TY - JOUR
T1 - Non-linear equation in the re-summed next-to-leading order of perturbative QCD
T2 - the leading twist approximation
AU - Contreras, Carlos
AU - Levin, Eugene
AU - Meneses, Rodrigo
AU - Sanhueza, Michael
N1 - Publisher Copyright:
© 2020, The Author(s).
PY - 2020/11/1
Y1 - 2020/11/1
N2 - In this paper, we use the re-summation procedure, suggested in Ducloué et al. (JHEP 1904:081, 2019), Salam (JHEP 9807:019 1998), Ciafaloni et al. (Phys Rev D 60:1140361999) and Ciafaloni et al. (Phys Rev D 68:114003, 2003), to fix the BFKL kernel in the NLO. However, we suggest a different way to introduce the non-linear corrections in the saturation region, which is based on the leading twist non-linear equation. In the kinematic region: τ≡r2Qs2(Y)≤1, where r denotes the size of the dipole, Y its rapidity and Qs the saturation scale, we found that the re-summation contributes mostly to the leading twist of the BFKL equation. Assuming that the scattering amplitude is small, we suggest using the linear evolution equation in this region. For τ>1 we are dealing with the re-summation of (α¯Slnτ)n and other corrections in NLO approximation for the leading twist. We find the BFKL kernel in this kinematic region and write the non-linear equation, which we solve analytically. We believe the new equation could be a basis for a consistent phenomenology based on the CGC approach.
AB - In this paper, we use the re-summation procedure, suggested in Ducloué et al. (JHEP 1904:081, 2019), Salam (JHEP 9807:019 1998), Ciafaloni et al. (Phys Rev D 60:1140361999) and Ciafaloni et al. (Phys Rev D 68:114003, 2003), to fix the BFKL kernel in the NLO. However, we suggest a different way to introduce the non-linear corrections in the saturation region, which is based on the leading twist non-linear equation. In the kinematic region: τ≡r2Qs2(Y)≤1, where r denotes the size of the dipole, Y its rapidity and Qs the saturation scale, we found that the re-summation contributes mostly to the leading twist of the BFKL equation. Assuming that the scattering amplitude is small, we suggest using the linear evolution equation in this region. For τ>1 we are dealing with the re-summation of (α¯Slnτ)n and other corrections in NLO approximation for the leading twist. We find the BFKL kernel in this kinematic region and write the non-linear equation, which we solve analytically. We believe the new equation could be a basis for a consistent phenomenology based on the CGC approach.
UR - http://www.scopus.com/inward/record.url?scp=85096406535&partnerID=8YFLogxK
U2 - 10.1140/epjc/s10052-020-08580-w
DO - 10.1140/epjc/s10052-020-08580-w
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AN - SCOPUS:85096406535
SN - 1434-6044
VL - 80
JO - European Physical Journal C
JF - European Physical Journal C
IS - 11
M1 - 1029
ER -