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JHEP03(2018)048
Published for SISSA by Springer
Received: January 31, 2018
Accepted: March 2, 2018
Published: March 8, 2018
Double-Higgs boson production in the high-energy
limit: planar master integrals
Joshua Davies,
a
Go Mishima,
a,b
Matthias Steinhauser
a
and David Wellmann
a
a
Institut f¨ur Theoretische Teilchenphysik, Karlsruhe Institute of Technology (KIT),
Wolfgang-Gaede Straße 1, 76128 Ka r lsruhe, Germany
b
Institut f¨ur Kernphysik, Karlsruhe Institute of Technology (KIT),
Hermann-von-Helmholtz-Platz 1, 76344 Eggenstein-Leopoldshafen, Germany
E-mail:
joshua.davies@kit.edu, go.mishima@kit.edu,
matthias.steinhauser@kit.edu, david.wellmann@kit.edu
Abstract: We consider the virtual corrections to the proc e ss gg → HH at NLO in the
high energy limit and compute the corresponding planar master integrals in an expansion
for small top quark mass. We provide details on the evaluation of the boundary conditions
and present analytic results expressed in terms of harmonic polylogarithms.
Keywords: NLO Computations, Q CD Phenomenology
ArXiv ePrint:
1801.09696
Open Access,
c
The Authors.
Article funded by SCOAP
3
.
https://doi.org/10.1007/JHEP03(2018)048
JHEP03(2018)048
Contents
1 Introduction 1
2 gg → HH amplitude and kinematics 3
3 One-loop considerations 4
4 Reduction to master integrals 5
5 Calculation of master integrals 7
5.1 Differential equations 7
5.2 Boundary conditions 8
5.3 Solving the diff er e ntial equations 12
6 Conclusions 13
A One- and two-loop master integrals 14
B Reducing the dimensionality of Mellin-Barnes integrals 16
1 Introduction
One of the main aims of particle physics in the coming years is the ex p l or ati on of the scalar
sector of the theory which describes fundamental interactions, be it the Standard Model
or an extension. One h as to clarify whe t her the Higgs boson is a fundamental particle and
how the particles of the theory obtain their mass. A process which h el p s to find answers to
these questions is the production of Higgs boson pairs, since it is the simplest process which
is sensitive to the triple-Higgs boson coupling. Although experimentally quite challe ngi ng,
there is a chance that double Higgs production will be ob se r ved after the high-luminosity
upgrade of the CERN LHC.
The leading order (LO) corrections to Higgs boson pair production have been comput ed
in refs. [
1, 2] incl udi n g the exact dependence on the top quark mass and the M ande l st am
variables. At next-to-leading order (NLO), QCD corrections were computed for the fir st
time in ref. [
3] in the infinite top quark mass limit using an effective theory and an inde-
pendent cross check was provided in [
4] by performing an asymptotic ex p ansi on in the full
theory. In this way a quantitative estimate of the quark mass effects could be provided.
Virtual NLO corrections in the large-m
t
limit have also been computed in ref. [
5], c onfir m-
ing the results of ref. [
4]. Finite top quark mass effects have also been consi d er e d i n r e f. [6],
in which the exact real radiation contribution is combined with the effective-theory virtual
corrections. Within the effective theory also next-to-next-to-leading (NNLO) contributions
– 1 –
JHEP03(2018)048
are available [7, 8]. The NNLO result was completed in ref. [9] in which the three-loop
matching coefficient of the effective operator for two Higgs bosons and two, three or four
gluons was computed. Note that it differs from that of single Higgs boson producti on.
The re sul t of [
9] has been complemented by power-suppressed terms i n the top quark
mass in ref. [
10], where the soft-virtual approximation was constructed. The resummation
of threshold-enhanced logarithms to next-to-next-to-leading logarithmic (NNLL) accur acy
has been perfor me d in refs. [
11, 12] and differential distributions through NNLO for various
observables were c ompu te d in ref. [
13] in the heavy-top li mi t . Finally, exact NLO results
became available in refs. [
14, 15] using a numerical approach for the computation of t he
two-loop v i r t ual corrections. Bas ed on these results t he transverse momentum resumma-
tion has been considered in ref. [
16]. More recently the results of refs. [14, 15] have been
matched to parton shower s in refs. [
17, 18].
In this paper we study a class of massive two-loop four-point functions with massless
external particles. We describe in detail the methods used for the computation of the
amplitudes and in particular the evaluation of the master integrals. We aim to study
double Higgs boson production via the process gg → HH. Numerical NLO results are
available [
14, 15], however the calculation of cross sections is computationally expe nsi ve
and we want to provide an independent cross check in th e high-ene r gy region. We wish to
provide results in terms of compac t analytic expressions which can be used to construct
simple approximations or can be used directly in the kinematic region in which they are
valid. In thi s paper we provide the first step towards this goal by considering the part of
the amplitude whi ch is expressed in terms of planar master integrals.
