Abstract
We investigate the origin of next-to-leading power (NLP) corrections to the event shapes’ thrust and c-parameter, at next-to-leading order. For both event shapes, we trace the origin of such terms in the exact calculation, and compare with a recent approach involving the eikonal approximation and momentum shifts that follow from the Low–Burnett–Kroll–Del Duca (LBKD) theorem. We assess the differences both analytically and numerically. For the c-parameter both exact and approximate results are expressed in terms of elliptic integrals, but near the elastic limit it exhibits patterns similar to the thrust results.
Similar content being viewed by others
References
T Kinoshita and A Ukawa, Lect. Notes Phys. 39, 55 (1975), https://doi.org/10.1007/BFb0013300
T D Lee and M Nauenberg, Phys. Rev. B 133, 1549 (1964), https://doi.org/10.1103/PhysRev.133.B1549
G Parisi, Phys. Lett. B 90, 295 (1980), https://doi.org/10.1016/0370-2693(80)90746-7
G Curci and M Greco, Phys. Lett. B 92, 175 (1980), https://doi.org/10.1016/0370-2693(80)90331-7
G Sterman, Nucl. Phys. B 281, 310 (1987), https://doi.org/10.1016/0550-3213(87)90258-6
S Catani and L Trentadue, Nucl. Phys. B 327, 323 (1989), https://doi.org/10.1016/0550-3213(89)90273-3
S Catani and L Trentadue, Nucl. Phys. B 353, 183 (1991), https://doi.org/10.1016/0550-3213(91)90506-S
J G M Gatheral, Phys. Lett. B 133, 90 (1983), https://doi.org/10.1016/0370-2693(83)90112-0
J Frenkel and J C Taylor, Nucl. Phys. B 246, 231 (1984), https://doi.org/10.1016/0550-3213(84)90294-3
G F Sterman, AIP Conf. Proc. 74, 22 (1981), https://doi.org/10.1063/1.33099
G P Korchemsky and G Marchesini, Nucl. Phys. B 406, 225 (1993), https://doi.org/10.1016/0550-3213(93)90167-N
G P Korchemsky and G Marchesini, Phys. Lett. B 313, 433 (1993), https://doi.org/10.1016/0370-2693(93)90015-A
S Forte and G Ridolfi, Nucl. Phys. B 650, 229 (2003), https://doi.org/10.1016/S0550-3213(02)01034-9
H Contopanagos, E Laenen and G F Sterman, Nucl. Phys. B 484, 303 (1997), https://doi.org/10.1016/S0550-3213(96)00567-6
T Becher and M Neubert, Phys. Rev. Lett. 97, 082001 (2006), https://doi.org/10.1103/PhysRevLett.97.082001
M D Schwartz, Phys. Rev. D 77, 014026 (2008), https://doi.org/10.1103/PhysRevD.77.014026
C W Bauer, S Fleming, C Lee and G Sterman, Phys. Rev. D 78, 034027 (2008), https://doi.org/10.1103/PhysRevD.78.034027
J-Y Chiu, A Fuhrer, R Kelley and A V Manohar, Phys. Rev. D 80, 094013 (2009), https://doi.org/10.1103/PhysRevD.80.094013
E Gardi, Nucl. Phys. B 622, 365 (2002), https://doi.org/10.1016/S0550-3213(01)00594-6
N Agarwal, A Mukhopadhyay, S Pal and A Tripathi, JHEP 03, 155 (2021), https://doi.org/10.1007/JHEP03(2021)155
E Laenen, Pramana – J. Phys. 63, 1225 (2004), https://doi.org/10.1007/BF02704892
G Luisoni and S Marzani, J. Phys. G 42, 103101 (2015), https://doi.org/10.1088/0954-3899/42/10/103101
