What is the Mass-Radius Relation for a White Dwarf with 0.6 Solar Masses?

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Homework Help Overview

The discussion revolves around calculating the mass-radius relation for a white dwarf with a mass of 0.6 solar masses. The original poster attempts to compute a numerical constant for an electron gas and determine the radius of the white dwarf based on given parameters and equations.

Discussion Character

  • Exploratory, Assumption checking, Mathematical reasoning

Approaches and Questions Raised

  • Participants discuss the calculation of the constant C and its implications for the radius of the white dwarf. Questions arise regarding the use of Avogadro's number and the units of density, prompting a review of unit conversions between grams, cubic centimeters, and cubic meters.

Discussion Status

Participants are actively engaging in unit analysis to clarify calculations. Some have noted that adjusting the units leads to a more reasonable radius for the white dwarf, indicating a productive direction in the discussion.

Contextual Notes

There is an ongoing examination of the assumptions regarding the density and the constants used in the calculations, particularly the interpretation of N0 and its units. The original poster expresses uncertainty about the values used, which may affect the outcome.

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Homework Statement



Compute the numerical constant C for an electron gas (take Z = 6 and A = 12) and determine the radius of a white dwarf whose mass is 0.6 solar masses.

h\ =\ 6.62606876(52)\ \times\ 10^{-34}\ Jh\ =\ 6.62606876(52)\ \times\ 10^{-34}\ J\ s\ s

m_{e}\ =\ 9.10938188(72)\ \times\ 10^{-31}\ kg

G\ =\ 6.673(10)\ \times\ 10^{-11}G\ =\ 6.673(10)\ \times\ 10^{-11}\ m^{3} kg^{-1} s^{-2}\ m^{3} kg^{-1} s^{-2}

Mass of the white dwarf: \ 1.2 \times\ 10^{30}kg

Homework Equations



M = \frac{f}{R^{3}}

f = \frac{π}{3}\left(\frac{15C}{2πG} \right)^{3}

\frac{N}{V} = \frac{ρN_{0}}{2}, since Z/A = 1/2

P=Cρ^{\frac{5}{3}} = \left(\frac{N}{V}\right)^{\frac{5}{3}} \left(\frac{3h^{3}}{8π}\right)^{\frac{2}{3}}\frac{1}{5m}

The Attempt at a Solution



C = \frac{1.064\times10^{-67}}{5m}\left(\frac{N_{0}}{2}\right)^{\frac{5}{3}}

I took N_{0} = 6.02 x 10^{23} so C = 31.57

\frac{15C}{2πG}=\frac{473.53}{4.19\times 10^{-10}}=1.13\times10^{12}

Putting that into f, we get f = 1.511\times10^{36}

Now, 1.2\times10^{30} = \frac{1.511\times10^{36}}{R^{3}}

and finally R = 107.98m, which doesn't make any sense to me. The only place where I think I might have it wrong is the value of N_{0}.
 
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Working with units would help to spot the error.
What is N0? If it is the avogadro constant, why do you get it as factor between a density and another density? Which units do you use for ρ?
 
I hate the textbook and the class notes but, per class notes, I assume ρ is in g/cc, and N/V is in particles per cubic meter.
 
cc? cm3? Then you need an additional factor of 10^6 to convert between m3 and cm3.
 
But then I'd have to divide by 1,000 to go from grams to kilograms... so I'd need an additional factor of 1,000 rather than 10^6.
 
As you can see, it would be useful to work with units everywhere. It is easier to spot (or avoid) those prefactors if you know the units of your parameters.
 
And now it gives a more sensible size (somewhat larger than Earth in volume, yet on the same order of magnitude); I find that the Coulomb pressure wouldn't affect the radius very much.
 

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