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Numerator Seagull and Extended Symmetries of Feynman Integrals

High Energy Physics - Theory · Submitted 10 Sep 2020

abstract compiled · 2026-09-23 · no language-model review

The authors' main claim We solve the equation system in two cases: over the singular locus and in a certain 3 scale sector where we obtain novel closed-form evaluations and epsilon expansions, thereby extending previous results for the numerator-free case.

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arXiv ID2009.04947 (version 2)
Pith IDLD7EC6KE, Pith's permanent record of this paper and its review
CitationAmit Schiller, Barak Kol, Ruth Shir. "Numerator Seagull and Extended Symmetries of Feynman Integrals." arXiv:2009.04947 (2020). https://pith.science/paper/LD7EC6KE
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What the abstract itself states, as probabilities: claims first 0.94 · states limitation 0.19 · human participants 0.01 · controlled comparison 0.06 · randomized assignment 0.01 · states quantitative result 0.57 · compares with prior results 0.90 · mentions code or data availability 0.02.

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arXiv listing abstract v2. Results and the main claim are underlined; .

The Symmetries of Feynman Integrals (SFI) method is extended for the first time to incorporate an irreducible numerator. This is done in the context of the so-called vacuum and propagator seagull diagrams, which have 3 and 2 loops, respectively, and both have a single irreducible numerator. For this purpose, an extended version of SFI (xSFI) is developed. For the seagull diagrams with general masses, the SFI equation system is found to extend by two additional equations. The first is a recursion equation in the numerator power, which has an alternative form as a differential equation for the generating function. The second equation applies only to the propagator seagull and does not involve the numerator. We solve the equation system in two cases: over the singular locus and in a certain 3 scale sector where we obtain novel closed-form evaluations and epsilon expansions, thereby extending previous results for the numerator-free case.

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What the classifier reports for each sentence. The number is the probability it gave the label.
#sentencerolethe authors' own workstates the main conclusionstrength
s0 The Symmetries of Feynman Integrals (SFI) method is extended for the first time to incorporate an irreducible numerator. contribution 1.00 0.87 0.49 asserted 1.00
s1 This is done in the context of the so-called vacuum and propagator seagull diagrams, which have 3 and 2 loops, respectively, and both have a single irreducible numerator. background 0.53 0.43 0.08 asserted 1.00
s2 For this purpose, an extended version of SFI (xSFI) is developed. contribution 0.52 0.92 0.11 asserted 1.00
s3 For the seagull diagrams with general masses, the SFI equation system is found to extend by two additional equations. result 0.83 0.92 0.14 asserted 1.00
s4 The first is a recursion equation in the numerator power, which has an alternative form as a differential equation for the generating function. result 0.53 0.87 0.09 asserted 1.00
s5 The second equation applies only to the propagator seagull and does not involve the numerator. result 0.78 0.87 0.05 asserted 1.00
s6 We solve the equation system in two cases: over the singular locus and in a certain 3 scale sector where we obtain novel closed-form evaluations and epsilon expansions, thereby extending previous results for the numerator-free case. result 0.92 0.96 0.59 asserted 1.00

What kind of paper the classifier reports this is: method or tool 0.96 · evidence from proof or derivation 1.00.

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The paper
Original abstract

The Symmetries of Feynman Integrals (SFI) method is extended for the first time to incorporate an irreducible numerator. This is done in the context of the so-called vacuum and propagator seagull diagrams, which have 3 and 2 loops, respectively, and both have a single irreducible numerator. For this purpose, an extended version of SFI (xSFI) is developed. For the seagull diagrams with general masses, the SFI equation system is found to extend by two additional equations. The first is a recursion equation in the numerator power, which has an alternative form as a differential equation for the generating function. The second equation applies only to the propagator seagull and does not involve the numerator. We solve the equation system in two cases: over the singular locus and in a certain 3 scale sector where we obtain novel closed-form evaluations and epsilon expansions, thereby extending previous results for the numerator-free case.

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1 arXiv paper cite this in 1 sentence

Each citing sentence is taken from the citing paper's LaTeX source and typed by Pith's classifier. A label appears at probability 0.8 or more (0.95 for support), a contest at 0.7 or more; the quoted words are the citing authors'. How each label was checked · JSON

What it cites · 26 sentences without a confident label

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  • The main novel evaluation extends the evaluation of the numerator-free vacuum seagull within a 3 mass scale sector [ref] to $I_1^VS$, which includes the numerator to the first power: * Eq. [ref] presents $I_1^VS$ in terms of $I^VS, J_1^VS$, which are detailed below it.

