By Edoardo Amaldi, U. Fano, L. V. Spencer, M. J. Berger
661 tures, resembling happens in stellar atmospheres and in thermonuc1ear strategies, aren't thought of 1. simply because photoelectric absorption predominates thoroughly at low photon energies, and penetration idea is straightforward lower than those stipulations, cognizance is directed during this artic1e to photon energies above ""20 kev. at the excessive power aspect, this artic1e doesn't disguise the cascade bathe techniques that are dealt 2 with in cosmic ray reviews • during this connection it really is recalled that the cascade bathe approach, which comprises electrons and positrons along with X rays, turns into essential above 10 Mev in heavy parts, and above a hundred Mev in mild ones. Theories constructed for the learn of cascade showers in cosmic rays depend upon assumptions concerning the prob skill of interactions with subject that are enough in basic terms at energies of the order of one Gev or extra. lower than this power there's a hole during which penetration phenomena are qualitatively recognized and understood yet haven't but been calculated intimately. a number of certain experimental stories which were made at energies as much as three hundred Mev could be reviewed during this article.
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Additional info for Neutrons and Related Gamma Ray Problems / Neutronen und Verwandte Gammastrahlprobleme
35 scattering, the second term as internat (or resonance) scattering. This distinction is further c1arified by noticing that if the nuc1eus were replaced by a perlectty impenetrable sphere 01 radius R, the condition that the wave function had to fulfill at the nuc1ear surface would be Ul (R) = 0, which implies, according to (21. 3), Il--+ 00. 7) where the potential scattering arises from the small penetrability of the nuc1eus for the incident neutrons and is usually described in terms of an impenetrable sphere, while the internal or resonance scattering depends on the internal structure of the nuc1eus.
20) below] of the Cd absorber used (for a collimated beam): group C covers the thermal region in which the velocity distribution is roughly Maxwellian but it differs from it, because of the capture of neutrons in the moderator, and because of the continuous supply of other neutrons slowed down from higher energies. 4ev where the energy spectrum tends to decrease as 1/E (see Sect. 107). The problem of determining the energies corresponding to the characteristic absorption lines and the widths of the latter, was also attacked and roughly solved by making use of a technique based on the diffusion properties of neutrons in paraffin 1 ,4.
25) it may change sign. 7) reduces to Us = 4n A~sin2 k R ~ 4nR2. 13). 21 ) 2 ;:). In agreement with our previous considerations the reaction cross section depends only on the imaginary part of the scattering length. 21. The distinction between potential scattering and resonance scattering. In this section we shall summarize a procedure of transformation of the scattering cross section of neutrons of angular momentum I, Eq. 11), which allow a c1ear distinction between potential scattering and resonance scattering (Sect.