Higgs Production at NNLL$'$+NNLO using Rapidity Dependent Jet Vetoes

The rapidity-dependent jet veto observables $\mathcal{T}_{Bj}$ and $\mathcal{T}_{Cj}$ provide a tight jet veto at central rapidity, gradually transitioning to a loose veto at forward rapidities. They divide the phase space into exclusive jet bins in a different way to the traditional jet veto observable $p_{Tj}$, and are advantageous to use under harsh pile-up conditions. We obtain predictions for the $0$-jet gluon-fusion (ggF) Higgs cross section using both of these veto observables at NNLL$'+$NNLO, and compare these predictions to the prior state-of-the-art of NLL$'+$NLO. A significant reduction in perturbative uncertainty is observed going from NLL$'+$NLO to NNLL$'+$NNLO, with the NNLL$'+$NNLO predictions lying inside the uncertainty band of the NLL$'+$NLO predictions. We also investigate the relative sensitivities of ggF Higgs cross sections with $\mathcal{T}_{Bj}$, $\mathcal{T}_{Cj}$ and $p_{Tj}$ jet vetoes to underlying event and hadronisation effects using an NLO+parton shower calculation. We find that the cross sections with $\mathcal{T}_{Bj}$ and $\mathcal{T}_{Cj}$ vetoes have a reduced sensitivity to underlying event and hadronisation effects compared to that with a $p_{Tj}$ veto.


Introduction
Jet vetoes find frequent application at the LHC, to separate different types of hard processes and cut away backgrounds. One key process where jet vetoes find application is in Higgs production -for example, in the H → W W * analysis, it is standard to apply a jet veto to reduce the dominant tt decay background.
For maximal background rejection, it is typically advantageous to set the jet veto scale T cut to be much smaller than the hard scale of the process Q. This induces large logarithms of T cut /Q in the perturbative series for the 0-jet cross section, which can be summed up to all orders to obtain precise predictions [1,2].
The standard jet variable by which jets are currently classified and vetoed is the transverse momentum p T j of a jet. One identifies all jets with a given radius R in an event, computes p T j for each jet, and vetoes the event if the p T j for any jet exceeds the veto scale p cut T j . Predictions for the 0-jet Higgs production cross section with a jet veto imposed via p T j have been obtained with a resummation of p T j /m H logarithms up to the NNLL order, matched to either NNLO or N 3 LO fixed order perturbation theory [3][4][5][6][7][8]. However, there are some drawbacks to using this variable. In harsh pile-up conditions, as are nowadays encountered at the LHC, it is hard to identify (and veto) jets with small p T j at large rapidity. This is due to the lack of tracking information at large |η j | ≥ 2.5, meaning that at large rapidities it is difficult to disentangle small p T j jets from the primary process from pile-up jets. One option is simply to raise the overall cut on p T j , but then the discriminating power of the jet veto is reduced. An alternative possibility is to consider a step-like jet veto, with a tight veto below some value of |η|, and a weaker veto above this value. The theoretical description of such step-like vetoes is discussed in Ref. [9].
A final possibility, proposed in Refs. [10,11] and which we focus on here, is to have a jet veto that is a smooth function of rapidity, being tight at central rapidities and gradually weakening as one goes forward. Four jet-veto variables of this kind were considered in Ref. [11]: T Bjcm = m T j e −|y j | T Cjcm = m T j 2 cosh (y j ) (1.2) where y j the rapidity of the jet and Y the rapidity of the Higgs. The transverse mass of the jet m T j = m 2 j + p 2 T j and is close to p T j for small jet radius R. The quantity T Bj(cm) has the same rapidity weighting as the global beam thrust hadronic event shape [1,12], whilst T Cj(cm) has the same rapidity weighting as the C-parameter defined for e + e − → hadrons. Resummation of veto logarithms for all of these observables can be achieved using the same framework (see Ref. [11] for details).
