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Towards an understanding of
jet substructure
1
Gavin Salam (CERN)with Mrinal Dasgupta, Alessandro Fregoso & Simone Marzani
Boost 2013Flagstaff, Arizona
August 2013
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013
As a field we’ve devised O(10-20) powerful methods to tag jet substructure.
Many of the methods have been tried out in searches and work; these kinds of methods will be crucial for
searches in the years to come.
2
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013
As a field we’ve devised O(10-20) powerful methods to tag jet substructure.
Many of the methods have been tried out in searches and work; these kinds of methods will be crucial for
searches in the years to come.
2
But from outside, the many methods make the field look pretty confusing.
And from inside, I get the impression we don’t always know why or how the methods work – which is bad if we’re looking for
robustness.
Is it time to get back to basics?
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013
What do we know currently?
At the time:• No clear picture of why the taggers might be similar or
different• No clear picture of how the parameter choices affect
the taggers
3
Boost 2010 proceedings:
1. Introduction
The Large Hadron Collider (LHC) at CERN is increasingly exploring phenomena at ener-
gies far above the electroweak scale. One of the features of this exploration is that analysis
techniques developed for earlier colliders, in which electroweak-scale particles could be con-
sidered “heavy”, have to be fundamentally reconsidered at the LHC. In particular, in the
context of jet-related studies, the large boost of electroweak bosons and top quarks causes
their hadronic decays to become collimated inside a single jet. Consequently a vibrant
research field has emerged in recent years, investigating how best to tag the characteristic
substructure that appears inside the single “fat” jets from electroweak scale objects, as
reviewed in Refs. [?,?,26]. In parallel, the methods that have been developed have started
to be tested and applied in numerous experimental analyses (e.g. [23–25] for studies on
QCD jets and [some searches]).
The taggers’ action is twofold: they aim to suppress or reshape backgrounds, while re-
taining signal jets and enhancing their characteristic jet-mass peak at the W/Z/H/top/etc.
mass. Nearly all the discussion of these aspects has taken place in the context of Monte
Carlo simulation studies [Some list], with tools such as Herwig [?, ?], Pythia [?, ?] and
Sherpa [?]. While Monte Carlo simulation is an extremely powerful tool, its intrinsic nu-
merical nature can make it di!cult to extract the key characteristics of individual taggers
and the relations between taggers (examining appropriate variables, as in [4], can be helpful
in this respect). As an example of the kind of statements that exist about them in the
literature, we quote from the Boost 2010 proceedings:
The [Monte Carlo] findings discussed above indicate that while [pruning,
trimming and filtering] have qualitatively similar e"ects, there are important
di"erences. For our choice of parameters, pruning acts most aggressively on the
signal and background followed by trimming and filtering.
While true, this brings no insight about whether the di"erences are due to intrinsic proper-
ties of the taggers or instead due to the particular parameters that were chosen; nor does it
allow one to understand whether any di"erences are generic, or restricted to some specific
kinematic range, e.g. in jet transverse momentum. Furthermore there can be significant
di"erences between Monte Carlo simulation tools (see e.g. [22]), which may be hard to diag-
nose experimentally, because of the many kinds of physics e"ect that contribute to the jet
structure (final-state showering, initial-state showering, underlying event, hadronisation,
etc.). Overall, this points to a need to carry out analytical calculations to understand the
interplay between the taggers and the quantum chromodynamical (QCD) showering that
occurs in both signal and background jets.
So far there have been three investigations into the analytical features that emerge from
substructure taggers. Ref. [19, 20] investigated the mass resolution that can be obtained
on signal jets and how to optimize the parameters of a method known as filtering [1].
Ref. [13] discussed constraints that might arise if one is to apply Soft Collinear E"ective
Theory (SCET) to jet substructure calculations. Ref. [14] observed that for narrow jets the
distribution of the N -subjettiness shape variable for 2-body signal decays can be resummed
– 2 –
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013
This talk → analytical understanding. Why?
4
Better Insight
Can guide taggers’ use in experimental
analyses
It may help us design better taggers
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013
This talk → analytical understanding. Why?
5
Better Insight
Can guide taggers’ use in experimental
analyses
It may help us design better taggers
Robustness
You know what you predict, what you don’t
Unlike MC, you have powerful handles for
cross-checks & accuracy estimates
There is a “right” answer
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013 6
Scope of our study
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013
What kind of events?
7
To fully understand “Boost” you want to study all possible signal (W/Z/H/top/…) and QCD jets.
But you need to start somewhere.We chose the QCD jets because:
(a) they have the richest structure.
(b) once you know understand the QCD jets,the route for understanding signal jets becomes clear too.
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013
study 3 taggers/groomers
8
Mass-drop tagger (MDT, aka BDRS)
Trimming
Pruning
Cannot possibly study all toolsThese 3 are widely used
Recluster
on scale Rsub
discard subjetswith < zcut pt
decluster &
discard soft junkrepeat until
find hard struct
jet mass/ptsets Rprune discard large-angle
soft clusteringsRecluster
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013 9
First use MC to get a panorama
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013
The key variables
10
For phenomenology
Jet mass: m
[as compared to W/Z/Hor top mass]
For QCD calculations
[R is jet opening angle– or radius]
Because ρ is invariant underboosts along jet direction
⇢ =m2
p2tR2⇢ =
m2
p2tR2⇢ =
m2
p2tR2
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013
!/"
d"
/ d
!
! = m2/(pt2 R2)
quark jets (Pythia 6 MC)
m [GeV], for pt = 3 TeV, R=1
Jets: C
/A w
ith R
=1. M
C: P
ythia
6.4
, DW
tune, p
arto
n-le
vel (n
o M
PI), q
q#
qq, p
t > 3
TeV
plain jet mass
0
0.1
0.2
0.3
10-6 10-4 0.01 0.1 1
10 100 1000
11
Start with “plain” jet mass
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013
!/"
d"
/ d
!
! = m2/(pt2 R2)
quark jets (Pythia 6 MC)
m [GeV], for pt = 3 TeV, R=1
Jets: C
/A w
ith R
=1. M
C: P
ythia
6.4
, DW
tune, p
arto
n-le
vel (n
o M
PI), q
q#
qq, p
t > 3
TeV
plain jet mass
0
0.1
0.2
0.3
10-6 10-4 0.01 0.1 1
10 100 1000
11
Physical mass for 3 TeV, R=1 jets
ρ ~ Rescaled mass2
(i.e. the QCD variable)
Start with “plain” jet mass
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013
mEW
!/"
d"
/ d
!
