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Gross-Neveu-Modell
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Das Gross-Neveu-Modell ist ein Modell aus der Quantenfeldtheorie zur Beschreibung von Dirac-Fermionen unter der Vier-Fermionen-Wechselwirkung in einer Zeitdimension und einer Raumdimension, beschrieben durch eine nichtlineare Dirac-Gleichung. Untersucht wurde das Gross-Neveu-Modell erstmals von David Gross und AndrΓ© Neveu im Jahr 1974.
Contents
β’ Lagrange-Dichte
β’ Siehe auch
β’ Literatur
ββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββ
Lagrange-Dichte
Die Lagrange-Dichte des Gross-Neveu-Modells verallgemeinert dabei die der Dirac-Gleichung durch einen zusΓ€tzlichen Wechselwirkungsterm:
L = Ο Ο Β― Β― j ( i β β / β β m ) Ο Ο j + g 2 2 n ( Ο Ο Β― Β― j Ο Ο j ) 2 . {\displaystyle {\mathcal {L}}={\bar {\psi }}_{j}(\mathrm {i} \partial \!\!\!/\,-m)\psi ^{j}+{\frac {g^{2}}{2n}}\left({\bar {\psi }}_{j}\psi ^{j}\right)^{2}.}
Mit der Euler-Lagrange-Gleichung ergibt sich daraus:
β β L β β Ο Ο Β― Β― j β β β β ΞΌ ΞΌ β β L β β ( β β ΞΌ ΞΌ Ο Ο Β― Β― j ) = ( i β β / β β m ) Ο Ο j + g 2 n ( Ο Ο Β― Β― k Ο Ο k ) Ο Ο j = 0. {\displaystyle {\frac {\partial {\mathcal {L}}}{\partial {\bar {\psi }}_{j}}}-\partial _{\mu }{\frac {\partial {\mathcal {L}}}{\partial (\partial _{\mu }{\bar {\psi }}_{j})}}=(\mathrm {i} \partial \!\!\!/\,-m)\psi _{j}+{\frac {g^{2}}{n}}\left({\bar {\psi }}_{k}\psi ^{k}\right)\psi _{j}=0.}
Es lΓ€sst sich ebenfalls eine verallgemeinerte Lagrange-Dichte fΓΌr das Gross-Neveu-Modell betrachten:
L = Ο Ο Β― Β― j ( i β β / β β m ) Ο Ο j + g 2 2 n ( ( Ο Ο Β― Β― j Ο Ο j ) 2 + ( Ο Ο Β― Β― j Ξ³ Ξ³ 5 Ο Ο j ) 2 ) . {\displaystyle {\mathcal {L}}={\bar {\psi }}_{j}(\mathrm {i} \partial \!\!\!/\,-m)\psi ^{j}+{\frac {g^{2}}{2n}}\left(\left({\bar {\psi }}_{j}\psi ^{j}\right)^{2}+\left({\bar {\psi }}_{j}\gamma _{5}\psi ^{j}\right)^{2}\right).}
FΓΌr diese folgt aus der Euler-Lagrange-Gleichung:
β β L β β Ο Ο Β― Β― j β β β β ΞΌ ΞΌ β β L β β ( β β ΞΌ ΞΌ Ο Ο Β― Β― j ) = ( i β β / β β m ) Ο Ο j + g 2 n ( Ο Ο Β― Β― k Ο Ο k ) Ο Ο j + g 2 n ( Ο Ο Β― Β― k Ξ³ Ξ³ 5 Ο Ο k ) Ξ³ Ξ³ 5 Ο Ο j = 0. {\displaystyle {\frac {\partial {\mathcal {L}}}{\partial {\bar {\psi }}_{j}}}-\partial _{\mu }{\frac {\partial {\mathcal {L}}}{\partial (\partial _{\mu }{\bar {\psi }}_{j})}}=(i\partial \!\!\!/\,-m)\psi _{j}+{\frac {g^{2}}{n}}\left({\bar {\psi }}_{k}\psi ^{k}\right)\psi _{j}+{\frac {g^{2}}{n}}\left({\bar {\psi }}_{k}\gamma ^{5}\psi ^{k}\right)\gamma ^{5}\psi _{j}=0.}
Siehe auch
Literatur
β’ David Gross und AndrΓ© Neveu: Dynamical symmetry breaking in asymptotically free field theories. In: Phys. Rev. D. 10 (10). 1974, S. 3235β3253, doi:10.1103/PhysRevD.10.3235, bibcode:1974PhRvD..10.3235G.