The veto observables in Eqs. (1.1) and (1.2) are closely linked, differing only in their reference point from which to define whether jets are 'central' and 'forward'; the observables in Eq. (1.1) do it with respect to the Higgs rapidity, whilst those in Eq. (1.2) do it with respect to the centre of momentum of the pp collision. In terms of avoiding the issues with forward pile-up jets, the latter alternative will be superior, although there should not be a drastic difference in performance between the two types of vetoes at the LHC, since the majority of Higgs bosons are produced at rather low rapidities. Here, we choose to focus on the observables in Eq. (1.1), motivated in part by the fact that these seem to be the preferred choice from an experimental perspective: in Ref. [13] the H + 0-jet cross section differential in T Cj was measured in the ATLAS H → γγ analysis.
Apart from the above considerations, given the general utility of jet binning it is clearly beneficial to have more than one way of dividing phase space up into jet bins -for certain analyses it may be advantageous to use T B/Cj rather than p T j . Vetoed cross sections using T B/Cj probe QCD radiation in a quite different way from cross sections with a p T j veto 1 , so studying and measuring these observables is also of interest in terms of testing our understanding of QCD radiation.
The factorisation framework to resum veto logarithms for colour-singlet 0-jet processes with a jet veto imposed via T B/Cj was established in Ref. [10,11] within soft collinear effective theory (SCET). For the gluon-fusion (ggF) Higgs cross section, predictions for the 0-jet cross section with a T B/Cj jet veto have been obtained at NLL +NLO [11]. In Ref. [14], the resummation ingredients (two-loop beam and soft functions) required for the NNLL resummation of colour-singlet 0-jet processes with a T B/Cj jet veto were computed.
The main goal of the present paper is to elevate the precision of the 0-jet ggF Higgs production predictions, for both T Bj and T Cj to NNLL in resummed logarithms of T B/Cj /m H , matched to NNLO fixed-order perturbation theory. We will include finite bottom and top quark mass effects up to two loops (NLO) in the Higgs production process, and resum timelike logarithms in the gg → H form factor to all orders [15][16][17][18][19][20]. Note that here we do not perform a resummation of logarithms of R (studied in Refs. [8,[21][22][23]), nor logarithms of m b /m H (studied in Refs. [24][25][26]).
A further goal is to investigate the relative sensitivity of the 0-jet ggH cross sections with T Bj , T Cj and p T j vetoes to the effects of hadronisation and underlying event (UE). These effects are difficult to describe from first principles and are typically modelled, so a minimal sensitivity to them is preferable. This investigation will be performed using a NLO + parton shower (PS) set-up, specifically Madgraph aMC@NLO [27] + Pythia8 [28]. We find that the cross sections with T Bj and T Cj vetoes are rather less sensitive to both UE and hadronisation than that with a p T j veto, which constitutes another advantage of using these veto observables.
This paper is organised as follows. In section 2 we review the SCET factorization formula derived in Refs. [10,11] for the H + 0-jet T B/Cj cross section, and outline the steps and necessary ingredients needed to obtain this cross section at NNLL +NNLO. In section 3 we give details of the procedure we use to determine the perturbative uncertainty in our results. Section 4 contains our results for the H + 0-jet T B/Cj cross section at NNLL +NNLO, and we investigate the effects of UE and hadronisation on the H + 0-jet T B/Cj and p T j cross sections using an NLO+PS set-up in section 5. Finally we conclude in section 6.

Factorization for the H + 0-jet cross section
The full pp → H + 0-jet cross section with a cut on the rapidity-dependent observable T f j < T cut (f = B, C) is given by, where the first term contains the resummed logarithms of T cut /m H , and dominates for small values of T cut , while the second term contains the nonsingular corrections which are suppressed by O(T cut /m H ) and become important at large T cut . The resummed H+0-jet cross section for T f j < T cut can be factorized as follows, [10,11] σ resum The hard function denoted by H gg contains the hard virtual corrections and is obtained by matching QCD onto the operator O ggH in SCET. The gluon beam function B g describes the collinear initial state radiation from the incoming gluons, while S f encodes the contribution from the soft radiation across the entire event. The term σ Rsub 0 contains O(R 2 ) corrections arising due to the clustering of two independent collinear or soft particles into one jet; following Refs. [7,10] we separate these off and treat them separately 2 .
