1954
DOI: 10.1143/ptp.12.481
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Renormalization in the Covariant Treatment of Pion-nucleon Scattering

Abstract: 481The problem of renormalization for pion-nucleon scattering is treated in the Bethe-Salpeter formalism. A method to subtract divergencies, especially, overlapping-divergencies, which appear in the solution of an integral equation, is proposed and it is shown that the Salam's prescriptions for the subtraction of overlapping-divergencies can be achieved in a closed form. Finally, the Green's function for T= 1/2 state is obtained in a form free from all the divergencies. § 1. IntroductionWhen we treat the probl… Show more

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Cited by 12 publications
(23 citation statements)
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“…It should be noted that the system they considered is different from that considered in this article and that their result is controversial. There are numerical analyses that may support or may not support the results of Nakamura, Shibata and Nakao for prolate collapse [13] and for cylindrical collapse [29,30].Due to the non-linear nature of the problem, it is difficult to analytically solve the Einstein equation. Therefore, numerical methods will provide the final tool.…”
mentioning
confidence: 99%
“…It should be noted that the system they considered is different from that considered in this article and that their result is controversial. There are numerical analyses that may support or may not support the results of Nakamura, Shibata and Nakao for prolate collapse [13] and for cylindrical collapse [29,30].Due to the non-linear nature of the problem, it is difficult to analytically solve the Einstein equation. Therefore, numerical methods will provide the final tool.…”
mentioning
confidence: 99%
“…Then a string is trapped and spatial if ε > 1/8, marginal and null if ε = 1/8, and untrapped and temporal if ε < 1/8, cf. Chiba [11]. In particular, unlike the spherically symmetric case [2] there is now a range of positive energy, 0 < ε < 1/8, for which axial singularities are locally naked.…”
Section: Cosmic Stringsmentioning
confidence: 96%
“…One may also say that an axial singularity is trapped (respectively untrapped) if it has a neighbourhood of trapped (respectively untrapped) cylinders, cf. Chiba [11]. If the singularity is smooth (as a boundary in the quotient space) it can alternatively be defined to be trapped, marginal or untrapped as ∇ ♯ r is temporal, null or spatial respectively.…”
Section: Black Holesmentioning
confidence: 99%
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