PHZ3400 Midterm Two Solution: Difference between revisions

From PhyWiki
Jump to navigation Jump to search
(Removing all content from page)
 
(124 intermediate revisions by 8 users not shown)
Line 1: Line 1:
==PHZ 3400 – Midterm Two Exam (with solutions) – April 10, 2009==


===Problem 1===
'' Explain the concept of the "Thermodynamic Limit", and present the corresponding domain wall argument (derivation of a formula) to estimate the relaxation time as a function of system size, at T < Tc.''
The partition function which applies in this case is 
<math>Z = \sum_{n}^{\infty}\varepsilon^{-\beta E_n}</math>  where n = the number of particles. 
However, symmetry breaking, including phase transitions, cannot occur for any finite system[1].  Thus systems must be sufficiently large, <math> n\rightarrow \infty</math>, in order to reach the thermodynamic limit and for spontaneous symmetry breaking to occur. 
Suppose we start in a system where all of the spins are up and we would like to make them spin down.  This can be done by applying a domain wall to the system.
[[Image:DomainWall.jpeg|left|thumb|300px|This illustrates the most energetically favorable configuration of the system.  The green line represents the Domain Wall.]]
 
[1]  [http://prola.aps.org/abstract/PR/v87/i3/p404_1
C. N. Yang and T. D. Lee, ''Statistical Theory of Equations of State and Phase Transitions. I. Theory of Condensation'' Phys. Rev. 87, 404 - 409 (1952)]
===Problem 2===
''Sketch the magnetization of a ferromagnet as a function of temperature T, for (A) Zero external magnetic field and (B) Finite external magnetic field.  How is the behavior around the Curie Temperature (Tc) affected by the field?''
(A) For zero external magnetic field, the magnetization of a ferromagnet as a function of temperature T should go through the Curie Temperature (Tc).
===Problem 3===
===Problem 4===
Consider a neutron of radius R = 10km, and mass M = 3x10^30 kg (approximately 1.5 solar masses). Given that the mass of a single neutron is m=1.7*10^-27 kg, that h-bar = 1x10^-34 m^2 kg/s, and that neutrons obey Fermi-Dirac Statistics, calculate:
a. The number density n=N/V of this star.
b. Derive in detail the relation between Fermi energy and the number density.

Latest revision as of 20:43, 17 March 2011

Retrieved from "http://wiki.physics.fsu.edu/index.php?title=PHZ3400_Midterm_Two_Solution&oldid=11357"