T Becher, A Broggio and A Ferroglia, Introduction to soft-collinear effective theory (Springer, 2015) Vol. 896
J Campbell, J Huston and F Krauss, The black book of quantum chromodynamics: A primer for the LHC era (Oxford University Press, 2017)
N Agarwal, L Magnea, C Signorile-Signorile and A Tripathi, Phys. Rep. 994, 1 (2023), https://doi.org/10.1016/j.physrep.2022.10.001
C W Bauer, S Fleming and M E Luke, Phys. Rev. D 63, 014006 (2000), https://doi.org/10.1103/PhysRevD.63.014006
C W Bauer and I W Stewart, Phys. Lett. B 516, 134 (2001), https://doi.org/10.1016/S0370-2693(01)00902-9
C W Bauer, S Fleming, D Pirjol and I W Stewart, Phys. Rev. D 63, 114020 (2001), https://doi.org/10.1103/PhysRevD.63.114020
C W Bauer, D Pirjol and I W Stewart, Phys. Rev. D 65, 054022 (2002), https://doi.org/10.1103/PhysRevD.65.054022
D Bonocore, E Laenen, L Magnea, S Melville, L Vernazza and C D White, JHEP 2015, 8 (2015), https://doi.org/10.1007/JHEP06(2015)008
D Bonocore, E Laenen, L Magnea, L Vernazza and C D White, JHEP 2016, 121 (2016), https://doi.org/10.1007/JHEP12(2016)121
I Moult, I W Stewart, G Vita and H X Zhu, JHEP 08, 013 (2018), https://doi.org/10.1007/JHEP08(2018)013
M Beneke, A Broggio, S Jaskiewicz and L Vernazza, JHEP 07, 078 (2020), https://doi.org/10.1007/JHEP07(2020)078
I Moult, I W Stewart and G Vita, JHEP 11, 153 (2019), https://doi.org/10.1007/JHEP11(2019)153
N Bahjat-Abbas et al, JHEP 11, 002 (2019), https://doi.org/10.1007/JHEP11(2019)002
M Beneke, M Garny, S Jaskiewicz, R Szafron, L Vernazza and J Wang, JHEP 01, 094 (2020), https://doi.org/10.1007/JHEP01(2020)094
I Moult, G Vita and K Yan, JHEP 07, 005 (2020), https://doi.org/10.1007/JHEP07(2020)005
A H Ajjath, P Mukherjee, V Ravindran, A Sankar and S Tiwari, JHEP 04, 131 (2021), https://doi.org/10.1007/JHEP04(2021)131
M Beneke, M Garny, S Jaskiewicz, R Szafron, L Vernazza and J Wang, JHEP 10, 196 (2020), https://doi.org/10.1007/JHEP10(2020)196
A H Ajjath, P Mukherjee and V Ravindran, Phys. Rev. D 105, 094035 (2022), https://doi.org/10.1103/PhysRevD.105.094035
M van Beekveld, L Vernazza and C D White, JHEP 12, 087 (2021), https://doi.org/10.1007/JHEP12(2021)087
Z L Liu and M Neubert, JHEP 04, 033 (2020), https://doi.org/10.1007/JHEP04(2020)033
M Krämer, E Laenen and M Spira, Nucl. Phys. B 511, 523 (1998), https://doi.org/10.1016/S0550-3213(97)00679-2
R D Ball, M Bonvini, S Forte, S Marzani and G Ridolfi, Nucl. Phys. B 874, 746 (2013), https://doi.org/10.1016/j.nuclphysb.2013.06.012
C Anastasiou, C Duhr, F Dulat, F Herzog and B Mistlberger, Phys. Rev. Lett. 114, 212001 (2015), https://doi.org/10.1103/PhysRevLett.114.212001
M van Beekveld, W Beenakker, E Laenen and C D White, JHEP 03, 106 (2020), https://doi.org/10.1007/JHEP03(2020)106
M van Beekveld, E Laenen, J S Damsté and L Vernazza, JHEP 05, 114 (2021), https://doi.org/10.1007/JHEP05(2021)114
