Graph e111|e| — Masses zzzz|z|

Edge list: (e,0|z) (0,1|z) (0,1|z) (0,1|z) (e,1|z)
Nickel index: e111|e|:zzzz|z|
Database path: 2/2/3/e111|e|/01234/zzzz|z|

e111|e|:zzzz|z|
Propagator P1
Propagator P2
Propagator P3

External Leg E1
External Leg E2

View public records for this configuration ↓BELOW↓ or choose different configuration ↑ABOVE↑

Orders in ε: all
Authors: F.A. Berends, M. Böhm, M. Buza, R. Scharf
Description: The two-loop sunrise integral with three arbitrary masses is computed as a function of space-time dimension D. The result is a linear combination of Lauricella functions of type C.
Record 1501195102.h4Cm
added 27 Jul 2017 22:38 UTC
last modified 31 Aug 2017 22:48 UTC
Orders in ε: 0
Reference: arXiv:1504.03255
Authors: Luise Adams, Christian Bogner, Stefan Weinzierl
Description: The two-loop sunrise integral with three arbitrary masses is computed near 4 dimensions in the Euclidean region. The result is given in terms of an elliptic generalization of polylogarithms.
Record 1501610276.YLKm
added 01 Aug 2017 17:57 UTC
last modified 31 Aug 2017 22:41 UTC
Orders in ε: all
Reference: arXiv:1512.05630
Authors: Luise Adams, Christian Bogner, Stefan Weinzierl
Description: The two-loop sunrise integral with three equal masses is computed in D = 2 dimensions in the Euclidean region to arbitrary order. The results are obtained in terms of elliptic generalizations of polylogarithms.
Record 1501610510.crDo
added 01 Aug 2017 18:01 UTC
last modified 31 Aug 2017 22:41 UTC
Orders in ε: 0
Reference: arXiv:1112.4360
Authors: Stefan Müller-Stach, Stefan Weinzierl, Raphael Zayadeh
Description: A Picard–Fuchs differential equation is derived for the two-loop sunrise integral with three arbitrary masses in D = 2 dimensions. The equation was later solved in arXiv:1302.7004 and arXiv:1405.5640. The method by which the differential equation was obtained was generalized in arXiv:1212.4389.
Record 1501611166.Vp9t
added 01 Aug 2017 18:12 UTC
last modified 31 Aug 2017 22:42 UTC
Orders in ε: 0
Reference: arXiv:1601.08181
Authors: Spencer Bloch, Matt Kerr, Pierre Vanhove
Description: The two-loop sunrise integral with three arbitrary masses is computed in D = 2 dimensions using elliptic dilogarithms. A Calabi-Yau 3-fold associated to the underlying elliptic curve is discussed.
Record 1501613786.yMaN
added 01 Aug 2017 18:56 UTC
last modified 31 Aug 2017 22:42 UTC
Orders in ε: -2,-1,0
Reference: hep-ph/0501132
Authors: Stephen P. Martin, David G. Robertson
Description: TSIL (Two-loop Self-energy Integral Library) can be obtained from https://www.niu.edu/spmartin/TSIL/ or http://faculty.otterbein.edu/DRobertson/TSIL/
Submitter: spmartin@niu.edu
Record 1561740094.yWm7
added 28 Jun 2019 16:41 UTC
last modified 28 Jun 2019 16:41 UTC

If you use these results in your calculation, please also cite arXiv:1709.01266.

Add new record

Hover over Field name for details

Integrand type:     if other, please specify:

Propagator powers (the n in (p² - m²)-n for which result is valid, separate by comma if necessary, leave empty if n/a):
P1   P2   P3  

Order(s) in ε (separate by comma, empty if n/a):

Reducible:     Number of master integrals:

Reference (arXiv:yymm.nnnnn or hep-xx/yymmnnn preferred, empty if n/a):

Relevant equations in reference:

Authors:

Special chars for copy & paste:
q̄ ζ π ∏ ∑ ∞ → – ≤ ≥
Description (package URL, dimension computed in, type of functions, Euclidean/physical kinematics, weight, free text, etc.):

Submitter (e-mail, optional):

Additional material (PDFs not on arXiv, Mathematica/Maple/FORM/Python/Fortran programs, etc.):