By Gerd Baumann

ISBN-10: 0387219331

ISBN-13: 9780387219332

This moment variation of Baumann's Mathematica in Theoretical Physics indicates readers the way to resolve actual difficulties and care for their underlying theoretical innovations whereas utilizing Mathematica to derive numeric and symbolic strategies. each one instance and calculation will be evaluated via the reader, and the reader can swap the instance calculations and undertake the given code to similar or comparable difficulties. the second one version has been thoroughly revised and multiplied into volumes: the 1st quantity covers classical mechanics and nonlinear dynamics. either subject matters are the foundation of a standard mechanics path. the second one quantity covers electrodynamics, quantum mechanics, relativity, and fractals and fractional calculus.

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**Additional info for Mathematica for Theoretical Physics: Electrodynamics, Quantum Mechanics, General Relativity and Fractals**

**Sample text**

The domain G is free of charges. The domain G is free of any charges and the potential FHr, jL is regular and finite for r Ø 0. To solve the problem efficiently, we choose coordinates which reflect the geometry of our problem. In this case, they are plane cylindrical coordinates. Since G is free of any charges, Laplace's equation in plane cylindrical coordinates takes the form 2 F 1 F ÅÅÅÅ1r ÅÅÅÅ ÅÅ Ir ÅÅÅÅ ÅÅÅ M + ÅÅÅÅ Å ÅÅÅÅÅÅÅÅÅ = 0. 32) When deriving the solution, we assume that the coordinates are separated.

3 One-Dimensional Potential extension. Beyond the maximum extension, the potential vanishes. 6. 6. The potential well of depth V . , T < V0 ). The total energy E of the system is E = T - V0 < 0. 6. In classical mechanics, the particle cannot be found in these regions. Contrary to classical mechanics, however, quantum mechanics allows the existence of particles in regions where they are classically forbidden. 12) where k2 = -2 m E ê Ñ2 > 0 is a positive constant containing the total energy. Primes denote differentiation with respect to the spatial coordinate.

The handling of Eqs. 89). Note that Eqs. 4 Penning Trap to the secular equations of the Paul trap. Both systems of equations are derived from a Lagrangian given by 1 1 n2 1 Hr'2 + z '2 L - J ÅÅÅÅ Hr2 + 2 l2 z 2 L + ÅÅÅÅÅÅÅÅ ÅÅÅÅÅÅÅÅÅÅÅ + ÅÅÅÅ ÅÅÅÅÅ N. 3 = ÅÅÅÅ è!!!!!!!!!!!!!!! 5]. If we wish to choose parameters, we need to integrate the equations numerically. Mathematica supports numerical integrations and we use this property to find numerical solutions for Eqs. 91). 3, contains the necessary function PenningI[] to integrate Eqs.

### Mathematica for Theoretical Physics: Electrodynamics, Quantum Mechanics, General Relativity and Fractals by Gerd Baumann

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