Relativistic Doppler Shift and a Star breaking up

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SUMMARY

The discussion centers on calculating the velocities and angles of two remnants from a star that breaks apart, emitting light at frequencies of 7.135 x 1014 Hz and 4.282 x 1014 Hz, while the original star emitted light at 6.690 x 1014 Hz. The participants utilized the relativistic Doppler shift equations, specifically v' = v γ [1 - β cos θ] and v' = v √((1 + β)/(1 - β)), to derive the speed of the remnants as 0.235c and β as 0.47. They encountered challenges in determining the angles between the remnants and the line of sight, leading to discussions about the relationship between speed and angle, ultimately concluding that the data provided may contain inconsistencies that prevent a valid solution.

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  • #61
Lets see where I went wrong:

\beta( \frac{7.135*10^{14}}{(6.690*10^{14})\gamma} - 1)) = -\beta(\frac{ 4.282*10^{14}}{(6.690*10^{14})\gamma} - 1)

\gamma = \sqrt{\frac{1}{1 - \beta^2}}

So:

\beta( \frac{7.135*10^{14}}{(6.690*10^{14})(\sqrt{\frac{1}{1 - \beta^2}})} - 1)) = -\beta(\frac{ 4.282*10^{14}}{(6.690*10^{14})(\sqrt{\frac{1}{1 - \beta^2}})} - 1)

Also, can't Gamma be expressed as:

\gamma = \frac{1}{\sqrt{1 - \beta^2}}

??

TFM
 
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  • #62
Yeah gamma can have that form too, I would have written like that but I couldn't get the latex to do it for me.
 
  • #63
So, first cancel out the exp. and the beta's:

\frac{7.135}{(6.690)\gamma} - 1 = -\frac{ 4.282}{(6.690)\gamma} + 1

Reinsert gamma:

\frac{7.135}{(6.690)(\frac{1}{\sqrt{1 - \beta^2}} )} - 1 = -\frac{ 4.282}{(6.690)({\frac{1}{\sqrt{1 - \beta^2}}} )} + 1

Multiiply out:

\frac{7.135}{(\frac{6.690}{\sqrt{1 - \beta^2}} )} - 1 = -\frac{ 4.282}{({\frac{6.690}{\sqrt{1 - \beta^2}}} )} + 1

Move over the 1:

\frac{7.135}{(\frac{6.690}{\sqrt{1 - \beta^2}} )} = -\frac{ 4.282}{({\frac{6.690}{\sqrt{1 - \beta^2}}} )} + 2

\frac{7.135}{(\frac{6.690}{\sqrt{1 - \beta^2}} )} + \frac{ 4.282}{({\frac{6.690}{\sqrt{1 - \beta^2}}} )} = 2

Does this look okay?

TFM
 
  • #64
This can go to:

\frac{7.135(\sqrt{1 - \beta^2})}{6.690} + \frac{ 4.282( \sqrt{1 - \beta^2})}{6.690}} = 2

get rid of denominator:

7.135(\sqrt{1 - \beta^2}) + 4.282( \sqrt{1 - \beta^2}) = 2*6.690

This can go to:

11.417 (\sqrt{1 - \beta^2}) = 13.38

and:

\sqrt{1 - \beta^2} = 13.38/11.417

\sqrt{1 - \beta^2} = 1.172

so square out the root:

1 - \beta^2 = 1.373

and:

1 - 1.373 = \beta^2

Is the data still wrong, or have I done something wrong, because I now get beta squared as
-0.373

??

TFM
 
  • #65
Your math looks fine, your answer is the same as my own. It's as Doc Al said, the data is wrong. Slightly annoying because I think it makes it impossible to find the angle, as requested in the second part, though I may be wrong.
 
  • #66
Yes, the data is wrong. When I checked it earlier, I used my own calculations (with correct expression for \gamma).
 
  • #67
Hey all,

Is there a possibility that the answer is imaginary because one velocity is the negative of the other?

Vuldoraq
 
  • #68
I finally have the answer sheet for the question:

Quoted from Sheet:

Since the fragments have equal masses, they must have equal velocities. Using the general Doppler shift relation, we find that for one of the fragments

\frac{v prime}{v} = \frac{6.690*10^{-14}}{7.135*10{-14}} = 0.9376 = \gamma - \beta \gamma cos \theta

whereas for the other

\frac{v prime}{v} = \frac{6.690*10^{-14}}{4.282*10{-14}} = 1.562 = \gamma + \beta \gamma cos \theta

Adding these, we obtain 2γ =2.5 so γ =1.25=5/4 and so

\beta^2 = 1 - \frac{1}{\gamma^2} = 1 - \frac{16}{25} = \frac{9}{25}

and therefore

\beta = \frac{3}{5} = 0.6

which gives a velocity of 0.6 × 3×108 = 1.83 × 108 m/s.
Substituting back into the first equation of this part, we find

0.936 = 1.25(1 - 0.6cos \theta)

0.75 = 1 - 0.6cos \theta

cos \theta = \frac{0.25}{0.6}0.4167

and so the angle is θ = 65.4°.

End Sheet Quote

TFM
 
  • #69
Yeah, I really messed this one up big time. I had reversed the primed and unprimed frequencies (mixing up source and observer). D'oh!

My apologies. :redface:
 

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