radiant pressure and force on the surface

Case-I: Let the photons are completely absorbed by surface

psin F2
Photon
F1
Photon F2
 p F1 Photon rest
pcos
FBD of surface FBD of photon
Just before Absorption Just after Absorption
At the time of Absorption
F1 = Change of component of momentum of photons perpendicular to surface per unit time
IA cos2  F Icos2 
 F1  nAp cos    Radiant pressure due to absorption  pa  1 
c A c
F2 = Change of component of momentum of photons along the surface per unit time
IA cos  sin 
 F2  nAp sin  
c
Case-II: Let the photons are completely reflected by surface

psin Photon
F1
Photon F1
 p pcos pcos
FBD of surface FBD of photon
Photon psin
Just before Absorption At the time of Absorption
Just after Absorption
F1 = Change of component of momentum of photons perpendicular to surface per unit time
2IA cos2  F 2Icos2 
 F1  2nAp cos    Radiant pressure due to reflection  pr  1 
c A c
Let r be the reflection co-efficient of surface, so
Radiant pressure  r pr  1  r   pa
Note: If intensity and cos are constant, concept of projected area is useful.

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