We perform our calculation in the limit of vanishing Higgs boson mass which provides,
as we will demonstrate in section
3, a good approximation to the general case where
m
H
6= 0. Furthermore, finite Higgs-mass effec ts can be incorporated by a simple Taylor
expansion. Recently the amplitudes for single-Higgs boson plus jet production have been
considered in the limit of lar ge Higgs transverse momentum [
19]. In this reference an
expansion for small Higgs boson mass has been performed and thus the underlying integrals
are the same as those of our calculation, so part of our findings can be cross checked
against ref. [
19].
In the recent literature one can find se veral calculations where two-lo op box integrals
are also involved. However, the underlying integral families and/or the kinematics of the
external and internal masses are different. For example, in ref. [
20] the amplitude of a
Higgs boson and three partons has been considered. In the limit m
H
→ 0 their integral s
are also the same as ours. However, this limit cannot been taken since the calculation
is perf or med in the Euclidean region with the assumption m
2
H
< s < 0 an d the results
are expres se d in terms of multiple polylogarithms, which can not easily be analytically
continued into ot her regions. Si mi l ar arguments apply to other recent calculations such
as [
21] or [22]; analytic results have been ob tai ne d in terms of multiple polylogarithms
which can in principle be evaluated numerically, but are very unwieldy. This is a another
reason why we have decided to perform an expansion in the high ener gy limit. Our final
results have a simple structure in terms of harmonic polyl ogari t hms and can be evaluated
numerically in a fast and rel i abl e manner.
– 2 –
JHEP03(2018)048
An interesting approach to obtain simple and easy-to-evaluate expressions for gg →HH
at NLO has been developed in ref. [
23] where the large top mass expansion has been
combined with expansion terms obtained for the top threshold. A good approximation
of t he exact (purely numerical) result [
14, 15] has been constructed by combining the
different kinematic regions using Pad´e approximants. Further improvement is expec t ed
after inc orporating information about the gg → HH amplitude at high energies which is
the main purpose of this work.
The remain der of the pap e r is organized as follows: we introduce our notation in
section
2. In section 3 we briefly consider the one-loop correction s to gg → HH in the
high-energy limit to provide motivation for our calculation, and section
4 describes the
reduction of the amplitude t o master integrals. The main part of the paper is section
5 in
which we discuss t he calculation of the master integrals. We describe in detail the method
we used to compute the boundary values necessary for the soluti on of differential equations
for t he master integrals. In this paper we refrain from presenting long formulae, which
instead can be found in the ancillary file of thi s paper [24] .
2 gg → HH amplitude and kinematics
The amplitude g(q
1
)g(q
2
) → H(q
3
)H(q
4
), where all momenta are incoming, is conveniently
described in terms of the following variables
s = (q
1
+ q
2
)
2
, t = (q
1
+ q
3
)
2
, u = (q
2
+ q
3
)
2
, (2.1)
where we have that
q
2
1
= q
2
2
= 0 , q
2
3
= q
2
4
= m
2
H
, s + t + u = 2m
2
H
. (2.2)
Here we make the approximation m
H
= 0 which significantly simplifies the two-loop cal-
culation. Then we have instead that
s = 2q
1
· q
2
, t = 2q
1
· q
3
, u = 2q
2
· q
3
= −s − t, (2.3)
and integrals will depend on the variables s, t, m
2
t
. Note that finite Higgs mass effects can be
implemented by a simple Taylor expansion. Each integral is proportional to s
a
1
(s/µ
2
)
−ǫa
2
where a
2
= 1(2) at one-(two-)loop order, a
1
is its overall mass dimension, µ is the renor-
malization scale and we work in d = 4 − 2ǫ dimensions. In our calculation of the master
integrals we expand the integrals for small top quark mass. Thus, effectively we assume
that m
2
t
≪ s, t.
Due to Lorentz and gauge invariance there are only two independent Lorentz structures
and we can write
M = ε
1,µ
ε
2,ν
M
µν
= ε
1,µ
ε
2,ν
(M
1
A
µν
1
+ M
2
A
µν
2
) , (2.4)
where
A
µν
1
= g
µν
−
1
q
12
q
ν
1
q
µ
2
,
A
µν
2
= g
µν
+
q
33
q
2
T
q
12
q
ν
1
q
µ
2
−
2q
23
q
2
T
q
12
q
ν
1
q
µ
3
−
2q
13
q
2
T
q
12
q
ν
3
q
µ
2
+
2
q
2
T
q
µ
3
q
ν
3
, (2.5)
– 3 –
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