! = m2/(pt2 R2)
quark jets (Pythia 6 MC)
m [GeV], for pt = 3 TeV, R=1
Jets: C
/A w
ith R
=1. M
C: P
ythia
6.4
, DW
tune, p
arto
n-le
vel (n
o M
PI), q
q#
qq, p
t > 3
TeV
plain jet mass
0
0.1
0.2
0.3
10-6 10-4 0.01 0.1 1
10 100 1000
11
Physical mass for 3 TeV, R=1 jets
ρ ~ Rescaled mass2
(i.e. the QCD variable)
Start with “plain” jet mass
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013
mEW
!/"
d"
/ d
!
! = m2/(pt2 R2)
quark jets (Pythia 6 MC)
m [GeV], for pt = 3 TeV, R=1
Jets: C
/A w
ith R
=1. M
C: P
ythia
6.4
, DW
tune, p
arto
n-le
vel (n
o M
PI), q
q#
qq, p
t > 3
TeV
plain jet mass
0
0.1
0.2
0.3
10-6 10-4 0.01 0.1 1
10 100 1000
12
Quark and gluonjets are different,so we treat themseparately
Start with “plain” jet mass
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013
mEW
13
!/"
d"
/ d
!
! = m2/(pt2 R2)
gluon jets (Pythia 6 MC)
m [GeV], for pt = 3 TeV, R=1
Jets: C
/A w
ith R
=1. M
C: P
ythia
6.4
, DW
tune, p
arto
n-le
vel (n
o M
PI), q
q#
qq, p
t > 3
TeV
plain jet mass
0
0.1
0.2
0.3
10-6 10-4 0.01 0.1 1
10 100 1000
Quark and gluonjets are different,so we treat themseparately
Start with “plain” jet mass
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013 14
!/"
d"
/ d
!
! = m2/(pt2 R2)
quark jets (Pythia 6 MC)
m [GeV], for pt = 3 TeV, R=1
Jets: C
/A w
ith R
=1. M
C: P
ythia
6.4
, DW
tune, p
arto
n-le
vel (n
o M
PI), q
q#
qq, p
t > 3
TeV
plain jet mass
Trimmer (zcut=0.05, Rsub=0.3)
Pruner (zcut=0.1)
MDT (ycut=0.09, µ=0.67)
0
0.1
0.2
0.3
10-6 10-4 0.01 0.1 1
10 100 1000
Different taggerscan be
quite similar
Now examine “taggers/groomers”
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013 15
!/"
d"
/ d
!
! = m2/(pt2 R2)
quark jets (Pythia 6 MC)
m [GeV], for pt = 3 TeV, R=1
Jets: C
/A w
ith R
=1. M
C: P
ythia
6.4
, DW
tune, p
arto
n-le
vel (n
o M
PI), q
q#
qq, p
t > 3
TeV
plain jet mass
Trimmer (zcut=0.05, Rsub=0.3)
Pruner (zcut=0.1)
MDT (ycut=0.09, µ=0.67)
0
0.1
0.2
0.3
10-6 10-4 0.01 0.1 1
10 100 1000
But only for a limited range
of masses
Now examine “taggers/groomers”
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013 16
!/"
d"
/ d
!
! = m2/(pt2 R2)
quark jets (Pythia 6 MC)
m [GeV], for pt = 3 TeV, R=1
Jets: C
/A w
ith R
=1. M
C: P
ythia
6.4
, DW
tune, p
arto
n-le
vel (n
o M
PI), q
q#
qq, p
t > 3
TeV
Trimmer (zcut=0.05, Rsub=0.3)
0
0.1
0.2
0.3
10-6 10-4 0.01 0.1 1
10 100 1000
What do we want to find out?
Where exactly are the kinks? How do their locations depend
on zcut, Rsub?Kinks are especially dangerous for data-driver backgrounds
What physics is relevant in the different regions?
Because then you have an idea of how well you
control itAnd maybe you can make better taggers
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013
The parameters & approximations
17
TrimmingTake all particles in a
jet of radius R and recluster them into subjets with a jet
definition with radius Rsub < R
The subjets that satisfy the condition
pt(subjet) > zcut pt(jet) are kept and merged to
form the trimmed jet.
Krohn, Thaler & Wang ’09
Our approximations
• ρ ≪ 1logs of ρ get resummed
• pretend R ≪ 1• zcut ≪ 1,
but (log zcut) not large
These approximations are not as “wild”as they might sound.
They can also be relaxed. But our aim for now is to
understand the taggers — we leave highest precision
calculations till later.
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013
Leading Order — 2-body kinematic plane
18
At O(αs), a quark jet emits a gluon. We study thisas a function of the gluon momentum fraction zand the quark-gluon opening angle θ
z
sub
Rsub
(1!z)
R
!
R
0.01
0.1
1 0.1 1
both particles in 1 subjet 2 subjets
z
�qgRsub
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013
Leading Order — 2-body kinematic plane
19
z
sub
Rsub
(1!z)
R
!
R
0.01
0.1
1 0.1 1
both particles in 1 subjet 2 subjets
z
�qgRsub
zcut
trimmed away
At O(αs), a quark jet emits a gluon. We study thisas a function of the gluon momentum fraction zand the quark-gluon opening angle θ
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013 20
0.01
0.1
1 0.1 1
both particles in 1 subjet 2 subjets
z
�qgRsub
zcut
trimmed away
↵sCF
⇡
d✓2
✓2dz
z
matrix element
emission probability ~ constantin log θ – log z plane
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013 21
0.01
0.1
1 0.1 1
both particles in 1 subjet 2 subjets
z
�qgRsub
zcut
� = 0.200
trimmed away
jet mass↵sCF
⇡
d✓2
✓2dz
z
matrix element
emission probability ~ constantin log θ – log z plane
length of fixed-ρ contour givesLO differential cross section
⇢ = z(1� z)✓2
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013 22
0.01
0.1
1 0.1 1
both particles in 1 subjet 2 subjets
z
�qgRsub
zcut
� = 0.200
trimmed away
jet mass↵sCF
⇡
d✓2
✓2dz
z
matrix element
emission probability ~ constantin log θ – log z plane
length of fixed-ρ contour givesLO differential cross section
⇢ = z(1� z)✓2
!/"
d"
/ d
!