The hard function is the IR-finite part of the MS renormalized ggH form factor, and is expressed in terms of the matching coefficient C ggH as, At NNLL , we require the hard function up to NNLO: where the C (0,1,2) ggH are the perturbative expansion coefficients of C ggH : Note that since C ggH begins at O(α s ) we absorb one power of α s into each coefficient C ggH . In C (0) and C (1) we include the top and bottom loops with the full mass dependence using the results of Refs. [29,30]. For the NNLO coefficient C (2) , we use the NNLO m t → ∞ result extracted from Refs. [31,32], reweighted by the ratio of C (0) with finite m t to C (0) with m t → ∞ (both with m b = 0). This approach to the NNLO term is the same as in Ref. [2].
The beam functions B g are the same for both the T Bj and T Cj observables as they describe collinear emissions in the regions of large forward rapidities where the measurement function for both these observables is the same. They can be computed as a convolution between the perturbative matching kernel I ij and the standard parton distribution functions (PDFs) as follows [1,33], For NNLL precision we require the matching kernel up to O(α 2 s ): This scheme is the second one discussed in section 3.2 of Ref. [14]. This implies that in the two-loop B and S, we do not include the ∆I indep , SC and ∆S f,indep terms computed in Ref. [14], and remove the C 2 A R 2 term associated with independent emission contributions from the anomalous dimensions of B and S.
The one-loop coefficients I (1) are given in Ref. [11] and are equal to the cumulants of the one-loop virtuality-dependent beam function matching coefficients computed in Ref. [2]. One can write the two-loop coefficients I (2) as follows: where the I G are the cumulants of the two-loop virtuality-dependent beam function matching coefficients computed in Ref. [34], and the expressions for ∆I (2) are given in section 3.1.2 of Ref. [14].
The soft function is defined as a vacuum matrix element of the product of soft Wilson lines along the two incoming gluon directions, with a measurement function imposing T f j < T cut . As with the other ingredients, we require its expansion to NNLO: The one-loop soft functions S (1) f for T Bj and T Cj are equal to the cumulants of the one-loop soft functions for thrust and C-parameter respectively; the expressions for both observables are given in Ref. [11]. Let us decompose the two-loop soft function as follows: The quantity S (2),non-Ab G,f is the cumulant of the 'non-Abelian' part of the two-loop thrust/Cparameter soft function. Expressions for ∆S (2) f are given in section 3.1.1 of Ref. [14]. Analytic results for S (2),non-Ab G,B can be extracted from the results in Refs. [35][36][37][38], whilst for S (2),non-Ab G,C we extracted numerical results for n f = 5 from Ref. [39]. In both cases the results are of the form: where a G,f and b G,f are given by: Numerical results for the two-loop soft functions S (2) f (T cut , R, µ) have also been obtained using SoftSERVE [40][41][42], where these results agree with those obtained using the procedure above.
