Hi,
My textbooks says that "Josef Stefan investigated the increasing brightness of a black body as it is heated and discovered that the total intensity of radiation emitted over all wavelenghts increases as the fourth power of the aboslute temperature"
MY question is this: Is the "total...
Hi there. I have a couple of questions regarding the derivation of the Boltzmann equation in Dodelson for photons when given scalar overdensity perturbations to the FRW metric.
To start with, let ##\Theta(\vec{x})## denote the temperature perturbations to the Bose-Einstein distribution of the...
I'm studying by Statistical Mechanics (Huang, page 180) but can't understand many things there, can anyone provide a good bibliography to study this? I don't understand what's an occupation number of a given momentum: if it's the number of particles with that given momentum, why can it only be 0...
I am little bit confused about derivation for Boltzmann equation for electron
look at this link http://relativity.livingreviews.org/Articles/lrr-2008-10/articlesu25.html
which is final boltazmann equation ?
Homework Statement
I have to find the Boltzmann ditribution of a 1 dimensional ideal gas.
The answer is given as:
\frac{dn}{n}=\sqrt{\frac{m}{2piKT}}e^{(\frac{-mc^2}{2KT})}
For the second part I have to find the mean kinetic energy.
2. Homework Equations / Attempt
For part 1...
I don't know how to integrate the Maxwell-Boltzmann distribution without approximation or help from Maple.
Given the Maxwell-Boltzmann distribution:
f(v) = 4\pi\left[\frac{m}{2\pi kT}\right]^{3/2}v^2\textrm{exp}\left[\frac{-mv^2}{2kT}\right]
Observe the appearance of the Boltzmann factor...
I don't know how to integrate the Maxwell-Boltzmann distribution without approximation or help from Maple.
Given the Maxwell-Boltzmann distribution:
f(v) = 4*pi*[m/(2*pi*k*T)]^(3/2)*v^2*exp[(-m*v^2)/(2*k*T)]
Observe the appearance of the Boltzmann factor exp[(-m*v^2)/(2*k*T)] with E =...
Below is part of derivation of the Boltzmann equation in an electric and magnetic field.
I don't understand how to arrive at the bottom equation though. It is known that the dependence of the original distribution function is the given. My idea is to use chain rule but I don't see how to get a...
A system has two non-degenerate energy levels E1 and E2, where E2>E1>0. The system is at tempreture T. The Average energy of the system is = E1+E2e^(-B*deltaE) / 1+e^(-B*deltaE) where deltaE= E2 -E1 and B=1/kT (k=Boltzmann constant). show that for very low temperatures kT<<deltaE, average...
A certain particle is interacting with a reservoir at 500 k and can be in any four possible states. The ground state has energy 3.1 eV and three excited states all have the same energy. what is the probability that the particle is in ground state? what is the probability that the particle is in...
This article insinuates that the physics community had forgotten Gibbs entropy long ago and has used Boltzmann entropy since. Isn't this nonsense? For me it was always clear that Boltzmann entropy is problematic...
Does anyone know if Max Planck knew about the Boltzmann distribution before he published his results in 1900? Also, when Planck introduced h, did he also give the value?
Suppose a set X describes the possible states of some system, and suppose a function x\mapsto E(x) tells the energy level of each state. At temperature T the Boltzmann-measure, which will be the probability measure describing the state of the system, is obtained by formula
dp(x) =...
Can anybody point me to a rough calculation of the probability of a disembodied brain appearing from a random fluctuation vs the probability of a brain evolving in a vary large random fluctuation?
I'm an eternalist. I find it easier to accept the ridiculous idea that the universe was always...
Homework Statement
You will recall from our discussion of the Franck-Hertz experiment that the energy difference between the first excited state of mercury and the ground state is 4.86 eV. If a sample of mercury vaporized in a flame contains 1.06×1020 atoms in thermal equilibrium at 1563 K...
I'm puzzled by the appearance in the literature of 2 conflicting forms:
P(E)=√(E)*exp(-E), which I understand as derived from the Maxwell distribution for speed.