! = m2/(pt2 R2)
trimmed quark jets: LO
m [GeV], for pt = 3 TeV, R=1
0
0.1
0.2
10-6 10-4 0.01 0.1 1
10 100 1000
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013 23
0.01
0.1
1 0.1 1
both particles in 1 subjet 2 subjets
z
�qgRsub
zcut
� = 0.150
trimmed away
jet mass↵sCF
⇡
d✓2
✓2dz
z
matrix element
emission probability ~ constantin log θ – log z plane
length of fixed-ρ contour ~LO differential cross section
⇢ = z(1� z)✓2
!/"
d"
/ d
!
! = m2/(pt2 R2)
trimmed quark jets: LO
m [GeV], for pt = 3 TeV, R=1
0
0.1
0.2
10-6 10-4 0.01 0.1 1
10 100 1000
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013 24
0.01
0.1
1 0.1 1
both particles in 1 subjet 2 subjets
z
�qgRsub
zcut
� = 0.100
trimmed away
jet mass↵sCF
⇡
d✓2
✓2dz
z
matrix element
emission probability ~ constantin log θ – log z plane
length of fixed-ρ contour ~LO differential cross section
⇢ = z(1� z)✓2
!/"
d"
/ d
!
! = m2/(pt2 R2)
trimmed quark jets: LO
m [GeV], for pt = 3 TeV, R=1
0
0.1
0.2
10-6 10-4 0.01 0.1 1
10 100 1000
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013 25
0.01
0.1
1 0.1 1
both particles in 1 subjet 2 subjets
z
�qgRsub
zcut
� = 0.030
trimmed away
jet mass↵sCF
⇡
d✓2
✓2dz
z
matrix element
emission probability ~ constantin log θ – log z plane
length of fixed-ρ contour ~LO differential cross section
⇢ = z(1� z)✓2
!/"
d"
/ d
!
! = m2/(pt2 R2)
trimmed quark jets: LO
m [GeV], for pt = 3 TeV, R=1
0
0.1
0.2
10-6 10-4 0.01 0.1 1
10 100 1000
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013 26
0.01
0.1
1 0.1 1
both particles in 1 subjet 2 subjets
z
�qgRsub
zcut
� = 0.009
trimmed away
jet mass↵sCF
⇡
d✓2
✓2dz
z
matrix element
emission probability ~ constantin log θ – log z plane
length of fixed-ρ contour ~LO differential cross section
⇢ = z(1� z)✓2
!/"
d"
/ d
!
! = m2/(pt2 R2)
trimmed quark jets: LO
m [GeV], for pt = 3 TeV, R=1
0
0.1
0.2
10-6 10-4 0.01 0.1 1
10 100 1000
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013 27
0.01
0.1
1 0.1 1
both particles in 1 subjet 2 subjets
z
�qgRsub
zcut
� = 0.003
trimmed away
jet mass↵sCF
⇡
d✓2
✓2dz
z
matrix element
emission probability ~ constantin log θ – log z plane
length of fixed-ρ contour ~LO differential cross section
⇢ = z(1� z)✓2
!/"
d"
/ d
!
! = m2/(pt2 R2)
trimmed quark jets: LO
m [GeV], for pt = 3 TeV, R=1
0
0.1
0.2
10-6 10-4 0.01 0.1 1
10 100 1000
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013 28
0.01
0.1
1 0.1 1
both particles in 1 subjet 2 subjets
z
�qgRsub
zcut
� = 0.001
trimmed away
jet mass↵sCF
⇡
d✓2
✓2dz
z
matrix element
emission probability ~ constantin log θ – log z plane
length of fixed-ρ contour ~LO differential cross section
⇢ = z(1� z)✓2
!/"
d"
/ d
!
! = m2/(pt2 R2)
trimmed quark jets: LO
m [GeV], for pt = 3 TeV, R=1
0
0.1
0.2
10-6 10-4 0.01 0.1 1
10 100 1000
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013 29
↵sCF
⇡
✓ln
r2
⇢� 3
4
◆
↵sCF
⇡
✓ln
1
zcut� 3
4
◆
↵sCF
⇡
✓ln
1
⇢� 3
4
◆
!/"
d"
/ d
!
! = m2/(pt2 R2)
trimmed quark jets: LO
m [GeV], for pt = 3 TeV, R=1
0
0.1
0.2
10-6 10-4 0.01 0.1 1
10 100 1000
zcut
r2zcut
r =Rsub
R
Trimming at LO in αs
⇢
�
d�(trim,LO)
d⇢=
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013 30
continue with all-orderresummation of terms
↵ns lnm ⇢
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013
→ all orders in αs
31
QCD pattern of multiple
soft/collinear emission Establish which
simplifying approximations
to use for tagger & matrix
elements
Inputs
Analysis of taggers’
behaviour for 1, 2, 3, … n,emissions
Output
approx. formula for
tagger’s mass distribution for
ρ ≪ 1
keeping only terms with largest powers of ln ρ,
e.g. m = 2n, 2n-1
⇢
�
d�
d⇢=
1X
n=1
cnm ↵ns lnm ⇢
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013
Trimming at all orders
32
Trimming
⇢trim(k1, k2, . . . kn) 'nX
i
⇢trim(ki)
⇠ max
i{⇢trim(ki)}
Trimmed jet reduces (~) to sum of trimmed emissions
Matrix element
X
n
1
n!
nY
i
d✓2i✓2i
dzizi
↵s(✓izipjett )CF
⇡
can use QED-like independent emissions, as if gluons don’t split
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013
Trimming at all orders
33
!/"
d"
/ d
!
! = m2/(pt2 R2)
trimmed quark jets: LO
m [GeV], for pt = 3 TeV, R=1
0
0.1
0.2
10-6 10-4 0.01 0.1 1
10 100 1000
LO
d�trim,resum
d⇢=
d�trim,LO
d⇢
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013
Trimming at all orders
34
d�trim,resum
d⇢=
d�trim,LO
d⇢exp
�Z
⇢d⇢0
1
�
d�trim,LO
d⇢0
�
!/"
d"
/ d
!
! = m2/(pt2 R2)
trimmed quark jets
m [GeV], for pt = 3 TeV, R=1
0
0.1
0.2
10-6 10-4 0.01 0.1 1
10 100 1000
LO
Resummed(fixed coupling)
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013
Trimming at all orders
35
d�trim,resum
d⇢=
d�trim,LO
d⇢exp
�Z
⇢d⇢0
1
�
d�trim,LO
d⇢0
�
!/"
d"
/ d
!
