https://phystev.cnrs.fr/wiki/ Mon, 06 Apr 2026 02:02:33 +0000 FeedCreator 1.8 https://phystev.cnrs.fr/wiki/lib/tpl/dokuwiki/images/favicon.ico https://phystev.cnrs.fr/wiki/ https://phystev.cnrs.fr/wiki/2023:groups:smhiggs:ggf-background-vbf:start?rev=1687246972&do=diff Gluon Fusion Background to VBF Topic Ideas * Study top mass dependence at NLO_FTapprox * Compare to impact of HEJ (see slide 6) * in HH, the effects were more sizeable [<https://arxiv.org/pdf/1803.02463.pdf]>; can we understand what differs for H+2j? * A possible simple prescription for Powheg: use LO ratio (exact/HTL) evaluated on Born-projected kinematics as a first approximation.$\sqrt{s} = 13.6\,\mathrm{TeV}$$M_\mathrm{H} = 125.09\,\mathrm{GeV}$$m_\mathrm{t} = 172.5\,\mathrm{GeV}$$… anonymous@undisclosed.example.com (Anonymous) 2023:groups:smhiggs:ggf-background-vbf Tue, 20 Jun 2023 09:42:52 +0000