The hard, beam and soft functions are evaluated at their natural scales µ H ∼ m H , µ B ∼ √ m H T cut and µ S ∼ T cut , to minimize the logarithms they contain, and then RG evolved to a common scale µ FO ∼ m H which sums the large logarithms. These satisfy RG equations with a multiplicative form due to the cumulant nature of the jet veto observables [10]: where the anomalous dimension has a generic form consisting of the µ-dependent cusp part and the non-cusp part as follows, The hard matching coefficient contains double logarithms of (−m 2 H −i0)/µ 2 H , so we choose µ H ∼ −im H in order to avoid large left over logarithms ln 2 (−1 − i0) = −π 2 . Choosing an imaginary hard scale ensures that the logarithms are fully resummed and results in better perturbative convergence. For NNLL resummation we require the cusp anomalous dimension Γ cusp up to 3 loops, and the non-cusp anomalous dimensions up to 2 loops. The expression for the former is given, for example, in Ref. [2] (using the results of Refs. [43,44]). The two-loop expression for γ g H [α s (µ)] can be found in the same paper (using the results of Refs. [45][46][47]). The dependence on jet radius enters through the two-loop non-cusp anomalous dimension of the beam and soft function, which can be split into a global and an R-dependent part, The global non-cusp anomalous dimensions γ g G,S [α s (µ)] and γ g G,B [α s (µ)] are those of the beam thrust soft and beam functions, and are given up to 2 loops in Ref. [2]. The R-dependent correction term for the soft function anomalous dimension, ∆γ g S [α s (µ), R], is given in section 3.1.1 of Ref. [14]; RGE consistency demands ∆γ g The solution of the RGE (Eq. (2.17)) has a similar structure for the hard, beam and soft functions. For the beam function, solving the RGE yields, with the evolution factor given by . (2.21) Explicit expressions for the evolution of the hard and soft functions along with the various factors relevant for the resummation at NNLL can be found in Refs. [2,11].
The contribution σ Rsub 0 in Eq. (2.2) takes account of the O(R 2 ) corrections for the clustering of independent emissions. The form of this term is as follows [4,7,14]: is the total NNLL evolution kernel, and µ avg = √ µ B µ S . Since the O(α 2 s ) corrections in the square brackets come from soft or collinear emissions, we choose to evaluate them at the geometric mean of the soft and beam scales, as in Ref. [7]. The expressions for these corrections can be found in section 3.2 of Ref. [14].
The nonsingular cross section computed at fixed order up to NNLO at scale µ FO can be obtained by expanding Eq. (2.1) up to NNLO with all scales set to µ FO . In Eq. (2.2) we expand the product of fixed order contributions to the H, B and S factors to O(α 2 s ), such that setting all scales to µ FO automatically results in the NNLO expansion. Thus: We compute the first term on the right hand side at NNLO as follows: is the full NNLO Higgs production cross section, and σ FO,NLO

≥1
(T f j > T cut ) is the NLO H + j cross section with the given cut.
We improve the NNLO nonsingular piece by including the resummation of time-like logarithms in this piece as well. The expression for the final NNLO nonsingular piece that we include is then [2,7]: In practice, the computation of σ nons,NNLO 0 is done with finite m b , m t up to NLO, and with m b → 0, m t → ∞ in the NNLO coefficient. This means that in the σ resum,NNLL 0 term of Eq. (2.24) we use a hard function H gg which is given by using Eq. (2.5) but with the m t → ∞ limit in the NNLO coefficient. The NNLO Higgs cross section is obtained using HNNLO [48][49][50], whilst the H +j cross section for T f j > T cut is generated using Madgraph5 aMC@NLO [27,51]. The computation of σ nons,NLO 0 is done with finite m t , m b using similar techniques. This procedure implies that for T cut → ∞, we reproduce the NNLO cross section including the resummation of time-like logarithms [20], which is numerically very close to the N 3 LO total cross section [52,53].

Profile scales and Perturbative Uncertainties
We now discuss how we choose the beam and soft scales as a function of T cut , which, following a standard convention for SCET computations, we refer to as the profile scales [54,55]. At small T cut m H , logarithms of T cut /m H are large, Eq. (2.2) applies, and we should set the beam and soft scales to their canonical values µ B ∼ √ m H T cut , µ S ∼ T cut to resum these logarithms appropriately. This is referred to as the resummation region. At large T cut m H , we enter the fixed-order region, in which the veto is sufficiently loose that the fixed-order formula applies, and we should set µ B ∼ m H , µ S ∼ m H . In the intermediate region, referred to as the transition region, one should ensure a smooth transition between these two behaviours, which we achieve through a suitable choice of profile scales.