! = m2/(pt2 R2)
trimmed quark jets
m [GeV], for pt = 3 TeV, R=1
0
0.1
0.2
10-6 10-4 0.01 0.1 1
10 100 1000
LO
Resummed(fixed coupling)
0.01
0.1
1 0.1 1
both particles in 1 subjet 2 subjets
z
�qgRsub
zcut
� = 0.030
trimmed away
VETO
Sudakov
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013
Trimming at all orders
36
d�trim,resum
d⇢=
d�trim,LO
d⇢exp
�Z
⇢d⇢0
1
�
d�trim,LO
d⇢0
�
!/"
d"
/ d
!
! = m2/(pt2 R2)
trimmed quark jets
m [GeV], for pt = 3 TeV, R=1
0
0.1
0.2
10-6 10-4 0.01 0.1 1
10 100 1000
LO
Resummed(fixed coupling)
0.01
0.1
1 0.1 1
both particles in 1 subjet 2 subjets
z
�qgRsub
zcut
� = 0.009
trimmed away
VETO
Sudakov
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013
Trimming at all orders
37
d�trim,resum
d⇢=
d�trim,LO
d⇢exp
�Z
⇢d⇢0
1
�
d�trim,LO
d⇢0
�
!/"
d"
/ d
!
! = m2/(pt2 R2)
trimmed quark jets
m [GeV], for pt = 3 TeV, R=1
0
0.1
0.2
10-6 10-4 0.01 0.1 1
10 100 1000
LO
Resummed(fixed coupling)
0.01
0.1
1 0.1 1
both particles in 1 subjet 2 subjets
z
�qgRsub
zcut
� = 0.003
trimmed away
VETO
Sudakov
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013
Trimming at all orders
38
d�trim,resum
d⇢=
d�trim,LO
d⇢exp
�Z
⇢d⇢0
1
�
d�trim,LO
d⇢0
�
!/"
d"
/ d
!
! = m2/(pt2 R2)
trimmed quark jets
m [GeV], for pt = 3 TeV, R=1
0
0.1
0.2
10-6 10-4 0.01 0.1 1
10 100 1000
LO
Resummed(fixed coupling)
0.01
0.1
1 0.1 1
both particles in 1 subjet 2 subjets
z
�qgRsub
zcut
� = 0.001
trimmed away
VETO
Sudakov
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013
Trimming at all orders
39
d�trim,resum
d⇢=
d�trim,LO
d⇢exp
�Z
⇢d⇢0
1
�
d�trim,LO
d⇢0
�
Resummed(fixed coupling)
!/"
d"
/ d
!
! = m2/(pt2 R2)
trimmed quark jets
m [GeV], for pt = 3 TeV, R=1
0
0.1
0.2
10-6 10-4 0.01 0.1 1
10 100 1000
Resummed(running coupling) Full resummation also
needs treatment of running coupling
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013
Trimming: MC v. analytics
40
!/"
d"
/ d
!
! = m2/(pt2 R2)
Analytic Calculation: quark jets
m [GeV], for pt = 3 TeV, R = 1
Trimming
Rsub=0.3, zcut=0.05
Rsub=0.3, zcut=0.1
0
0.05
0.1
0.15
0.2
0.25
0.3
10-6 10-4 0.01 0.1 1
10 100 1000
!/"
d"
/ d
!
! = m2/(pt2 R2)
Pythia 6 MC: quark jets
m [GeV], for pt = 3 TeV, R = 1
Trimming
Rsub = 0.3, zcut = 0.05
Rsub = 0.3, zcut = 0.1
0
0.05
0.1
0.15
0.2
0.25
0.3
10-6 10-4 0.01 0.1 1
10 100 1000
Monte Carlo Analytic
quark jets
Non-trivial agreement!(also for dependence on parameters)
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013
Trimming: MC v. analytics
41
!/"
d"
/ d
!
! = m2/(pt2 R2)
Analytic Calculation: gluon jets
m [GeV], for pt = 3 TeV, R = 1
Trimming
Rsub=0.3, zcut=0.05
Rsub=0.3, zcut=0.1
0
0.05
0.1
0.15
0.2
0.25
0.3
10-6 10-4 0.01 0.1 1
10 100 1000
!/"
d"
/ d
!
! = m2/(pt2 R2)
Pythia 6 MC: gluon jets
m [GeV], for pt = 3 TeV, R = 1
Trimming
Rsub = 0.3, zcut = 0.05
Rsub = 0.3, zcut = 0.1
0
0.05
0.1
0.15
0.2
0.25
0.3
10-6 10-4 0.01 0.1 1
10 100 1000
Monte Carlo Analytic
gluon jets
Non-trivial agreement!(also for dependence on parameters)
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013
What logs, what accuracy?
42
⌃(⇢) =
Z ⇢
0d⇢0
1
�
d�
d⇢0Theorists state accuracy for the “cumulant” Σ(ρ):
Trimming’s leading logs (LL, in Σ) are:
We also have next-to-leading logs (NLL):
↵sL2, ↵2
sL4, .... I.e. ↵n
sL2n↵n
sL2n↵n
sL2n Just like the
jet mass
↵nsL
2n�1↵nsL
2n�1↵nsL
2n�1
Use shorthand L = log 1/ρ
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013
What logs, what accuracy?
42
⌃(⇢) =
Z ⇢
0d⇢0
1
�
d�
d⇢0Theorists state accuracy for the “cumulant” Σ(ρ):
Trimming’s leading logs (LL, in Σ) are:
We also have next-to-leading logs (NLL):
↵sL2, ↵2
sL4, .... I.e. ↵n
sL2n↵n
sL2n↵n
sL2n Just like the
jet mass
↵nsL
2n�1↵nsL
2n�1↵nsL
2n�1
Use shorthand L = log 1/ρ
Could we do better? Yes: NLL in ln Σ:
Trimmed mass is like plain jet mass (with R → Rsub), and this accuracy involves non-global logs, clustering logs
ln⌃: ↵nsL
n+1 and ↵nsL
n
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013 43
Everything so far was at parton levelAre partons sufficient?
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013
mEW
44
!/"
d"
/ d
!
! = m2/(pt2 R2)
trimming: hadronisation (quark jets)
m [GeV], for pt = 3 TeV, R=1
Pyth
ia 6
DW
, C/A
R =
1, R
sub =
0.3
, zcu
t = 0
.05
parton level
hadron level (no UE)
hadron level (with UE)
0
0.1
0.2
0.3
0.4
10-6 10-4 0.01 0.1 1
10 100 1000
hadronisation adds roughly
to the trimmed-jet squared mass
�m2 ⇠ µNP pjett Rsub
⇠ (30GeV)2
non-perturbative QCD important for EW-scale
phenomenology...
It’s even worse for plain jet massbut better for other taggers...
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013
Comments Past years → a vast trove of ideas for jet substructure tagging.