A H Ajjath, P Mukherjee, V Ravindran, A Sankar and S Tiwari, Eur. Phys. J. C 82, 234 (2022), https://doi.org/10.1140/epjc/s10052-022-10174-7
E Laenen, G Stavenga and C D White, JHEP 2009, 054 (2009), https://doi.org/10.1088/1126-6708/2009/03/054
E Laenen, L Magnea, G Stavenga and C D White, JHEP 2011, 141 (2011), https://doi.org/10.1007/JHEP01(2011)141
G Soar, A Vogt, S Moch and J A M Vermaseren, Nucl. Phys. 832, 152 (2010)
D de Florian, J Mazzitelli, S Moch and A Vogt, JHEP 2014, 1 (2014)
N A L Presti, A A Almasy and A Vogt, Phys. Lett. B 737, 120 (2014)
D Bonocore, Asymptotic dynamics on the worldline for spinning particles, arXiv:2009.07863 [hep-th]
H Gervais, Phys. Rev. D 95, 125009 (2017), https://doi.org/10.1103/PhysRevD.95.125009
H Gervais, Phys. Rev. D 96, 065007 (2017), https://doi.org/10.1103/PhysRevD.96.065007
H P Gervais, Soft radiation theorems at all loop order in quantum field theory (Doctoral dissertion, State University of New York at Story Brook, 2017)
E Laenen, J Sinninghe Damsté, L Vernazza, W Waalewijn and L Zoppi, Phys. Rev. D 103, 034022 (2021), https://doi.org/10.1103/PhysRevD.103.034022
M Beneke et al, JHEP 07, 144 (2022), https://doi.org/10.1007/JHEP07(2022)144
D W Kolodrubetz, I Moult and I W Stewart, JHEP 05, 139 (2016), https://doi.org/10.1007/JHEP05(2016)139
I Moult, L Rothen, I W Stewart, F J Tackmann and H X Zhu, Phys. Rev. D 95, 074023 (2017), https://doi.org/10.1103/PhysRevD.95.074023
I Feige, D W Kolodrubetz, I Moult and I W Stewart, JHEP 11, 142 (2017), https://doi.org/10.1007/JHEP11(2017)142
M Beneke, M Garny, R Szafron and J Wang, JHEP 03, 001 (2018), https://doi.org/10.1007/JHEP03(2018)001
M Beneke, M Garny, R Szafron and J Wang, JHEP 11, 112 (2018), https://doi.org/10.1007/JHEP11(2018)112
A Bhattacharya, I Moult, I W Stewart and G Vita, JHEP 05, 192 (2019), https://doi.org/10.1007/JHEP05(2019)192
M Beneke, M Garny, R Szafron and J Wang, JHEP 09, 101 (2019), https://doi.org/10.1007/JHEP09(2019)101
G T Bodwin, J-H Ee, J Lee and X-P Wang, Phys. Rev. D 104, 116025 (2021), https://doi.org/10.1103/PhysRevD.104.116025
Z L Liu, B Mecaj, M Neubert and X Wang, Phys. Rev. D 104, 014004 (2021), https://doi.org/10.1103/PhysRevD.104.014004
R Boughezal, X Liu and F Petriello, JHEP 03, 160 (2017), https://doi.org/10.1007/JHEP03(2017)160
I Moult, I W Stewart and G Vita, JHEP 07, 067 (2017), https://doi.org/10.1007/JHEP07(2017)067
C H Chang, I W Stewart and G Vita, JHEP 04, 041 (2018), https://doi.org/10.1007/JHEP04(2018)041
M Beneke et al, JHEP 03, 043 (2019), https://doi.org/10.1007/JHEP03(2019)043
M A Ebert, I Moult, I W Stewart, F J Tackmann, G Vita and H X Zhu, JHEP 04, 123 (2019), https://doi.org/10.1007/JHEP04(2019)123
I Moult, I W Stewart, G Vita and H X Zhu, JHEP 05, 089 (2020), https://doi.org/10.1007/JHEP05(2020)089