One can determine the locations of the boundaries between these regions by plotting the fixed-order singular and nonsingular contributions to the fixed-order NNLO cross section differential in T f j . The singular piece directly follows from taking the derivative of Eq. (2.2) with respect to T cut , and contains the leading small T f j terms ∼ ln n (T f j /m H )/T f j (corresponding to the ln n (T cut /m H ) terms in the cumulant). The nonsingular contains the remainder of the NNLO cross section, obtained in practice by subtracting the singular contribution from a NLO H + j computation of the T f j spectrum from MadGraph5 aMC@NLO. At small T f j this should diverge at most as ln n (T f j /m H ). The resummation region should be defined by where the singular cross section greatly exceeds the nonsingular one, and we should enter the fixed-order region when the singular and nonsingular cross sections become of the same size.
We plot the singular, nonsingular and total NNLO cross sections differential in T Bj (left) and T Cj (right) in Fig. 1. One observes that at small T f j the computed nonsingular contribution indeed has a rather mild dependence on T f j , and does not diverge as strongly as 1/T f j ; 2) not proportional to δ(T cut ), which also appear in the singular spectrum calculation. Towards larger T f j values, around T f j ∼ 50 GeV, the singular and nonsingular contributions become comparable, and for T f j ∼ 70 GeV the singular contribution crosses zero. It is interesting to observe that the nonsingular contribution for T Cj is generally larger than that for T Bj . Comparing Fig. 1 to Fig. 2 of Ref. [11], we see no particular reason to adjust the boundaries of the resummation, transition and fixed-order regions from the ones chosen in the NLL +NLO calculation of Ref. [11]. The two boundaries are chosen to be at 18.75 GeV and 75 GeV for T Bj , and at 12.5 GeV and 68.75 GeV for T Cj .
The functional form of the profile scales we use are similar to those adopted in Refs. [7,11]. In particular, we have: where the profile function f run (x) is:

(3.2)
For r s = 1 the profiles reduce to those of Refs. [7,11]. For 2x 0 m H < T cut < x 1 m H , µ B and µ S have canonical scaling: µ S = r s T cut and µ B = √ r s m H T cut for µ FO = m H . The fixed-order region is reached at T cut = x 3 m H , with a smooth transition being achieved in two steps between x 1 m H and x 3 m H . We refer to T cut < 2x 0 m H as the 'nonperturbative region', and choose 2x 0 m H to be in vicinity of Λ QCD . In this region the variation of µ S/B is gradually turned off as T cut → 0, with µ S and µ B approaching the positive values x 0 µ FO and √ x 0 µ FO at T cut = 0. This is to avoid α s and the PDFs being evaluated at too low scales. In fact our purely perturbative predictions for the cross section will be insufficient in this (small) region, since neglected power corrections can become of O(1).
For the parameters x 0 − x 3 and µ FO , we make the same choices as in Ref. [11], which in particular enforces the same boundaries between resummation, transition and fixed-order regions as in that paper (and which are mentioned above). So, for T Bj we have: and for T Cj , The parameter r s should be chosen to be O(1). In the next section we will generate results using both r s = 1 and r s = 2.
Let us now move to a discussion of how we estimate the theoretical uncertainty in our predictions of the jet vetoed cross sections. These may be parametrized in terms of fully correlated (yield) and fully anti-correlated (migration) components [2,7,56,57]. The yield uncertainty corresponds to the fixed-order uncertainty ∆ FO . At large T cut this reproduces the fixed-order scale variation uncertainty in the total inclusive cross section. The migration uncertainty corresponds to the uncertainty in the resummed logarithmic series induced by the jet veto cut and is identified as the resummation uncertainty ∆ resum . The total uncertainty in the 0-jet cross section can be written as The resummation uncertainty ∆ resum can be obtained by varying the µ B and µ S scales using a multiplicative factor,

5)
For δ = 0, this reproduces the functional form of f vary used in Ref. [11]. Here we set δ = 0.05, so that when using r s = 2, we avoid either µ B or µ S rising above the fixed-order value of m H in any of the variations discussed below. The up and down variations of µ B and µ S are parametrized using this multiplicative factor as follows, with (α, β) = {(+1, 0), (−1, 0), (0, +1/6), (0, −1/6)}. The variations in the parameter α lead to a factor of 2 variation in µ S for T cut → 0, and a factor of √ 2 variation in µ B . The profiles thus obtained with α variation are shown for r s = 2 by the dashed curves in the middle panel of Fig. 2. The parameter β modifies µ B by varying the canonical relation µ B ∼ √ µ S µ H while keeping µ S fixed, as is shown for r s = 2 by the dotted lines in the right panel of Fig. 2. A detailed discussion about the choice of these parameters can be found in Ref. [11]. These variations in µ S and µ B vary the arguments of the logarithms in the evolution kernel, and thus help in estimating the higher-order corrections in the resummed results. The total resummation uncertainty ∆ resum is obtained by taking the maximum of the absolute deviation from the central profile.

