Snowplow model of a supernova remnant

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Discussion Overview

The discussion revolves around the snowplow model of a supernova remnant, focusing on the dynamics of a spherical shell expanding with a uniform mass density in the ambient medium. Participants engage with mathematical relationships and energy considerations related to the model, exploring the implications of momentum and kinetic energy in the context of supernova remnants.

Discussion Character

  • Technical explanation
  • Mathematical reasoning
  • Homework-related

Main Points Raised

  • One participant presents the snowplow model, outlining the relationship between the mass of the supernova remnant, its expansion speed, and the original mass ejected.
  • The participant proposes a mathematical expression for the momentum conservation in the form (M + M_0)v = M_0*v_0.
  • Another mathematical relationship is suggested regarding the kinetic energies, stating that E/E_0 and v/v_0 are equal to M_0/(M + M_0).
  • A participant introduces themselves and expresses interest in discussing problems related to their astrophysics class.
  • Another participant advises the newcomer to post their problem in the Homework section for better assistance, emphasizing the importance of clearly stating the problem and attempting a solution.

Areas of Agreement / Disagreement

There is no consensus on the specific mathematical derivations or the application of the snowplow model, as the discussion includes both technical exposition and requests for assistance with related problems. The thread remains unresolved regarding the specific solutions to the posed questions.

Contextual Notes

The discussion includes assumptions about the uniformity of mass density and the neglect of thermal pressure effects, which may influence the applicability of the snowplow model in different scenarios.

Who May Find This Useful

Students and enthusiasts in astrophysics, particularly those interested in supernova dynamics and energy conservation principles in expanding shells.

Tuugii
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Suppose a spherical shell identified as a supernova remnant is observed with radius r and
with outward expansion speed v. Assume the mass density of the ambient medium to have
the uniform value "ro_0". then the supernova remnant must have swept up mass M = ((ro_0)*4pi*r^3)/3.
Let the original mass M_0 be ejected at speed v_0. If we ignore communication between
different parts of the shell (via the thermal pressure of the hot interior), and suppose that
each piece of the shell preserves its outward linear momentum as it sweeps up more material initially at rest, we have the snowplow model.

a) Show that the snowplow model implies
(M +M_0)v = M_0*v_0.

b) The original kinetic energy E_0 of the ejected material equals (M_o*(v_0)^2)/2
0/2. The present
kinetic energy E of the shell equals ((M + M_0)v^2)/2. Show that the ratios E/E_0 and v/v_0 are given by:
E/E_0 = v/v_0 = M_0/(M +M_0).
 
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Tuugii! When did you show up, buddy?
 
hey Skip! :)

I am a newbie here. Looking for some discussions on some problems related to my astro class.
 
Welcome, Tuugii! If you will post this problem in the Homework section and follow the format for posting, you will likely get some help pretty soon. You're expected to state the problem clearly, with any variables, and take a shot at dissecting/solving the problem so that the homework helpers can figure out where your problem-solving is breaking down.

If you could come to Maine, you wouldn't be missing Mongolia this winter!
mountains.jpg
 
wow that picture looks awesome!

I'll visit your place at some point of this 4 years! :)

Tuugii
 

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