Computational Physics: Fortran Version by Steven Koonin, Dawn Meridith PDF

By Steven Koonin, Dawn Meridith

ISBN-10: 0201127792

ISBN-13: 9780201127799

ISBN-10: 0201386232

ISBN-13: 9780201386233

Computational Physics is designed to supply direct adventure within the desktop modeling of actual structures. Its scope contains the fundamental numerical concepts had to "do physics" on a working laptop or computer. each one of those is built heuristically within the textual content, due to basic mathematical illustrations. in spite of the fact that, the true price of the publication is within the 8 Examples and initiatives, the place the reader is guided in employing those innovations to giant difficulties in classical, quantum, or statistical mechanics. those difficulties were selected to complement the normal physics curriculum on the complex undergraduate or starting graduate point. The ebook may also be invaluable to physicists, engineers, and chemists attracted to computing device modeling and numerical ideas. even supposing the ordinary and entirely documented courses are written in FORTRAN, an informal familiarity with the other high-level language, equivalent to easy, PASCAL, or C, is enough. The codes in easy and FORTRAN can be found on the net at (Please stick to the hyperlink on the backside of the page). they're on hand in zip structure, that are improved on UNIX, Window, and Mac platforms with the right kind software program. The codes are appropriate to be used (with minor adjustments) on any laptop with a FORTRAN-77 suitable compiler or easy compiler. The FORTRAN images codes can be found besides. besides the fact that, as they have been initially written to run at the VAX, significant variations needs to be made to cause them to run on different machines.

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Additional resources for Computational Physics: Fortran Version

Example text

Reconcile your answrs in Step I with the result8 you obtGn. Calcu1;at;e the diflerentid cross section as a function of @ at these energies. Step 5 E your progrm is working comectly, ycru &odd observe, for ener@w E K t a siqulmity in the deflection function whese O appeaas to apprawh -m at some critical vdue of b, brit,that depends on E. " In this phenomenon, the integrmd in Eq. 6) has a linear, rather than a square root, singularity at the turning poiat, 80 thitt the scattering aggle becomes logiurithrnically iagnite.

7) . The following FORTRAN program integrates forward from s = O to I = 3 using Eq. 6) with the step size input, printing the result and its error zls it goes along. l@. LE. nmbsr of steps to reach. Q Y=Y+H*FUBG(X,Y) DTFF=EXP f -Q. 1. As expected fmm (&G), the errors decrease linearly with smaller h. However, the fractional error (error divided by y) increases with I as more steps me taken in the ilttegratlon asrd y beeernes smajtler. 2 k Error in integrating dy/cbz E d e r ? method ~ Eq. 6) @(l) ~(3) z: -zy with gf 0) Taylor series Eq.

Verify that there are no qualitative differences if you use a different separable potential, say the harmonic one of Eq. 34). 025. For each enera, consider various initid conditions and integrate each trajectory long enough in time (some will require going to t m 1100) to map out the surface-of-section adequateb. For each energy, see if you can find the elliptic fixed points, the tori (and tori of tori) around them, and the chaotic regions of phaee space and observe how the relative proportions of each change with increasing energy.

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Computational Physics: Fortran Version by Steven Koonin, Dawn Meridith

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