Resummed Predictions at NNLL +NNLO
In this section we present our results for the 0-jet gluon-fusion Higgs cross section at NNLL + NNLO with the jet veto imposed via the T Bj and T Cj variables. We compare these results to NLL +NLO and NLL results for the same cross sections, to study the perturbative convergence. Let us briefly summarise our set-up. For the PDFs we use the MMHT sets [58]: the mmht2014lo135 set for the NLL, the mmht2014nlo120 set for the NLL +NLO, and the mmht2014nnlo118 set for the NNLL +NNLO predictions. We take m H = 125 GeV, m t = 172.5 GeV, m b = 4.7 GeV, and set n f = 5 in all perturbative ingredients. The effect of finite m b , m t are taken into account in the hard function of the resummation H gg and the nonsingular cross section up to NLO; for the NNLO coefficient of the nonsingular cross section we use  We plot the cross section with T B/Cj < T cut as a function of T cut , for two choices of r s in Eq. (3.2): r s = 1 and r s = 2. In each case we make plots using both a linear and a logarithmic x-axis. The results for r s = 2 are given in Fig. 3 and Fig. 5, and those for r s = 1 are given in Fig. 4 and Fig. 6. In each figure, we plot our NNLL +NNLO results in orange, and give NLL +NLO and NLL results in blue and green respectively.
In general, we see a substantial reduction of uncertainties going from NLL to NNLL , due to the increase in the accuracy of resummation as well as matching. The predictions of higher orders fall within the uncertainty bands of lower orders, thereby indicating a good  Figure 5. The same plots as in Fig. 3, but with a logarithmic x-axis.  Figure 6. The same plots as in Fig. 4, but with a logarithmic x-axis. perturbative convergence.
Comparing the results with r s = 2 to those with r s = 1, we see a better convergence between different orders in resummed perturbation theory in the former case, where this is particularly noticeable for T Cj . In the case of T Cj with r s = 1, one also observes that the top of the uncertainty band at T cut ∼ 20 GeV greatly exceeds that of the total NNLO cross section. This is of course unphysical. For these reasons we would advocate to use the results with r s = 2 for T Cj . The choice of r s = 2, corresponding to the choice of canonical scale µ S = 2T cut , also seems physically reasonable for T Cj , since the cut T Cj < T cut corresponds to an m T j cut that is everywhere looser than m T j < 2T cut . For the case of T Bj , there is not a strong difference between the r s = 1 or r s = 2 results and one can use either of these.
We note in passing that similar conclusions with regards to the scales in the resummation region were also found for thrust and C-parameter in e + e − collisions, in Ref. [39]. Furthermore, we note that in Ref. [2], where NNLL+NNLO predictions were obtained for Higgs production with a cut on beam thrust (the global equivalent of T Bj ), profile scales that are rather close to µ S = 2T cut , µ B = √ m H µ S in the resummation region were used.
Finally, in Table 1 we present numbers for the H+0-jet cross section defined by T B/Cj < T cut , at two sample values of T cut : 20 GeV and 30 GeV. We give the central predictions and perturbative uncertainties, for both the r s = 1 and r s = 2 cases. These numbers highlight the improvement in perturbative convergence going from r s = 1 to r s = 2 that was already visible in Figs. 3 -6. For the results with r s = 2, the perturbative uncertainties are smaller compared to the results with r s = 1, and the NNLL +NNLO results lie closer to the NLL +NLO ones for r s = 2. We again see that this is more pronounced for the T Cj case, leading to the choice r s = 1 being disfavoured for T Cj .

