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The New Cosmic Onion: Quarks and the Nature of the Universe by Frank Close

By Frank Close

Now not when you consider that Newton's apple has there been a physics phenomenon as deliciously attractive to the loads as Frank Close's Cosmic Onion. generally embraced through scientists and laypersons alike, the e-book fast turned a world bestseller, has been translated into seven languages, and propelled the writer to turn into a well-known renowned technological know-how megastar world wide. a lot has replaced because the unique ebook in 1983, and the hot Cosmic Onion was once broadly revised and up-to-date to mirror our new view of the universe. holding the easiest contents from the former paintings, this new version contains large new fabric explaining the clinical demanding situations at the beginning of this century.

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Z. Phys. 51, 204–212 (1928) 3. : Wave mechanics and radioactive disintegration. Nature 22, 439 (1928) 4. : Physical and mathematical aspects of Gamow States. Phys. Rep. 396, 41–113 (2004) 5. A. ): Handbook of Mathematical Functions. , New York (1983) 6. : R-Matrix theory of nuclear reactions. Rev. Mod. Phys. 30, 257–353 (1958) 7. : Exact and approximate calculation of giant resonances. Nucl. Phys. A 584, 13–34 (1995) 8. : The use of resonant states in Eigenfunction expansions of scattering and reaction amplitudes.

38 Fig. 106). Different symbols correspond to cluster decays in Fig. 6. 111) for cluster emission processes, except a-decay. b Cluster mass number versus the fragmentation potential 2 Binary Emission Processes 0 -2 -4 -6 -8 -10 -12 -14 -16 -18 -20 10 40 35 30 25 20 15 10 5 0 10 (a) 15 20 25 30 35 40 45 50 55 60 20 25 30 35 40 45 50 55 60 (b) 15 Concerning the reduced widths of proton emitters, in Refs. [20, 32] it was pointed out the correlation between the reduced width and the quadrupole deformation.

Hx in Eq. 108 leads to "hx % 1:5 MeV; The above value of the slope Àlog10 e2 =" with the same order of magnitude as in the a-decay case. The relative large scattering of experimental data around the straight line in Fig. 103). Let us mention that a relation expressing the spectroscopic factor (proportional to the integral of the reduced width squared) for cluster emission processes was derived in Ref. [31] C À1Þ=3 ; S ¼ SðA a ð2:112Þ where AC is the mass of the emitted light cluster and Sa * 10-2.

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