Statistical physics at constant temp

BIn summary, we have a system of 32 spin-½ dipoles with a net magnetic moment of 8mu, where 20 dipoles are aligned with the magnetic field of strength B. Using the Boltzmann distribution, the temperature can be calculated as T=(8muBln(3/5))/kb. The standard deviation in mean energy is 4muB.
  • #1
oddiseas
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Homework Statement



A system of 32 spin-½ dipoles (each of moment μ) is held at a constant temperature in an external magnetic field, where on average, 20 dipoles are aligned with the magnetic field of strength B.
a) What is the temperature, in terms of given parameters?
b) What is the standard deviation in the mean energy, in terms of given parameters?

Homework Equations





The Attempt at a Solution


a) the net magnetic moment is 20mu-12m=8mu
p(spin up)=20/32
p(spin down)=12/32

Now i am a bit cofused in using this information in the boltzman distribution.

(p₂)/(p₁)=e^-(E₂-E₁)/(kT)

The energy for the dipoles is given by E=-muB
The net magnetic moment is 8mu and thus the total energy of the system in this state is E=-8muB.

So is the energy difference in the case simply the total energy of the system which is E=-8muB, or is it E(12)-E(20)
ie:
E(12)=12muB
E(20)=-20muB
Anyway i did the following:

(3/5)=e^-(8muB)/(kT)

Also is there are restriction on what (p₂)/(p₁) is interpreted as?
can i take it to be 12/20 or 20/12 without changing the result?
 
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  • #2
Solving this equation for T yields:T=(8muBln(3/5))/kb) Now to calculate the standard deviation i used the following formula:σ=sqrt((E²)-(E)²)/N where E is the mean energy, E² is the mean energy squared and N is the number of dipoles.Since E=-8muB we get:σ=sqrt((64μ²B²)-(-64μ²B²))/32σ=sqrt(128μ²B²/32)σ=(4μBsqrt(2))/sqrt(2)
 

Related to Statistical physics at constant temp

What is statistical physics at constant temperature?

Statistical physics at constant temperature is a branch of physics that studies the behavior and properties of systems at a fixed temperature. It uses statistical methods to describe the behavior of large numbers of particles and how they interact with each other.

Why is constant temperature important in statistical physics?

Constant temperature is important in statistical physics because it allows for the study of systems without the influence of temperature changes. This allows for a more accurate understanding of the behavior and properties of the system.

What are some examples of systems that can be studied using statistical physics at constant temperature?

Some examples of systems that can be studied using statistical physics at constant temperature include gases, liquids, and solids. Other examples include biological systems, such as proteins and DNA, and complex systems, such as networks and economies.

What are some key principles and laws used in statistical physics at constant temperature?

Some key principles and laws used in statistical physics at constant temperature include the Maxwell-Boltzmann distribution, which describes the probability distribution of particles in a system, and the Boltzmann factor, which relates the energy of a system to its temperature. Other important principles include entropy, thermodynamics, and the laws of probability.

How is statistical physics at constant temperature related to other branches of physics?

Statistical physics at constant temperature is closely related to other branches of physics, such as thermodynamics, quantum mechanics, and classical mechanics. It provides a statistical interpretation of these branches and allows for the prediction and understanding of macroscopic behavior based on microscopic interactions.

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