But maybe it’s time to try to go back to “basics” → detailed understanding about how our methods work.
Trimming was a particularly illustrative case:
• has non-trivial structure, relevant for phenomenology
• can mostly be understood from LO calculation & standard resummation techniques — quite similar to jet mass
• non-perturbative effects are relevant
Now over to Simone, who will discuss pruning and MDT
45
46
EXTRAS
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013
Trimming v. jet pt
47
!/"
d"
/ d
!
! = m2/(pt2 R2)
trimming: hadronisation (quark jets)
m [GeV], for pt = 3.0 TeV, R = 1
Pyth
ia 6
DW
, C/A
R =
1, R
sub =
0.3
, zcu
t = 0
.05
parton level
hadron level (no UE)
hadron level (with UE)
0
0.1
0.2
0.3
0.4
10-6 10-4 0.01 0.1 1
10 100 1000
EW
3000 GeV
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013
Trimming v. jet pt
48
!/"
d"
/ d
!
! = m2/(pt2 R2)
trimming: hadronisation (quark jets)
m [GeV], for pt = 2.0 TeV, R = 1
Pyth
ia 6
DW
, C/A
R =
1, R
sub =
0.3
, zcu
t = 0
.05
parton level
hadron level (no UE)
hadron level (with UE)
0
0.1
0.2
0.3
0.4
10-6 10-4 0.01 0.1 1
10 100 1000
EW
2000 GeV
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013
Trimming v. jet pt
49
!/"
d"
/ d
!
! = m2/(pt2 R2)
trimming: hadronisation (quark jets)
m [GeV], for pt = 1.3 TeV, R = 1
Pyth
ia 6
DW
, C/A
R =
1, R
sub =
0.3
, zcu
t = 0
.05
parton level
hadron level (no UE)
hadron level (with UE)
0
0.1
0.2
0.3
0.4
10-6 10-4 0.01 0.1 1
10 100 1000
EW
1300 GeV
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013
Trimming v. jet pt
50
!/"
d"
/ d
!
! = m2/(pt2 R2)
trimming: hadronisation (quark jets)
m [GeV], for pt = 0.8 TeV, R = 1
Pyth
ia 6
DW
, C/A
R =
1, R
sub =
0.3
, zcu
t = 0
.05
parton level
hadron level (no UE)
hadron level (with UE)
0
0.1
0.2
0.3
0.4
10-6 10-4 0.01 0.1 1
1 10 100
EW
800 GeV
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013
Trimming v. jet pt
51
!/"
d"
/ d
!
! = m2/(pt2 R2)
trimming: hadronisation (quark jets)
m [GeV], for pt = 0.5 TeV, R = 1
Pyth
ia 6
DW
, C/A
R =
1, R
sub =
0.3
, zcu
t = 0
.05
parton level
hadron level (no UE)
hadron level (with UE)
0
0.1
0.2
0.3
0.4
10-6 10-4 0.01 0.1 1
1 10 100
EW
500 GeV
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013
Trimming v. jet pt
52
!/"
d"
/ d
!
! = m2/(pt2 R2)
trimming: hadronisation (quark jets)
m [GeV], for pt = 0.3 TeV, R = 1
Pyth
ia 6
DW
, C/A
R =
1, R
sub =
0.3
, zcu
t = 0
.05
parton level
hadron level (no UE)
hadron level (with UE)
0
0.1
0.2
0.3
0.4
10-6 10-4 0.01 0.1 1
1 10 100
EW
300 GeV
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013
cuts on N-subjettiness, etc.?
• These cuts are nearly always for a jet whose mass is somehow groomed. All the structure from the grooming persists.
• So tagging & shape must probably be calculated together
53
!/"
d"
/ d
!
! = m2/(pt2 R2)
trimming & #21 cut (MC quark jets)
m [GeV], for pt = 3 TeV, R=1
Pyth
ia 6
DW
, C/A
R =
1, R
sub =
0.2
, zcu
t = 0
.1
Trimmed
Trimmed + #21$=1, kt axes < 0.3
0
0.1
0.2
10-6 10-4 0.01 0.1 1
10 100 1000
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013
kinematic plane and jet masses
54
Figure 2. Lund diagrams [45] representemission kinematics in terms of two vari-ables: vertically, the logarithm of an emis-sion’s transverse momentum kt with respectto the jet axis, and horizontally, the loga-rithm of the inverse of the emission’s angle !with respect to the jet axis, i.e. its rapiditywith respect to the jet axis. Here the dia-gram shows a line of constant jet mass, to-gether with a shaded region corresponding tothe part of the kinematic plane where emis-sions are vetoed, leading to a Sudakov formfactor.
jet m
ass
θln zln kt
ln 1/θ
regionsoft collinear
smallangles
largeangles
Lundkinematicdiagram
~
y ~
hard collinear region
line o
f con
stant
soft large−angle region
Let us define
D(") =
! 1
!
d"!
"!
! 1
!!dz pgq(z)
#s(z"!R2p2t )CF
$, (3.1a)
! #sCF
$
"
1
2ln2
1
"" 3
4ln
1
"+O (1)
#
, (fixed coupling approx.) , (3.1b)
where pgq =1+(1"z)2
2z is the quark-gluon splitting function, stripped of its colour factor, and
the fixed-coupling approximation in the second line helps visualise the double-logarithmic
structure of D(").
To NLL accuracy,3 i.e. control of terms #nsL
n+1 and #nsL
n in ln!("), where L # ln 1! ,
the integrated jet mass distribution is given by
!(") = e"D(!) · e""ED!(!)
"(1 +D!("))· N (") . (3.2)
The first factor, which is double logarithmic, accounts for the Sudakov suppression of
emissions that would induce a (squared, normalised) jet mass greater than ". In terms of
the “Lund” representation of the kinematic plane [45], Fig. 2, it accounts for the probability
of there being no emissions in the shaded region, with the 12 ln
2 1/" term in Eq. (3.1b) for
D(") coming from the bulk of the area (soft divergence of pgq), while the "34 ln 1/" term
comes from the hard collinear region (finite z). The second factor in Eq. (3.2), defined in
terms of D!(") # %LD, encodes the single-logarithmic corrections associated with the fact
that the e#ects of multiple emissions add together to give the jet’s overall mass. These
emissions tend to be close to the constant-jet-mass boundary in Fig. 2. The third factor,
3Which requires the coupling in Eq. (3.1) to run with a two-loop !-function, and to be evaluated in the
CMW scheme [46], or equivalently taking into account the two-loop cusp anomalous dimension.
