2000
DOI: 10.1016/s0550-3213(00)00223-6
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Differential equations for two-loop four-point functions

Abstract: At variance with fully inclusive quantities, which have been computed already at the two-or three-loop level, most exclusive observables are still known only at one-loop, as further progress was hampered so far by the greater computational problems encountered in the study of multi-leg amplitudes beyond one loop. We show in this paper how the use of tools already employed in inclusive calculations can be suitably extended to the computation of loop integrals appearing in the virtual corrections to exclusive ob… Show more

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Cited by 949 publications
(1,122 citation statements)
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“…As explained in [14,15,16], the form factors coming from the computation of the trace operation introduced in the previous Section are expressed in terms of several hundreds of scalar integrals. It is possible to express all these integrals as a combination of only 17 independent scalar integrals, called the Master Integrals (MIs) of the problem, by means of the so-called Laporta algorithm [17], using integration-by-parts identities [18], Lorentz invariance [19] and general symmetry relations. This reduction algorithm is performed exactly in D = (4 − 2ǫ) dimensions [20].…”
Section: Unsubtracted Contributionsmentioning
confidence: 99%
“…As explained in [14,15,16], the form factors coming from the computation of the trace operation introduced in the previous Section are expressed in terms of several hundreds of scalar integrals. It is possible to express all these integrals as a combination of only 17 independent scalar integrals, called the Master Integrals (MIs) of the problem, by means of the so-called Laporta algorithm [17], using integration-by-parts identities [18], Lorentz invariance [19] and general symmetry relations. This reduction algorithm is performed exactly in D = (4 − 2ǫ) dimensions [20].…”
Section: Unsubtracted Contributionsmentioning
confidence: 99%
“…2. method of [11], but also the Lorentz invariance identities [12] and the symmetry relations, that can occur in particular mass configurations. The identities can then be solved by standard techniques (Gauss substitution rule), whose implementation is, however, algebraically very demanding.…”
Section: Reduction To Mismentioning
confidence: 99%
“…As the spinor traces are in D-dimensional space-time, in all the above formulas Eqs. (7)(8)(9)(10)(11), all the r.h.s., strictly speaking, should be multiplied by the overall constant (1/4) Tr1, where Tr1 is the trace of the unit Dirac matrix in D-continuous dimensions. The overall constant is in fact undetermined for arbitrary D, except for its limiting value at D = 4, which is 1.…”
mentioning
confidence: 99%