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Minimal subtraction scheme

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Renormalization scheme in quantum field theory
Renormalization and regularization

In quantum field theory, the minimal subtraction scheme, or MS scheme, is a particular renormalization scheme used to absorb the infinities that arise in perturbative calculations beyond leading order, introduced independently by Gerard 't Hooft and Steven Weinberg in 1973.[1] [2] The MS scheme consists of absorbing only the divergent part of the radiative corrections into the counterterms.

In the similar and more widely used modified minimal subtraction, or MS-bar scheme (MS), one absorbs the divergent part plus a universal constant that always arises along with the divergence in Feynman diagram calculations into the counterterms. When using dimensional regularization, i.e.   d 4 p μ 4 d d d p   , {\displaystyle \ \mathrm {d} ^{4}p\to \mu ^{4-d}\mathrm {d} ^{d}p\ ,} {\displaystyle \ \mathrm {d} ^{4}p\to \mu ^{4-d}\mathrm {d} ^{d}p\ ,} it is implemented by rescaling the renormalization scale:   μ 2 μ 2 e γ E 4   π   , {\displaystyle \ \mu ^{2}\to \mu ^{2}{\frac {e^{\gamma _{\mathrm {E} }}}{4\ \pi }}\ ,} {\displaystyle \ \mu ^{2}\to \mu ^{2}{\frac {e^{\gamma _{\mathrm {E} }}}{4\ \pi }}\ ,} with the Euler–Mascheroni constant,   γ E   . {\displaystyle \ \gamma _{\mathrm {E} }\ .} {\displaystyle \ \gamma _{\mathrm {E} }\ .}

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