– 6 –
for QCD emissions
log of 1/(emission angle)
log of transverse
momentumof emission wrt jet axis
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013
kinematic plane and jet masses
55
Figure 2. Lund diagrams [45] representemission kinematics in terms of two vari-ables: vertically, the logarithm of an emis-sion’s transverse momentum kt with respectto the jet axis, and horizontally, the loga-rithm of the inverse of the emission’s angle !with respect to the jet axis, i.e. its rapiditywith respect to the jet axis. Here the dia-gram shows a line of constant jet mass, to-gether with a shaded region corresponding tothe part of the kinematic plane where emis-sions are vetoed, leading to a Sudakov formfactor.
jet m
ass
θln zln kt
ln 1/θ
regionsoft collinear
smallangles
largeangles
Lundkinematicdiagram
~
y ~
hard collinear region
line o
f con
stant
soft large−angle region
Let us define
D(") =
! 1
!
d"!
"!
! 1
!!dz pgq(z)
#s(z"!R2p2t )CF
$, (3.1a)
! #sCF
$
"
1
2ln2
1
"" 3
4ln
1
"+O (1)
#
, (fixed coupling approx.) , (3.1b)
where pgq =1+(1"z)2
2z is the quark-gluon splitting function, stripped of its colour factor, and
the fixed-coupling approximation in the second line helps visualise the double-logarithmic
structure of D(").
To NLL accuracy,3 i.e. control of terms #nsL
n+1 and #nsL
n in ln!("), where L # ln 1! ,
the integrated jet mass distribution is given by
!(") = e"D(!) · e""ED!(!)
"(1 +D!("))· N (") . (3.2)
The first factor, which is double logarithmic, accounts for the Sudakov suppression of
emissions that would induce a (squared, normalised) jet mass greater than ". In terms of
the “Lund” representation of the kinematic plane [45], Fig. 2, it accounts for the probability
of there being no emissions in the shaded region, with the 12 ln
2 1/" term in Eq. (3.1b) for
D(") coming from the bulk of the area (soft divergence of pgq), while the "34 ln 1/" term
comes from the hard collinear region (finite z). The second factor in Eq. (3.2), defined in
terms of D!(") # %LD, encodes the single-logarithmic corrections associated with the fact
that the e#ects of multiple emissions add together to give the jet’s overall mass. These
emissions tend to be close to the constant-jet-mass boundary in Fig. 2. The third factor,
3Which requires the coupling in Eq. (3.1) to run with a two-loop !-function, and to be evaluated in the
CMW scheme [46], or equivalently taking into account the two-loop cusp anomalous dimension.
– 6 –
!/"
d"
/ d
!
! = m2/(pt2 R2)
quark jets (Pythia 6 MC)
m [GeV], for pt = 3 TeV, R=1
Jets: C
/A w
ith R
=1. M
C: P
ythia
6.4
, DW
tune, p
arto
n-le
vel (n
o M
PI), q
q#
qq, p
t > 3
TeV
plain jet mass
0
0.1
0.2
0.3
10-6 10-4 0.01 0.1 1
10 100 1000
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013
kinematic plane and jet masses
56
Figure 2. Lund diagrams [45] representemission kinematics in terms of two vari-ables: vertically, the logarithm of an emis-sion’s transverse momentum kt with respectto the jet axis, and horizontally, the loga-rithm of the inverse of the emission’s angle !with respect to the jet axis, i.e. its rapiditywith respect to the jet axis. Here the dia-gram shows a line of constant jet mass, to-gether with a shaded region corresponding tothe part of the kinematic plane where emis-sions are vetoed, leading to a Sudakov formfactor.
jet m
ass
θln zln kt
ln 1/θ
regionsoft collinear
smallangles
largeangles
Lundkinematicdiagram
~
y ~
hard collinear region
line o
f con
stant
soft large−angle region
Let us define
D(") =
! 1
!
d"!
"!
! 1
!!dz pgq(z)
#s(z"!R2p2t )CF
$, (3.1a)
! #sCF
$
"
1
2ln2
1
"" 3
4ln
1
"+O (1)
#
, (fixed coupling approx.) , (3.1b)
where pgq =1+(1"z)2
2z is the quark-gluon splitting function, stripped of its colour factor, and
the fixed-coupling approximation in the second line helps visualise the double-logarithmic
structure of D(").
To NLL accuracy,3 i.e. control of terms #nsL
n+1 and #nsL
n in ln!("), where L # ln 1! ,
the integrated jet mass distribution is given by
!(") = e"D(!) · e""ED!(!)
"(1 +D!("))· N (") . (3.2)
The first factor, which is double logarithmic, accounts for the Sudakov suppression of
emissions that would induce a (squared, normalised) jet mass greater than ". In terms of
the “Lund” representation of the kinematic plane [45], Fig. 2, it accounts for the probability
of there being no emissions in the shaded region, with the 12 ln
2 1/" term in Eq. (3.1b) for
D(") coming from the bulk of the area (soft divergence of pgq), while the "34 ln 1/" term
comes from the hard collinear region (finite z). The second factor in Eq. (3.2), defined in
terms of D!(") # %LD, encodes the single-logarithmic corrections associated with the fact
that the e#ects of multiple emissions add together to give the jet’s overall mass. These
emissions tend to be close to the constant-jet-mass boundary in Fig. 2. The third factor,
3Which requires the coupling in Eq. (3.1) to run with a two-loop !-function, and to be evaluated in the
CMW scheme [46], or equivalently taking into account the two-loop cusp anomalous dimension.
– 6 –
!/"
d"
/ d
!
! = m2/(pt2 R2)
quark jets (Pythia 6 MC)
m [GeV], for pt = 3 TeV, R=1
Jets: C
/A w
ith R
=1. M
C: P
ythia
6.4
, DW
tune, p
arto
n-le
vel (n
o M
PI), q
q#
qq, p
t > 3
TeV
plain jet mass
0
0.1
0.2
0.3
10-6 10-4 0.01 0.1 1
10 100 1000
increase inphasespace
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013
kinematic plane and jet masses
57
Figure 2. Lund diagrams [45] representemission kinematics in terms of two vari-ables: vertically, the logarithm of an emis-sion’s transverse momentum kt with respectto the jet axis, and horizontally, the loga-rithm of the inverse of the emission’s angle !with respect to the jet axis, i.e. its rapiditywith respect to the jet axis. Here the dia-gram shows a line of constant jet mass, to-gether with a shaded region corresponding tothe part of the kinematic plane where emis-sions are vetoed, leading to a Sudakov formfactor.
jet m
ass
θln zln kt
ln 1/θ
regionsoft collinear
smallangles
largeangles
Lundkinematicdiagram
~
y ~
hard collinear region
line o
f con
stant
soft large−angle region
Let us define
D(") =
! 1
!
d"!
