Escape velocity ratio of stars after mass transfer
Two spherical stars and have densities and , respectively. and have the same radius, and their masses and are related by . Due to an interaction process, star loses some of its mass, so that its radius is halved, while its spherical shape is retained, and its density remains . The entire mass lost by is deposited as a thick spherical shell on with the density of the shell being . If and are the escape velocities from and after the interaction process, the ratio . The value of is ____.
Topics & Concepts
Step-by-Step Solution
To find the value of , we analyze the parameters of stars and before and after the interaction process.
1. Initial Parameters of Stars and
Let be the initial radius of both spherical stars and .
- The initial mass of star is , given by:
- The initial mass of star is .
2. Parameters of Star After Mass Transfer
After the interaction:
- The radius of star becomes .
- The density remains .
The new mass of star , , is:
The mass lost by star is:
3. Parameters of Star After Mass Transfer
The mass lost by , , is deposited as a thick spherical shell on with density .
- Inner radius of the shell =
- Let be the outer radius of star with the shell.
The volume of the shell is:
Since the mass of the shell is :
Canceling common terms:
The total mass of star after the interaction is:
4. Ratio of Escape Velocities
The escape velocity from a spherical body of mass and radius is given by:
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Escape velocity from ():
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Escape velocity from ():
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Ratio :
5. Determination of
Comparing the derived ratio with the given expression:
Equating the numerators inside the square root: