Snowplow model of a supernova remnant

In summary: This model implies that the present kinetic energy and velocity of the shell are proportional to the original values, with the ratio being equal to the original mass divided by the total mass of the shell and the original mass. The conversation also includes a suggestion to post the problem in the Homework section for assistance.
  • #1
Tuugii
15
0
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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  • #2
Tuugii! When did you show up, buddy?
 
  • #3
hey Skip! :)

I am a newbie here. Looking for some discussions on some problems related to my astro class.
 
  • #4
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
 
  • #5
wow that picture looks awesome!

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

Tuugii
 

1. What is the Snowplow model of a supernova remnant?

The Snowplow model is a theoretical model that explains the evolution of a supernova remnant, which is the expanding shell of debris from a supernova explosion. The model suggests that as the remnant expands, it sweeps up and compresses the surrounding interstellar medium, creating a shock wave that heats up the gas and causes it to emit X-rays.

2. How does the Snowplow model explain the X-ray emission in a supernova remnant?

The Snowplow model proposes that the X-ray emission in a supernova remnant is caused by the heated gas in the shock wave. As the shock wave travels through the interstellar medium, it compresses and heats up the gas, causing it to emit X-rays. This X-ray emission can be observed and studied to understand the properties of the supernova remnant.

3. What are the key assumptions of the Snowplow model?

The Snowplow model is based on several key assumptions, including the idea that the supernova explosion is spherically symmetric and that the interstellar medium is uniform and has a constant density. The model also assumes that the remnant expands at a constant velocity and that there is no energy lost or gained during the expansion.

4. How does the Snowplow model contribute to our understanding of supernova remnants?

The Snowplow model provides a framework for understanding the evolution of supernova remnants and the physical processes that occur within them. It helps scientists to interpret observations of X-ray emission and other properties of supernova remnants, and to make predictions about their future evolution.

5. Are there any limitations or criticisms of the Snowplow model?

Some scientists have criticized the Snowplow model for its simplifying assumptions and its inability to accurately predict the properties of specific supernova remnants. Additionally, the model does not account for the effects of magnetic fields or other complex physical processes that may occur in a supernova remnant. However, it remains a useful tool for understanding the general behavior of these objects.

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