Z L Liu and M Neubert, JHEP 06, 060 (2020), https://doi.org/10.1007/JHEP06(2020)060
Z L Liu, B Mecaj, M Neubert, X Wang and S Fleming, JHEP 07, 104 (2020), https://doi.org/10.1007/JHEP07(2020)104
J Wang, Resummation of double logarithms in loop-induced processes with effective field theory, arxiv:1912.09920
A Banfi, G Salam and G Zanderighi, JHEP 0201, 018 (2002)
S Catani, G Turnock and B Webber, Phys. Lett. B 295, 269 (1992), https://doi.org/10.1016/0370-2693(92)91565-Q
S Catani, L Trentadue, G Turnock and B Webber, Nucl. Phys. B 407, 3 (1993), https://doi.org/10.1016/0550-3213(93)90271-P
R Ellis, W Stirling and B Webber, QCD and collider physics (Cambridge University Press, 2011) Vol. 8
Y L Dokshitzer, A Lucenti, G Marchesini and G P Salam, JHEP 1998, 011 (1998), https://doi.org/10.1088/1126-6708/1998/01/011
M Dasgupta and G P Salam, JHEP 2002, 017 (2002), https://doi.org/10.1088/1126-6708/2002/03/017
V Antonelli, M Dasgupta and G P Salam, JHEP 2000, 001 (2000), https://doi.org/10.1088/1126-6708/2000/02/001
A G-D Ridder, T Gehrmann, E Glover and G Heinrich, JHEP 2007, 094 (2007), https://doi.org/10.1088/1126-6708/2007/12/094
T Becher and M D Schwartz, JHEP 2008, 034 (2008), https://doi.org/10.1088/1126-6708/2008/07/034
S Weinzierl, Phys. Rev. Lett.. 101, 162001 (2008), https://doi.org/10.1103/PhysRevLett.101.162001
A Gehrmann-De Ridder, T Gehrmann, E W N Glover and G Heinrich, Phys. Rev. Lett. 99, 132002 (2007), https://doi.org/10.1103/PhysRevLett.99.132002
T Becher and M D Schwartz, JHEP 0807, 034 (2008), https://doi.org/10.1088/1126-6708/2008/07/034
M Dasgupta and G P Salam, J. Phys. G 30, R143 (2004), https://doi.org/10.1088/0954-3899/30/5/R01
S Catani, G Turnock, B R Webber and L Trentadue, Phys. Lett. B 263, 491 (1991), https://doi.org/10.1016/0370-2693(91)90494-B
F Caola, S F Ravasio, G Limatola, K Melnikov and P Nason, JHEP 01, 093 (2022), https://doi.org/10.1007/JHEP01(2022)093
F Caola, S F Ravasio, G Limatola, K Melnikov, P Nason and M A Ozcelik, JHEP 12, 062 (2022), https://doi.org/10.1007/JHEP12(2022)062
P Nason and G Zanderighi, JHEP 06, 058 (2023), https://doi.org/10.1007/JHEP06(2023)058
V Del Duca, E Laenen, L Magnea, L Vernazza and C White, JHEP 11, 057 (2017), https://doi.org/10.1007/JHEP11(2017)057
M van Beekveld, W Beenakker, R Basu, E Laenen, A Misra and P Motylinski, Phys. Rev. D 100, 056009 (2019), https://doi.org/10.1103/PhysRevD.100.056009
M van Beekveld, W Beenakker, E Laenen, A Misra and C D White, PoS RADCOR2019, 053 (2019), https://doi.org/10.22323/1.375.0053
E Laenen, J Sinninghe Damsté, L Vernazza, W Waalewijn and L Zoppi, Phys. Rev. D 103, 034022 (2021), https://doi.org/10.1103/PhysRevD.103.034022
F E Low, Phys. Rev. 110, 974 (1958), https://doi.org/10.1103/PhysRev.110.974
T H Burnett and N M Kroll, Phys. Rev. Lett. 20, 86 (1968), https://doi.org/10.1103/PhysRevLett.20.86
