Encyclopedia of Physical Science and Technology, Volume 2Academic Press, 1992 - Physical sciences |
From inside the book
Results 1-3 of 86
Page 11
... result on Banach spaces is worth stating : Theorem 20. Let 1 < p < . Then C ( , ) is proximinal in B ( l ) . However , C ( X ) is not prox- iminal in B ( X ) for X C [ 0 , 1 ] or X = L , [ 0 , 1 ] , 1 < p < ∞ , p 2 . = Nevertheless ...
... result on Banach spaces is worth stating : Theorem 20. Let 1 < p < . Then C ( , ) is proximinal in B ( l ) . However , C ( X ) is not prox- iminal in B ( X ) for X C [ 0 , 1 ] or X = L , [ 0 , 1 ] , 1 < p < ∞ , p 2 . = Nevertheless ...
Page 12
... results of the subject . We first limit ourselves to approximation by polynomials and splines in one variable . For polynomial approximation in the uniform ( or su- premum ) norm , the following result is known : Theorem 28. Let k be ...
... results of the subject . We first limit ourselves to approximation by polynomials and splines in one variable . For polynomial approximation in the uniform ( or su- premum ) norm , the following result is known : Theorem 28. Let k be ...
Page 320
... result for σ ( x ) is identical to the classical result . When more than one im- pact parameter contributes at a given scattering angle , σ ( x ) is oscillatory . For rainbow scatter- ing , which we discussed earlier , a schematic dia ...
... result for σ ( x ) is identical to the classical result . When more than one im- pact parameter contributes at a given scattering angle , σ ( x ) is oscillatory . For rainbow scatter- ing , which we discussed earlier , a schematic dia ...
Contents
Guide to Using the Encyclopedia ix Atomic Physics | 339 |
Approximations and Expansions 1 Atomic Spectrometry | 357 |
Archaeological Geology 31 Atomic Spectroscopy | 381 |
Copyright | |
17 other sections not shown
Other editions - View all
Common terms and phrases
absorption acid aldoses angular momentum approximation asbestos atmosphere atoms auroral BASIC battery black hole Boolean algebra carbon fibers catalyst cell chemical chrysotile clouds collision complex components concentration convection cross section curve density developed disaccharide disk distribution dust electron elements emission emitted energy engine equations example expert system flux function galaxies heat hydrogen hydroxyl groups infrared input interaction interstellar interstellar medium ionization ions mass material measurements mechanism ment metal molecular molecules monosaccharides neutron stars nucleophile observed oligosaccharides operator orbital oxidation oxygen parameter particles photons plume problem radiation reaction reactor region result saccharide solar solution space spectral spectroscopy spectrum speed spline stable stars stellar structure surface techniques telescope temperature Theorem thermal tion tive turbulence ture typical variable velocity vertical wave wavelength weight white dwarf wind