Effect of underlying event and hadronisation
The analytic resummed calculations presented in the previous section do not take into account the effects of underlying event or hadronisation. These effects are formally suppressed, but it is interesting to assess their practical numerical impact, and compare how much T B/Cj are affected with respect to the conventional jet veto observable p T j . In order to do this, we employ a NLO + parton shower set-up, as implemented in Mad-Graph5 aMC@NLO interfaced with Pythia8. In Pythia8, the parameters have been set to their default values as specified by the MadGraph5 aMC@NLO interface. These parameter values mainly correspond to the Monash 2013 tune [59] -in particular the underlying event and hadronisation parameters are set as in this tune. We generate ggF Higgs events, compute the cumulant distributions for T Bj , T Cj and p T j from these events, and investigate the effect of turning on and off hadronisation and underlying event (UE) in the shower on  Figure 7. NLO + parton shower results for the Higgs cross section for T B/Cj , p T j < T cut and R = 0.5, generated using MadGraph5 aMC@NLO interfaced with Pythia8. The overall normalisation of these predictions has been adjusted such that the central predictions reproduce the NNLO Higgs cross section (including resummation of time-like logarithms) for T cut → ∞. The green, red and purple bands represent various configurations with regards to the hadronisation and underlying event. For the T B/Cj cases, we also plot in blue the NNLL +NNLO analytic prediction for comparison. these cumulant distributions. Jets with R = 0.5 are identified in the events using the anti-k T algorithm [60].
In Fig. 7, we give the NLO+PS plots for all jet vetoes, for three configurations of the parton shower: hadronisation and UE turned on, hadronisation on and UE off, and both hadronisation and UE turned off. Fig. 8 presents the same plots, but with a logarithmic xaxis. For the T B/Cj cases, we also give the NNLL +NNLO prediction, using the same set-up as in section 4 and taking r s = 1 (r s = 2) for T Bj (T Cj ). To allow for a meaningful comparison, we rescale all NLO+PS predictions to the total cross section of our NNLL +NNLO predictions. The uncertainty bands on the NLO+PS results reflect the (rescaled) fixed-order scale variation.
From these plots, one can see that hadronisation tends to shift the p T j and T B/Cj distributions towards lower values, whilst UE pushes these distributions towards higher values. Non-perturbative hadronisation 'smears out' the energy in QCD particle sprays over a larger area in η − φ phase space, resulting in a loss of p T j and T B/Cj from any given jet with fixed R. UE sprays extra particles fairly evenly over the η − φ phase space, with these extra particles pushing up the p T j and T B/Cj values of all jets [61].
One can also already see from these plots that the cross section with a p T j veto is more strongly affected by hadronisation and UE effects than those with T Bj and T Cj vetoes. Finally, it is interesting to note that the rescaled NLO+PS predictions for T Bj and T Cj turn out to lie fairly close to the NNLL +NNLO predictions.
In order to exhibit in more detail the extent to which all three vetoed cross sections are sensitive to UE and hadronisation, we plot in Fig. 9 the following ratios: The first ratio indicates the extent to which each observable is sensitive to UE, and the second indicates the extent to which each observable is sensitive to hadronisation. The closer the R value is to 1, the lower the sensitivity is. For p T j and T Bj , the cumulant cross sections σ 0 T cut are computed by integrating p T j or T Bj up to T cut as before, whilst for T Cj we integrate up to T cut /2. We do this so that at a given point on the x-axis in Fig. 9 all the different veto observables correspond to the same 'central' p T j veto at y j = Y in the limit of small jet radius R (namely, p T j | y j =Y,R 1 < T cut ). These results confirm that the cross sections with T Bj and T Cj vetoes are less sensitive to UE and hadronisation effects than that with the p T j veto, and show that the cross section with the T Bj veto is less sensitive than that with the T Cj veto for the same central p T j veto. Reduced sensitivity is of course advantageous, given that our current theoretical description of these effects is based on models rather than first principles theory.