V Del Duca, Nucl. Phys. B 345, 369 (1990), https://doi.org/10.1016/0550-3213(90)90392-Q
E Farhi, Phys. Rev. Lett. 39, 1587 (1977), https://doi.org/10.1103/PhysRevLett.39.1587
ALEPH Collaboration: A Heister et al, Eur. Phys. J. C 35, 457 (2004), https://doi.org/10.1140/epjc/s2004-01891-4
ALEPH Collaboration, The ALEPH QCD web site, https://aleph.web.cern.ch/aleph/aleph/newpub/physics.html
J F Donoghue, F E Low and S-Y Pi, Phys. Rev. D 20, 2759 (1979), https://doi.org/10.1103/PhysRevD.20.2759
G C Fox and S Wolfram, Phys. Rev. Lett. 41, 1581 (1978), https://doi.org/10.1103/PhysRevLett.41.1581
G Parisi, Phys. Lett. B 50, 367 (1974), https://doi.org/10.1016/0370-2693(74)90692-3
R K Ellis, D A Ross and A E Terrano, Nucl. Phys. B 178, 421 (1981), https://doi.org/10.1016/0550-3213(81)90165-6
S Catani and B R Webber, JHEP 10, 005 (1997), https://doi.org/10.1088/1126-6708/1997/10/005
E Gardi and L Magnea, JHEP 0308, 030 (2003)
A Erdelyi, Higher transcendental functions (McGraw Hill Company, 1953), Vol. II
M Abramowitz and I E Stegun, Handbook of mathematical functions (National Bureau of standards AMS, 1972), Vol. X
L Buonocore, M Grazzini, F Guadagni and L Rottoli, Subleading power corrections for event shape variables in\(e^+ e^-\)annihilation. arxiv:2311.12768
S Catani and B Webber, Phys. Lett. B 427, 377 (1998), https://doi.org/10.1016/S0370-2693(98)00359-1, https://arxiv.org/abs/hep-ph/9801350
A H Hoang, D W Kolodrubetz, V Mateu and I W Stewart, Phys. Rev. D 91, 094017 (2015), https://doi.org/10.1103/PhysRevD91.094017
Y L Dokshitzer and B R Webber, Phys. Lett. B 352, 451 (1995), https://doi.org/10.1016/0370-2693(95)00548-Y. https://arxiv.org/abs/hep-ph/9504219
R Akhoury and V I Zakharov, Phys. Lett. B 357, 646 (1995), https://doi.org/10.1016/0370-2693(95)00866-J. https://arxiv.org/abs/hep-ph/9504248
G P Korchemsky and G F Sterman, Nucl. Phys. B 437, 415 (1995), https://doi.org/10.1016/0550-3213(94)00006-Z. https://arxiv.org/abs/hep-ph/9411211
C Lee and G Sterman, Phys. Rev. D 75, 014022 (2007), https://doi.org/10.1103/PhysRevD.75.014022
Acknowledgements
MvB acknowledges support from a Royal Society Research Professorship (RP\(\backslash \)R1\(\backslash \)180112), the European Research Council under the European Union’s Horizon 2020 research and innovation programme (grant agreement No. 788223, PanScales), and by the Science and Technology Facilities Council under ST/T000864/1. EL and AT would like to thank the MHRD, Government of India, for the SPARC grant SPARC/2018–2019/P578/SL, Perturbative QCD for Precision Physics at the LHC. SM would like to thank CSIR, Govt. of India, for the SRF fellowship (09/1001(0052)/2019-EMR-I). The authors would like to thank Buonocore et al [113] for spotting a mistake in the expansion of \( \Pi [n_1(c), m_1(c)] \) in eq. (86).
