Acceleration of a circulatory particle

In summary, when a particle moves close to the speed of light around a circular path, its acceleration in its own reference frame is called proper acceleration and corresponds to the G-force experienced by the particle. Equation 30.16 in a book states that the proper acceleration can be calculated using the particle's relativistic gamma-factor and its coordinate acceleration in the inertial frame where it is moving. Assuming special relativity, the proper acceleration can be calculated as \alpha = \frac{u^2}{r * (1 - u^2/c^2)}, where u is the tangential velocity and r is the radius of the circle. However, in the curved spacetime of general relativity, a particle can be in a circular orbit and
  • #1
ehasan
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a particle moves close to the speed of light, say u, around a circular path. what is acceleration according to particle's own reference frame?
 
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  • #2
The acceleration in the particle's own instantaneous inertial rest frame (also called the 'comoving frame') is called the "proper acceleration", it also corresponds to the G-force that would be experienced by the particle (the reading on an accelerometer moving along with the particle). If I'm reading it correctly, equation 30.16 in this book says that if a particle is moving in a circle in some inertial frame, and its coordinate acceleration in that frame is [tex]a[/tex] while its relativistic gamma-factor is [tex]\gamma_u = \frac{1}{\sqrt{1 - u^2/c^2}}[/tex], then its proper acceleration [tex]\alpha[/tex] would be given by:

[tex]\alpha = \gamma_u^2 * a[/tex]

Someone correct me if I'm misunderstanding the meaning of that equation. But assuming that's correct, then the coordinate acceleration [tex]a[/tex] in the inertial frame where the particle is moving in a circle of radius r with tangential velocity u would just the standard centripetal acceleration, [tex]a = \frac{u^2}{r}[/tex], so putting that together with the above, the proper acceleration would be [tex]\alpha = \frac{u^2}{r * (1 - u^2/c^2)}[/tex]

Of course this assumes we are talking about special relativity where some nongravitational force is causing the particle to move in a circle, in the curved spacetime of general relativity a particle can be moving in a circular orbit and experiencing no G-forces because it's in free fall (see the equivalence principle).
 
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  • #3
thnaks
 

FAQ: Acceleration of a circulatory particle

What is acceleration of a circulatory particle?

Acceleration of a circulatory particle refers to the rate at which the velocity of a particle changes over time as it moves in a circular or curved path.

How is acceleration of a circulatory particle calculated?

The acceleration of a circulatory particle can be calculated using the equation a = v^2/r, where a is the acceleration, v is the velocity of the particle, and r is the radius of the circular path.

What factors affect the acceleration of a circulatory particle?

The acceleration of a circulatory particle is affected by the velocity of the particle, the radius of the circular path, and the magnitude and direction of the force acting on the particle.

How does acceleration of a circulatory particle differ from linear acceleration?

Acceleration of a circulatory particle is a type of centripetal acceleration, which refers to the acceleration towards the center of a circular or curved path. Linear acceleration, on the other hand, refers to acceleration in a straight line.

What are some real-world applications of acceleration of a circulatory particle?

Acceleration of a circulatory particle is an important concept in physics and has many practical applications, such as in the design of roller coasters and other amusement park rides, the motion of planets and satellites, and the flow of blood in the circulatory system.

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