1999 European School of High-Energy Physics: Časta-Papiernička, Slovak Republic, 22 August-4 September 1999 : ProceedingsA. Olchevski |
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Page 36
... integral m The Ao function is defined by the integral iñ2 Ao ( m ) = μ2 μ1- " / 8 " q q2 + m2 - it ' 1 " — ie ( 161 ) where we introduced the t'Hooft scale parameter μ in order to prevent changing the dimension of this integral at the ...
... integral m The Ao function is defined by the integral iñ2 Ao ( m ) = μ2 μ1- " / 8 " q q2 + m2 - it ' 1 " — ie ( 161 ) where we introduced the t'Hooft scale parameter μ in order to prevent changing the dimension of this integral at the ...
Page 37
... integral may be reduced in a similar way , see Section 5.1.1.2 of Ref . [ 1 ] . 3.5 Two - point integrals , B ... integral The scalar Bo function is defined by the integral containing two propagators do and di , one of which depends on ...
... integral may be reduced in a similar way , see Section 5.1.1.2 of Ref . [ 1 ] . 3.5 Two - point integrals , B ... integral The scalar Bo function is defined by the integral containing two propagators do and di , one of which depends on ...
Page 44
... integrals The rank one tensor integral is defined by -n in2C1 ( p } , p2 , Q2 ; m1 , m2 , M3 = μ Ꮄ q զի dodid2 " μ and its decomposition looks like in2 [ C11 ( pỉ , p2 , Q2 ; m1 , m2 , M3 ) P14 + C12 ( Pỉ , P2 , Q2 ; m1 , M2 , M3 ) ...
... integrals The rank one tensor integral is defined by -n in2C1 ( p } , p2 , Q2 ; m1 , m2 , M3 = μ Ꮄ q զի dodid2 " μ and its decomposition looks like in2 [ C11 ( pỉ , p2 , Q2 ; m1 , m2 , M3 ) P14 + C12 ( Pỉ , P2 , Q2 ; m1 , M2 , M3 ) ...
Contents
Field Theory and the Standard Model | 1 |
Astrophysics and cosmology | 109 |
Determination of cosmological parameters | 126 |
39 other sections not shown
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