It is a chi -square distribution with 3 degrees of freedom.
P(E)=exp(-E), which seems wrong to me.
But it is not simply a...
Homework Statement
A system in thermal equilibrium at temperature T consists of N particles that have two
energy states separated by an energy Δε.
If the number of particles in the two states is N1 and N2, show that:
N{1} = N(\frac{1}{1+exp(-Δε/k{B}T})) and N{2} =...
Homework Statement
Solve the Boltzmann equation for a homogeneous plasma with not external forces present when the collision term is
\frac{\partial f(v,t)}{\partial t} = -\nu (f(v,t) - f_0(v)),
where \nu and f_0 are constants.
Homework Equations
Boltzmann equation
\frac{\partial...
According the the kinetic theory of gases, molecules moving along the x direction are given by Σx= (1/2) mv^2, where m = mass and vx is the velocity in the x direction
The distribution of particles over velocities is given by the Boltzmann law p(x)=e^[(-mv^2)/ekT]
where velocities range from...
Homework Statement
Hi.
I have a course where I am supposed to show how to get to the Boltzmann equation from a nonequilibrium distrubution function.
At the moment I'm kinda lost to how this is done, so hopefully a hint or two would be of some help :)Homework Equations
The nonequilibrium...
At 293K, helium atoms have a root mean square speed of about 1.35 km/s, whereas escape velocity at the Earth's surface is about 11km/s. Explain why is it nevertheless possible for helium atoms to escape from the Earth into space.
Is it because near the top of the atmosphere the temperature...
Homework Statement
Okay i want to ask 2 questions.
Question 1
Hyperstoichiometric compound Al3O has a vibrational energy spacing of 3.08x 10^-21J
how many molecules are present in the ground state at 300k and 3000K
Question 2
Calirimetric data for protein unfolding yielded following...
Hi PFers. I am interested in Maxwell Boltzmann Distribution. I have searched in Internet for the derivation but I am not satified with them. Can somebody show me the way to derivate it? Thanks.
ψ(v)=(m/2*pi*kT)^(3/2) e^(-mv^2/2kT)
From theory, we know that Boltzmann entropy for a given distribution, defined through a set of occupancy numbers {ni}, of the macrostate M, is given by:
S=k log(Ω{ni})
where omega is the number of microstates for the previously given set of occupancy number, {ni} . Assuming that the system...
I was reading about the thermodynamics of the free-electron gas last night, and my mind veered to fundamental concepts of statistical mechanics. I was able to reorganize my knowledge in a way that made everything clearer. In it, energy does not play a role more privileged than any other...
Hello!
I have two questions for knowledge.
Q) Explain under what conditions Maxwell Boltzmann and Fermi Dirac statistics are applied on free electrons.
Q) Explain each parameter of Boltzmann Transport's equation.
Thank you in advance. :-)
Homework Statement
The three quantities Vmost probable, Vaverage, and Vrms, are not the same for the Maxwell speed distribution in 3D. If you restrict the gas to only be one dimensional, are these three quantities equal to each other? Justify your answer with a short explanation.
Homework...
Hello,
Please could someone explain to me about Boltzmann distribution and Fourier transformation? or point me in the direction of some really really easy-to-understand guide?
I need to understand it for biology - to understand NMR and mass spectrometry.
Thanks.
Im recently studying Boltzmann Constant for Landauer's principle.
I wondered is there a volume for that? What's the units they use(cm or m) when we derive the Boltzmann constant?
I've been looking through the internet but I found nothing. Any Help? Thanks
Hey Guys,
so I had a longish discussion with colleagues and on reddit about thermal equilibrium and the sun and how you cannot heat up anything above the surface temperature of the sun using clever mirrors and stuff.
However, somebody came up with Napkin calculations of the Stefan Boltzmann...
Dear All
I have a question about the validity of Maxwell Boltzmann velocity distribution in the case of nanoscale systems.
When you consider a nanoscale system such as flow of water molecules (less than 100 molecules) through a carbon nanotube or graphene sheet, is it possible to expect a...