"!
! 1
!!dz pgq(z)
#s(z"!R2p2t )CF
$, (3.1a)
! #sCF
$
"
1
2ln2
1
"" 3
4ln
1
"+O (1)
#
, (fixed coupling approx.) , (3.1b)
where pgq =1+(1"z)2
2z is the quark-gluon splitting function, stripped of its colour factor, and
the fixed-coupling approximation in the second line helps visualise the double-logarithmic
structure of D(").
To NLL accuracy,3 i.e. control of terms #nsL
n+1 and #nsL
n in ln!("), where L # ln 1! ,
the integrated jet mass distribution is given by
!(") = e"D(!) · e""ED!(!)
"(1 +D!("))· N (") . (3.2)
The first factor, which is double logarithmic, accounts for the Sudakov suppression of
emissions that would induce a (squared, normalised) jet mass greater than ". In terms of
the “Lund” representation of the kinematic plane [45], Fig. 2, it accounts for the probability
of there being no emissions in the shaded region, with the 12 ln
2 1/" term in Eq. (3.1b) for
D(") coming from the bulk of the area (soft divergence of pgq), while the "34 ln 1/" term
comes from the hard collinear region (finite z). The second factor in Eq. (3.2), defined in
terms of D!(") # %LD, encodes the single-logarithmic corrections associated with the fact
that the e#ects of multiple emissions add together to give the jet’s overall mass. These
emissions tend to be close to the constant-jet-mass boundary in Fig. 2. The third factor,
3Which requires the coupling in Eq. (3.1) to run with a two-loop !-function, and to be evaluated in the
CMW scheme [46], or equivalently taking into account the two-loop cusp anomalous dimension.
– 6 –
!/"
d"
/ d
!
! = m2/(pt2 R2)
quark jets (Pythia 6 MC)
m [GeV], for pt = 3 TeV, R=1
Jets: C
/A w
ith R
=1. M
C: P
ythia
6.4
, DW
tune, p
arto
n-le
vel (n
o M
PI), q
q#
qq, p
t > 3
TeV
plain jet mass
0
0.1
0.2
0.3
10-6 10-4 0.01 0.1 1
10 100 1000
increase inphasespace
Sudakovsuppression
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013
Some key calculations related to jet mass
• Catani, Turnock, Trentadue & Webber, ’91: heavy-jet mass in e+e–
• Dasgupta & GPS, ‘01: hemisphere jet mass in e+e– (and DIS)
• Appleby & Seymour, ’02Delenda, Appleby, Dasgupta & Banfi ’06: impact of jet boundary
• Gehrmann, Gehrmann de Ridder, Glover ’08; Weinzierl ’08Chien & Schwartz ’10: heavy-jet mass in e+e– to higher accuracy
• Dasgupta, Khelifa-Kerfa, Marzani & Spannowsky ’12,Chien & Schwartz ’12,Jouttenus, Stewart, Tackmann, Waalewijn ’13:jet masses at hadron colliders
58
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013
Trimming
59
Take all particles in ajet of radius R and recluster them into subjets with a jet
definition with radius Rsub < R
The subjets that satisfy the condition
pt(subjet) > zcut pt(jet) are kept and merged to
form the trimmed jet.Krohn, Thaler & Wang ’09
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013
Trimming
59
Take all particles in ajet of radius R and recluster them into subjets with a jet
definition with radius Rsub < R
The subjets that satisfy the condition
pt(subjet) > zcut pt(jet) are kept and merged to
form the trimmed jet.Krohn, Thaler & Wang ’09
l < z cut r 2
l = z cut
r 2
= R
sub
e
Egluon = z
cut Ejet
l = z cut
ln 1/ e
Trimming
KEPT
REJ
ECTE
D
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013
Trimming
60
l < z cut r 2
l = z cut
r 2
= R
sub
e
Egluon = z
cut Ejet
l = z cut
ln 1/ e
Trimming
KEPT
REJ
ECTE
D!/"
d"
/ d
!
! = m2/(pt2 R2)
trimmed quark jets (Pythia 6 MC)
m [GeV], for pt = 3 TeV, R=1
Jets: C
/A w
ith R
=1. M
C: P
ythia
6.4
, DW
tune, p
arto
n-le
vel (n
o M
PI), g
g#
gg, p
t > 3
TeV 0
0.1
0.2
10-6 10-4 0.01 0.1 1
10 100 1000
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013
Trimming
61
l < z cut r 2
l = z cut
r 2
= R
sub
e
Egluon = z
cut Ejet
l = z cut
ln 1/ e
Trimming
KEPT
REJ
ECTE
D!/"
d"
/ d
!
! = m2/(pt2 R2)
trimmed quark jets (Pythia 6 MC)
m [GeV], for pt = 3 TeV, R=1
Jets: C
/A w
ith R
=1. M
C: P
ythia
6.4
, DW
tune, p
arto
n-le
vel (n
o M
PI), g
g#
gg, p
t > 3
TeV 0
0.1
0.2
10-6 10-4 0.01 0.1 1
10 100 1000
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013
Trimming
62
l < z cut r 2
l = z cut
r 2
= R
sub
e
Egluon = z
cut Ejet
l = z cut
ln 1/ e
Trimming
KEPT
REJ
ECTE
D!/"
d"
/ d
!
! = m2/(pt2 R2)
trimmed quark jets (Pythia 6 MC)
m [GeV], for pt = 3 TeV, R=1
Jets: C
/A w
ith R
=1. M
C: P
ythia
6.4
, DW
tune, p
arto
n-le
vel (n
o M
PI), g
g#
gg, p
t > 3
TeV 0
0.1
0.2
10-6 10-4 0.01 0.1 1
10 100 1000
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013
Trimming
63
l < z cut r 2
l = z cut
r 2
= R
sub
e
Egluon = z
cut Ejet
l = z cut
ln 1/ e
Trimming
KEPT
REJ
ECTE
D!/"
d"
/ d
!
! = m2/(pt2 R2)
trimmed quark jets (Pythia 6 MC)
m [GeV], for pt = 3 TeV, R=1
Jets: C
/A w
ith R
=1. M
C: P
ythia
6.4
, DW
tune, p
arto
n-le
vel (n
o M
PI), g
g#
gg, p
t > 3
TeV 0
0.1
0.2
10-6 10-4 0.01 0.1 1
10 100 1000
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013
What about actual calculations of the taggers?