Author information
Authors and Affiliations
Corresponding author
Appendices
Appendix A. Transformation of incomplete elliptic integrals
In this Appendix, we demonstrate how we handle the incomplete elliptic integrals that appear in the expression of c-parameter distribution. The final expression for the c-parameter distribution is written in a compact manner in eq. (83), where K, E and \( \Pi \) are the complete elliptic integrals of the first, second and third kinds, respectively given in eq. (84). However, when we perform integration over final variable y in eqs (78), (97) and (108), this integration produces incomplete elliptic integrals F, E and \( \Pi \). These incomplete elliptic integrals are later converted into complete integrals to arrive at eq. (83), as first written in [110]. The three kinds of incomplete elliptic integrals appearing in c-parameter distribution are
Here, \( \phi , m \) and n are called the amplitude, parameter and characteristic of the elliptic integrals, respectively. Equation (84) gives their respective complete forms. The corresponding transformation into a complete elliptic integral can be performed using the rules
The above transformation is only possible when the amplitude \(\phi =\pi /2\). The indefinite integration of eqs (78), (97) and (108) results in multiple incomplete elliptic integrals with only two unique amplitudes in their arguments, namely \( \phi _1(c,y) \) and \(\phi _2(c,y)\), given by
The amplitudes \( \phi _1(c,y) \) and \(\phi _2(c,y) \) are present in the arguments of all three kinds of incomplete elliptic integrals. If we directly substitute the upper limit (\(y_2\)) after integration, then none of the incomplete elliptic integrals with the amplitude \( \phi _1(c,y) \) can be reduced to a complete elliptic integral since
The transformation to complete elliptic integrals holds only when \( \phi _1 =\pi /2 \) as given in eq. (A.4). However, the incomplete elliptic integrals with the amplitude \( \phi _2(c,y), \) upon substitution of the upper limit, can be directly reduced to a complete elliptic integral as
We observe a similar but opposite behaviour when we substitute the lower limit (\( y_1 \)) into the integration result. This time, the incomplete elliptic integrals with the amplitude \(\phi _1(c,y)\) can be reduced to the complete elliptic integral as
while the elliptic integrals with amplitude \( \phi _2(c,y) \) cannot be reduced to the complete elliptic integral as
In order to resolve the issue of transforming the incomplete elliptic integrals to complete elliptic integrals, we modify the upper and lower limits of y integration as
where e is an infinitesimal real off-set parameter that will be taken to zero at the end. The relative sign of e does not affect the final expression for the c-parameter distribution, which is independent of this off-set parameter. When we substitute the upper limit of integration \(y_2 \) with the off-set parameter as defined in the above expression, the amplitudes \( \phi _1(c,y) \) and \(\phi _2(c,y) \) modify and have the following form:
Similarly, from the lower limit, the amplitudes take the form
Note that, it is necessary to use this parameter because the straightforward substitution of limits did not allow the transformation of every incomplete elliptic integral. Let us consider a few examples to demonstrate how this off-set parameter solves the problem with incomplete elliptic integrals that cannot be reduced into complete elliptic integrals as their amplitude \( \phi \ne \pi /2 \). We categorise all the elliptic integrals appearing after y integration into two classes according to their amplitudes \(\phi \) as (i) non-reducible incomplete elliptic integrals \( (\phi \ne \pi /2) \) and (ii) reducible incomplete elliptic integrals \( (\phi = \pi /2) \).
1.1 Appendix A.1 Non-reducible incomplete elliptic integrals
Here we consider an incomplete elliptic integral that appears from the upper limit contributions, and the expression of the elliptic integral is
where \( m_1 \) is given in eq. (85). The amplitude of this elliptic function is
The elliptic integral in eq. (A.16) cannot be reduced to a complete elliptic integral as in the limit \(e \rightarrow 0\) the amplitude \( \phi _1(c,e) \rightarrow 0\). However, we can expand this elliptic integral in powers of e around \(e = 0\), and upon expanding we get
The expansion’s first term, proportional to \(e^{1/2}\), is the only significant term in the limit when \(e\rightarrow 0\).
