Revolution of electron and that of the planets

AakashPandita
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planets do not loose energy when they orbit the sun due to interplay of centripetal and centrifugal force. Then why is this system not able to explain that electrons do not loose energy while orbiting the nucleus?
 
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Hi Aakash! :smile:
AakashPandita said:
planets do not loose energy when they orbit the sun due to interplay of centripetal and centrifugal force. Then why is this system not able to explain that electrons do not loose energy while orbiting the nucleus?

The problem is that an accelerating charge emits electromagnetic radiation (and therefore loses energy).

(this is easy to prove, and has nothing to do with quantum theory).

So a planet with a net charge would lose energy. :wink:
 
AakashPandita said:
planets do not loose energy when they orbit the sun due to interplay of centripetal and centrifugal force. Then why is this system not able to explain that electrons do not loose energy while orbiting the nucleus?
Electrons also do not orbit the nucleus. This is Rutherford's antiquated view of the atom that has since been replaced by the understanding that electrons exist in "clouds" determined by their wavefunctions.
 
thank you
 
AakashPandita said:
planets do not loose energy when they orbit the sun due to interplay of centripetal and centrifugal force. Then why is this system not able to explain that electrons do not loose energy while orbiting the nucleus?

In fact a planet orbiting a star does lose energy, albeit extremely slowly, to gravitational radiation. This is very closely analogous to the way an orbiting charge loses energy to electromagnetic radiation. But gravity is a very weak force, so energy losses due to gravitational radiation are unmeasurably small except in special cases.

In both cases, the point is that while centripetal and centrifugal forces do balance out, there is another force acting on the orbiting body. The radiation it emits "pushes back" on it, so there is a drag force that slows the body down and causes it to spiral inward.

To explain why this doesn't happen to electrons in atoms we need quantum mechanics.
 
AakashPandita said:
planets do not loose energy when they orbit the sun due to interplay of centripetal and centrifugal force.


Not really. According to Newton's first law - "The velocity of a body remains constant unless the body is acted upon by an external force", i.e. in the abscence of such, it remains in motion. Then come the centripetal and centrifugal forces.



Then why is this system not able to explain that electrons do not loose energy while orbiting the nucleus?


Your example is a very bad analogy, but i'd say they don't lose energy because they are not really in motion. Lots of stuff at the micro scale is motion-like, real-like, spinning-like, etc. -like(but not quite so in reality).
 
In GR, frame dragging induces orbital instability.
 
Maui said:
Not really. According to Newton's first law - "The velocity of a body remains constant unless the body is acted upon by an external force", i.e. in the abscence of such, it remains in motion. Then come the centripetal and centrifugal forces.

http://en.wikipedia.org/wiki/Abraham-Lorentz_force
 
Maui said:
Not really. According to Newton's first law - "The velocity of a body remains constant unless the body is acted upon by an external force", i.e. in the abscence of such, it remains in motion.
One problem with that: Newton's laws are not (exactly) correct. They are instead approximately correct in a limited regime velocities that are very, very low compared to the speed of light, distances that are very, very large compared to the Schwarzschild radius.

The_Duck in post #5 was referring to one of the predicted effects of general relativity. Gravitational radiation is immeasurably small in the case of the planets orbits about the Sun. The effect is not so small in the case of two very massive object orbiting very close to one another. It has in fact been observed. The observations eventually led to the discoverers receiving the 1993 Nobel Prize in physics.
 

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