This ordering of sensitivities to UE and hadronisation effects actually makes intuitive sense. The rapidity-dependent vetoes T B/Cj impose a similar veto as p T j at y j = Y , but as one moves away from the Higgs rapidity and |y j − Y | increases, the veto is lifted and one moves towards simply measuring the inclusive Higgs cross section in these forward regions. The inclusive Higgs cross section is, of course, much less affected by hadronisation and UE than the cross section with a restriction on p T j , and this leads to the cross sections with a T B/Cj veto being less sensitive to UE and hadronisation than that with a p T j veto. With the same 'central' p T j veto at y j = Y , the veto is lifted more quickly as one goes forward in rapidity for T Bj than T Cj (see Fig. 1 of Ref. [11]), and this leads to the cross section with a T Bj veto being less sensitive to UE and hadronisation than the cross section with a T Cj veto.

Conclusions
In this paper, we obtained NNLL +NNLO predictions for the 0-jet gluon-fusion Higgs cross section, σ 0 (T cut ), where the jet veto is imposed by requiring that no identified jet has a value of T B/Cj greater than T cut . The observables T Bj and T Cj , defined in Eq. (1.1), correspond to a rapidity-dependent jet veto: they impose the tightest constraint on jet transverse mass at 'central' rapidities close to the Higgs rapidity, with the veto gradually loosening as one goes to forward rapidities away from the Higgs. The perturbative uncertainty in these predictions has been estimated through combined scale variations of the different resummation and fixedorder scales involved. We compared the NNLL +NNLO predictions to lower-order NLL and NLL +NLO ones, observing in general that the perturbative uncertainties significantly reduce as the perturbative order is increased, and that the predictions of higher orders fall within the uncertainty bands of lower orders, indicating good perturbative convergence. Explicit results have been provided for jet radius R = 0.5, but results for other jet radii can be provided on request to the authors.
In the 'resummation region' T cut m H , the soft and beam resummation scales µ S and µ B in our predictions should be chosen to be r s T cut and √ r s m H T cut respectively, where r s is some number of order 1. We investigated the use of both r s = 1 and r s = 2. Whilst for T Bj the r s = 1 and r s = 2 predictions look rather similar, for T Cj use of r s = 2 notably improves the perturbative convergence and avoids an unphysical behaviour in the jet-vetoed cross section. For these reasons, we advocate the use of our r s = 2 results for T Cj . Taking r s = 2 for T Cj , we find, setting T cut to the benchmark value of 20 GeV and R to 0.5, that the perturbative uncertainty on the vetoed cross section reduces from 15.7% at NLL +NLO to 9.77% at NNLL +NNLO, with the central value increasing from 33.4 pb to 37.3 pb. Repeating the exercise with T Bj and taking r s = 1, we find a reduction in uncertainty from 21.2% to 10.9%, with the central value increasing from 32.9 pb to 37.0 pb.
Using an NLO+PS set-up, we compared the effect of underlying event (UE) and hadronisation on 0-jet ggH cross sections where the jet veto constraint was implemented via T Bj , T Cj or the conventional jet veto observable p T j . Adjusting all three vetoes such that they imposed the same jet veto at central rapidities (at small R), we found that the cross-section with the T Bj veto was minimally sensitive to both UE and hadronisation, followed by that with T Cj , and then finally the cross section with the p T j veto was the most sensitive. The fact that the cross sections with rapidity-dependent jet vetoes have a reduced sensitivity to these theoretically less-well-understood effects is one advantage of using such vetoes.
The use of T B/Cj rather than p T j to classify and veto jets has practical advantages, and also provides complementary information on the properties of additional jet production in a given hard process. We look forward to comparing our predictions for 0-jet ggH cross sections with a T B/Cj veto against data from the LHC experiments.