    The vacuum seagull: evaluating a 3-loop Feynman diagram with 3 mass scales · Summary and discussion · 1.00

Uses the method or tool of 1 paper
Uses data or values from 3 papers
  • The other ingredient for computing the $ϵ$-expansion of the vacuum seagull with numerator in the 3-mass sector through Equation ([ref]) is the $ϵ$-expansion for the vacuum seagull in this sector, which can be found in [ref] , and is repeated here for completeness: I^VS = 1/ϵ^3 I^(-3) + 1/ϵ^2 I^(-2) + 1/ϵ I^(-1) + O(ϵ^0), where I^(-3) = 1/6 [x_1+x_3 +2x_5] I^(-2) = x_1(1-1/2 ln(x_1/Q^2)) + x_3(1-1/2ln(x_3/Q^2)) +x_5(5/3-ln(x_5/Q^2))] I^(-2) = -2/3x_5 -2/3(x_1+x_3 +2x_5)ln(1-x_3/x_1)ln(1-x_5/x_1) + 3(x_1(1-1/2 lnx_1) + x_3(1-1/2lnx_3) +x_5(5/3-ln(x_5/Q^2)))(2-ln(x_5/Q^2)) + x_5/4( x_1/x_5 ln^2(x_1/x_5) + x_3/x_5 ln^2(x_3/x_5)) + 1/6(x_1+x_3 +2x_5)(7 +π^2/4 -9/2(2-ln(x_5/Q^2))^2) + x_5(1-x_1/x_5)Li_2(1-x_1/x_5) + x_5 (1-x_3/x_5)Li_2(1-x_3/x_5) + 2/3 (x_1+x_3 +2x_5) ( Li_1,1(x_1/x_3, x_3/x_5) + Li_1,2(x_3/x_1, x_1/x_5) .

    The vacuum seagull: evaluating a 3-loop Feynman diagram with 3 mass scales · Epsilon expansion of the 3 scale sector of the vacuum seagull · 0.85

  • The $ϵ$-expansions of the diagrams which appear in the source terms ([ref]), are [ref] Tad_1(x) = 1/ϵx - A(x) - ϵA_ϵ(x) Dia_1,1,1(x,y,z) = 1/2 ϵ^2 (x+y+z) - 1/ϵ (A(x) + A(y) + A(z) -1/2(x+y+z) ) -I_0(x,y,z) Melon_1,1,1,1(x,y,z,u) = 1/3 ϵ^3(xy + xz + xu + yz + yu + zu) +1/ϵ^2 [-1/2((y+z+u)A(x)+(x+z+u)A(y) +(x+y+u)A(z)+(x+y+z)A(u)) +1/3(xy + xz + xu + yz + yu + zu) -1/12(x^2+y^2+z^2+u^2) ] + 1/ϵ [A(x)A(y)+A(x)A(z)+A(x)A(u)+A(y)A(z)+A(y)A(u)+A(z)A(u) -(y+z+u)(A_ϵ(x)+A(x))/2 - cyclic +(x A(x)+ y A(y)+ z A(z) + u A(u))/4 +1/3(xy + xz + xu + yz + yu + zu) -3 (x^2+y^2+z^2+u^2)/8].

    Evaluation of the general 3-loop vacuum Feynman integral · Epsilon expansion of the 3 scale sector of the vacuum seagull · 1.00

  • The $ϵ$-expansions of the diagrams which appear in the source terms ([ref]), are [ref] Tad_1(x) = 1/ϵx - A(x) - ϵA_ϵ(x) Dia_1,1,1(x,y,z) = 1/2 ϵ^2 (x+y+z) - 1/ϵ (A(x) + A(y) + A(z) -1/2(x+y+z) ) -I_0(x,y,z) Melon_1,1,1,1(x,y,z,u) = 1/3 ϵ^3(xy + xz + xu + yz + yu + zu) +1/ϵ^2 [-1/2((y+z+u)A(x)+(x+z+u)A(y) +(x+y+u)A(z)+(x+y+z)A(u)) +1/3(xy + xz + xu + yz + yu + zu) -1/12(x^2+y^2+z^2+u^2) ] + 1/ϵ [A(x)A(y)+A(x)A(z)+A(x)A(u)+A(y)A(z)+A(y)A(u)+A(z)A(u) -(y+z+u)(A_ϵ(x)+A(x))/2 - cyclic +(x A(x)+ y A(y)+ z A(z) + u A(u))/4 +1/3(xy + xz + xu + yz + yu + zu) -3 (x^2+y^2+z^2+u^2)/8].

    Effective potential at three loops · Epsilon expansion of the 3 scale sector of the vacuum seagull · 1.00

Compares with 1 paper
  • In this case we get the solution I^PS|_x_5=0 = (O_2-O_5)I^PS/x_12 +1/d-2[2x_3∂_3 -2x_4∂_4/x_34(O_3+O_4-O_5)I^PS|_x_5=0 -2x_1∂_1-2x_2∂_2/x_12O_5I^PS]_x_5=0 .Using equations for the sources in appendix [ref] we reproduce the result in equation (6) of [ref] , namely I^PS|_x_5=0 = [O_2I^PS/x_12-(O_3-O_4)I^PS/x_34 -x_12(2x_3∂_3 -2x_4∂_4 )-x_34(4x_2 ∂_2 + 2x_3 ∂_3 + 2x_4 ∂_4 + 8-3d)/(d-2)x_12x_34O_5 I^PS ]_x_5=0 .

    Counting master integrals: Integration by parts vs. functional equations · $x_5=0$ · 0.88

Cites as background 22 papers

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