The next term in the above expression is proportional to \(e^{3/2}\), and can be dropped. The small-e expression for these specific incomplete elliptic integrals occurring is then stored in the form
Now, we shift our attention toward the elliptic integrals that appears from the lower limit contribution, one such incomplete elliptic integral is
The above elliptic integral cannot be reduced into a complete elliptic integral as the amplitude \( \phi _2(c,e) \) is
and in the limit \( e \rightarrow 0 \) the amplitude \( \phi _2(c,e) \rightarrow 0 \). Following the similar procedure as in eq. (A.19), the elliptic integral in eq. (A.20) is expanded around \( e = 0 \), to get
The coefficients of these elliptic functions depend on e when the integration limits are modified in accordance with eq. (A.11). When we expand our final result in powers of e, the negative powers of \( \sqrt{e} \) from the coefficients combine with the positive powers of \( \sqrt{e} \) from the stored expressions of non-reducible incomplete elliptic integrals to yield a few terms independent of e. Subsequently, e can be set to zero.
1.2 Appendix A.2 Reducible incomplete elliptic integrals
The category of incomplete elliptic integrals, which can be reduced to complete elliptic integrals is easier to handle as compared with non-reducible ones. An elliptic integral appearing from the upper limit contribution is
where the amplitude \( \phi _2(c,e)\) reads as
In the limit \( e \rightarrow 0 \) the amplitude \( \phi _2(c,e) \rightarrow \pi /2 \) and this incomplete elliptic integral can be reduced directly to a complete elliptic integral using the reduction formula in eq. (A.4)
In this way, all reducible incomplete elliptic integrals are substituted with their corresponding complete elliptic integrals. Upon substituting all the incomplete elliptic integrals, our final result is expanded in powers of e. No negative powers occur and e can be taken to zero, yielding eq. (83).
Appendix B. Eikonal approximation and result summary
1.1 Appendix B.1 Eikonal approximation to the thrust and c-parameter distribution
In §3.3 and §4.3, we compared the shifted approximation with the LP expression of the exact distribution in figures 3a and 7a, for the thrust and c-parameter distribution, respectively. Here we add the results from the simpler eikonal approximation for comparison. The eikonal case follows from the approximated matrix element squared and is given by the first term in eq. (48) as
Using the above expression and the exact definitions of thrust and c-parameter in eqs (10) and (69), one finds for their respective distributions
The eikonal matrix element squared generates LL terms at LP correctly, together with some LL and NLL at NLP. It does not capture any NLL term at LP since it lacks contributions from hard-collinear gluon emission. In figures 8a and 8b, we plot these eikonal results together with the thrust and c-parameter distributions computed from the exact approach as given in eqs (28) and (83) along with the shifted approximation results up to NLP from eqs (47) and (101). Clearly for both event shapes, the shifted kinematics methods provides a significantly better approximation than the eikonal approximation.
1.2 Appendix B.2 Table of results
In table 1, we summarise our results for the thrust and the c-parameter using different approximations of the matrix elements squared: eikonal, exact, shifted kinematics, as well as the remainder/soft quark part.
Rights and permissions
Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law.
About this article
Cite this article
Agarwal, N., van Beekveld, M., Laenen, E. et al. Next-to-leading power corrections to event-shape variables. Pramana - J Phys 98, 60 (2024). https://doi.org/10.1007/s12043-024-02743-0
Received:
Revised:
Accepted:
Published:
DOI: https://doi.org/10.1007/s12043-024-02743-0
Keywords
- Perturbative quantum chromodynamics
- next-to-leading order calculation
- next-to-leading power
- leading logarithms