Download An Introduction to Macroscopic Quantum Phenomena and Quantum by A. O. Caldeira PDF

By A. O. Caldeira

ISBN-10: 052111375X

ISBN-13: 9780521113755

Reviewing macroscopic quantum phenomena and quantum dissipation, from the phenomenology of magnetism and superconductivity to the presentation of different versions for quantum dissipation, this booklet develops the elemental fabric essential to comprehend the quantum dynamics of macroscopic variables. Macroscopic quantum phenomena are awarded via a number of examples in magnetism and superconductivity, constructed from basic phenomenological ways to every region. Dissipation obviously performs an incredible position in those phenomena, and for that reason semi-empirical types for quantum dissipation are brought and utilized to the learn of some very important quantum mechanical results. The e-book additionally discusses the relevance of macroscopic quantum phenomena to the regulate of meso- or nanoscopic units, rather people with strength purposes in quantum computation or quantum details. it truly is excellent for graduate scholars and researchers.

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Extra info for An Introduction to Macroscopic Quantum Phenomena and Quantum Dissipation

Example text

In other words, we are saying that v R (x, y) is Gaussian distributed and short-range correlated with correlation length l (which means that the delta function arguments are strongly peaked at 0 and smeared out over l). 3 Dynamics of the magnetization VR (y, u) R =0 VR (y1 , u 1 ) VR (y2 , u 2 ) and R 39 = R(u 1 − u 2 )δ(y1 − y2 ). 85) If we assume, for simplicity, that the wall profile ρ(x, y, u) is a Gaussian centered at u(y) with width ζ√ , we have R(u) = v 2R k(u) where k(u) is also a Gaussian but now spread over 2ζ .

8, which results in Fig. 9. As the temperature is lowered it becomes harder for the magnetization to be driven out of the well by thermal fluctuations and it might become frozen at the metastable configuration until the coercivity field is reached. 50). 71) =− ∂t 2I ∂θ 2 where I ≡ μ2 /2γg2 K 2 is the effective moment of inertia associated with the magnetic particle. This can be solved by the standard WKB approximation and provides us with the quantum rate of transition in the absence of dissipation.

This problem is well known and can be found in any textbook of quantum theory (see, for example, Merzbacher (1998)). What we look for is a simultaneous (z) eigenstate of S 2 = ( k Sk )2 and S (z) = k Sk , where k refers to any given spin of the system. The eigenstates of this problem are labeled by |S, M S , where S = N /2, (N − 2)/2, (N − 4)/2, . . , 1/2 or 0 depending on whether N is odd or even, respectively, and M S = S, (S − 1), (S − 2) . . − (S − 1), −S. For very high external magnetic fields,2 the lowest-energy eigenstates of our magnetic particle are approximately |N /2, M S and its ground state is then |N /2, N /2 , which we denote by | ↑ , ↑ , .

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