In Reif's book Fundamentals of Statistical and Thermal Physics, he labels two formulas as the Stefan-Boltzmann Law. They are both involve T^4 but the constant is different. In one, on page 376, the law is given as (pi2/15)*(kT)4/(c*hbar)3.
The other, on page 388, is...
Hi, I see that Boltzmann constant comes in different forms like: k=8.62*10-5 eV/K and also k=1.38*10-23J/K.
Which one should I use in , say formula for intrinsic carrier concentration ni = sqrt(Nc*Nv)*e-Eg(T)/2kT ?
Consider a resevoir of N atoms in contact with a single atom. Obviously, if the atom is in a high energy state then the multiplicity left for the resevoir is significantly lower. So this is in agreement with the fact that looking at the single atom, the probability for the ground state is very...
Why is the Boltzmann distribution for a collection of atoms independent of their total energy? (it only depends on their temperature)
One would assume that if the energy is high there'd be a greater tendency to be in excited states or am I wrong?
My classmate has already asked about this I think, but since I can't find the post I'll ask again..
Take a single atom with degenerate energy levels E1, E2 etc. We place the atom in a resevoir and want to find the probability of probability for finding the atom in the different energy states...
Homework Statement
A sealed container of volume 0.15 m^3 holds a sample of 5 × 10^1000 atoms of neon gas in equilibrium. The distribution of speeds of the neon atoms shows a peak at 2000 m s^−1.
(i) Calculate the temperature and pressure of the neon gas. (6 marks)
(ii) What is the...
Homework Statement
Use the Boltzmann distribution function to calculate the temperature at which 1.00% of a population of photons will have energy greater than 1.00 eV. The energy required to excite an atom is on the order of 1 eV.
The Attempt at a Solution
I attached my attempt but...
What is the Boltzmann distribution look like if we have a mix of two gasses with very different molecular weights? Say hydrogen at 2 amu and xenon at 132 amu. Do they have equal average momentum and hence the hydrogen has an average velocity 66 times the velocity of the xenon and an energy...
Hello everyone!
I have been on this website for quite a while, and found some interesting answers to many questions, and I decided to create an account to seek you help with a particular issue I encountered in my assignment.
Please have a read, and thank you for any input!
Homework...
Hello,
I'm working of the Boltzmann equation to simulate a partially ionized plasma, but I'm having troubles to solve the collision term. I'm using a splitting technique for the advection in the phase-space, but I'm quite stuck in the collision term. Any recommendations?
hi everyone,
consider two different masses of ideal gases with different molar masses, we're putting them in a uniform gravitational field and wait until they come to their equilibrium states. how would the density distribution change with height in this case?
( i came out with this question...
Why I can't calculate the same answer as the solution below? I use the value as what the below solution showed.
Q:
Where Nj is the number of atoms in excited state, No is the number of atoms in the
ground state, Pj and Po are constants determined by the number of states having equal
energy...
Homework Statement
The relative population of two atomic population states in equilibrium is given by Boltzmann Distribution:
n1/n0 (proportional to) e^(-ε/(κT)) , where ε is the energy difference between the two states, T is the temperature and κ is the Boltzmann constant = (1.38 x...
With an extensive system, I mean a system where energy is an extensive variable. But no need to state it so generally, since I have a specific system in mind which will make sure we don't get into a battle of semantics: if you double the size of a gravitational system, the energy is not...
In the Boltzmann equation,
{\bf{L}}\left[ f \right] = {\bf{C}}\left[ f \right], the right which is the collision term and in general it is{\bf{C}}[f]=\sum\limits_{p,p_1} {|Amplitiude|^2}{f(p)}. and explicitly, the collision term for decaying process is
\begin{eqnarray}
{\bf{C}}\left[ f...
For N(E)=Aexp(-E/kT), I know that N(E) is the no. of particles with a certain energy E,
but why does integrating N(E) from 0 to infinity equal to 1? Although I realize that it means that there is 100% probability to find a particle in this range, I want to know why summing up all no. of...