Need help calculating the size of the Stromgren sphere

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In summary, the conversation discusses the concept of a Stromgren sphere, which is the region surrounding a star where the gas is ionized by the star's photons. The question involves determining the number of protons and electrons in a fully ionized sphere of gas and how to use an integral to calculate the number density of electrons. The conversation also mentions the technique of radiative equilibrium and how to calculate it.
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Homework Statement



A stromgren sphere is the sphere surrounding a star where the photons from the star can ionize the gas. So the radius of the sphere is the extent from the star in which the gas is ionized. For a fully ionized (idealized, for this question) sphere of gas, the number of protons would equal the number of electrons in the sphere.

(Please look at the attached image to see the full question, it has a large equation that would be very difficult to type out)

Homework Equations


The Attempt at a Solution



The equation includes nenp, and these two quantities should be equal, so can I just rewrite it as ne2? I figure I will do an integral to find the number of electrons in time, but how can I apply that to the number density? I am assuming that ne and np stand for number of electrons and protons, so how can I calculate that to work out to 10^3/cm^3?

Or is my technique crrect at all? Would my integral be definite or indefinite? And since the temperature term doesn't deal with ne or t, can I pull it out and be left with a simple differential equation?

Also, what is radiative equilibrium and how would I calculate it?
 

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bump, anybody please?
 

FAQ: Need help calculating the size of the Stromgren sphere

What is a Stromgren sphere?

A Stromgren sphere is a region of ionized gas that surrounds a hot, massive star. It is created when the intense radiation from the star strips the electrons from the surrounding gas atoms, creating a bubble of ionized gas.

How is the size of a Stromgren sphere calculated?

The size of a Stromgren sphere can be calculated using the formula r = (3Q/4πn2αB)1/3, where r is the radius of the sphere, Q is the number of ionizing photons emitted by the star, n is the number density of the surrounding gas, and αB is the recombination coefficient.

What factors affect the size of a Stromgren sphere?

The size of a Stromgren sphere is primarily affected by the strength of the ionizing radiation from the star and the density of the surrounding gas. Other factors that may influence the size include the temperature and luminosity of the star, as well as the presence of any dust or magnetic fields in the surrounding environment.

How does the size of a Stromgren sphere change over time?

The size of a Stromgren sphere will initially increase as the star continues to emit ionizing radiation and the ionized gas expands. However, as the gas cools and recombines, the size of the sphere will eventually reach a steady state where the rate of ionization by the star is balanced by the rate of recombination.

What is the significance of calculating the size of a Stromgren sphere?

Calculating the size of a Stromgren sphere can provide valuable information about the properties of the hot, massive star at its center, such as its luminosity and ionizing radiation. It can also give insight into the surrounding interstellar medium and its density and composition. This information can help scientists better understand the formation and evolution of stars and galaxies.

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