Simpler More complex
mMDT > plain mass ~ trimming > Y-pruning > full pruning ≫ MDT
Dasgupta et al (full NLL, including non-global part)Chien et al (partial NNLL)Jouttenus et al (they say full NNLL; I remain to be convinced!)
LL in all cases, plus some subleading logs [NB: LL doesn’t mean the same thing in all cases!)
64
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013
Kinematic regions for different taggers
65
l < z cut r 2
l = z cut
r 2
= R
sub
e
Egluon = z
cut Ejet
l = z cut
ln 1/ e
Trimming
KEPT
REJ
ECTE
D
fatl < z cut l
fat
= zl
cut l
gluon
jet
E
E
= zcut
= zl
cut
= R
epr
une
eln 1/
Pruning
KEPTR
EJEC
TED
l cut < z
Ejet
cut
Egluon = z
cut
l = z
ln 1/e
eln
z mMDT
b
a
KEPT
REJ
ECTE
D
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013
Kinematic regions for different taggers
65
l < z cut r 2
l = z cut
r 2
= R
sub
e
Egluon = z
cut Ejet
l = z cut
ln 1/ e
Trimming
KEPT
REJ
ECTE
D
fatl < z cut l
fat
= zl
cut l
gluon
jet
E
E
= zcut
= zl
cut
= R
epr
une
eln 1/
Pruning
KEPTR
EJEC
TED
l cut < z
Ejet
cut
Egluon = z
cut
l = z
ln 1/e
eln
z mMDT
b
a
KEPT
REJ
ECTE
D
Signals live here
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013
Summary table
66
highest logs transition(s) Sudakov peak NGLs NP: m2 !
plain mass !nsL
2n — L ! 1/"!̄s yes µNP ptR
trimming !nsL
2n zcut, r2zcut L ! 1/"!̄s # 2 ln r yes µNP ptRsub
pruning !nsL
2n zcut, z2cut L ! 2.3/"!̄s yes µNP ptR
MDT !nsL
2n!1 ycut,14y
2cut, y
3cut — yes µNP ptR
Y-pruning !nsL
2n!1 zcut (Sudakov tail) yes µNP ptR
mMDT !nsL
n ycut — no µ2NP/ycut
Table 1. Table summarising the main features for the plain jet mass, the three original taggers of
our study and the two variants introduced here. In all cases, L = ln 1
!= ln R2p2
t
m2 , r = Rsub/R andthe log counting applies to the region below the smallest transition point. The transition pointsthemselves are given as " values. Sudakov peak positions are quoted for d#/dL; they are expressedin terms of !̄s $ !sCF /$ for quark jets and !̄s $ !sCA/$ for gluon jets and neglect corrections ofO (1). “NGLs” stands for non-global logarithms. The last column indicates the mass-squared belowwhich the non-perturbative (NP) region starts, with µNP parametrising the scale where perturbationtheory is deemed to break down.
9 Conclusions
In this paper we have developed an extensive analytical understanding of the action of
widely used boosted-object taggers and groomers on quark and gluon jets.
We initially intended to study three methods: trimming, pruning and the mass-drop
tagger (MDT). The lessons that we learnt there led us to introduce new variants, Y-pruning
and the modified mass-drop tagger (mMDT). The key features of the di!erent taggers are
summarised in table 1. We found, analytically, that the taggers are similar in certain
phase-space regions and di!erent in others, identified the transition points between these
regions and carried out resummations of the dominant logarithms of pt/m to all orders.
One tagger has emerged as special, mMDT, in that it eliminates all sensitivity to
the soft divergences of QCD. As a result its dominant logarithms are !nsL
n, entirely of
collinear origin. It is the first time, to our knowledge, that such a feature is observed,
and indeed all the other taggers involve terms with more logarithms than powers of !s.
One consequence of having just single, collinear logarithms is that the complex non-global
(and super-leading [57]) logarithms are absent. Another is that fixed-order calculations
have an enhanced range of validity, up to L % 1/!s rather than L % 1/"!s. The
modified mass-drop tagger is also the least a!ected by non-perturbative corrections. Finally
the parameters of the tagger can be chosen so as to ensure a mass distribution that is
nearly flat, which can facilitate the reliable identification of small signals. Also of interest
19In this context it may be beneficial to study a range of variables, such as N-subjettiness [26] and energy
correlations [32], or even combinations of observables as done in Refs [81, 82]. It is also of interest to examine
observables specifically designed to show sensitivity to colour flows, such as pull [83] and dipolarity [84],
though it is not immediately apparent that these exploit di!erences in the double logarithmic structure.
It would also, of course, be interesting to extend our analysis to other types of method such as template
tagging [85].
– 45 –
NEW
Special: only single logarithms (L = ln ρ)→ more accurately calculable
Special: better exploits signal/bkgd
differences
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013
!/"
d"
/ d
!
! = m2/(pt2 R2)
Analytic Calculation: quark jets
m [GeV], for pt = 3 TeV, R = 1
mMDT ycut=0.03
ycut=0.13
ycut=0.35 (some finite ycut)
0
0.1
0.2
10-6 10-4 0.01 0.1 1
10 100 1000
Modified Mass Drop Tagger
67
[mMDT is closest we have to a scale-invariant tagger,though exact behaviour depends on q/g fractions]
!/"
d"
/ d
!
! = m2/(pt2 R2)
Pythia 6 MC: quark jets
m [GeV], for pt = 3 TeV, R = 1
mMDT ycut=0.03
ycut=0.13
ycut=0.35
0
0.1
0.2
10-6 10-4 0.01 0.1 1
10 100 1000
Monte Carlo Analytic
quark jets
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013
Pruning
68
!/"
d"
/ d
!
! = m2/(pt2 R2)
Analytic Calculation: quark jets
m [GeV], for pt = 3 TeV, R = 1
Pruning, zcut=0.1
Y-pruning, zcut=0.1
I-pruning, zcut=0.1
0
0.1
0.2
10-6 10-4 0.01 0.1 1
10 100 1000
!/"
d"
/ d
!
! = m2/(pt2 R2)
Pythia 6 MC: quark jets
m [GeV], for pt = 3 TeV, R = 1
Pruning, zcut=0.1
Y-pruning, zcut=0.1
I-pruning, zcut=0.1
0
0.1
0.2
10-6 10-4 0.01 0.1 1
10 100 1000
Monte Carlo Analytic
quark jets
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013
Comparing MC & other tools
69
!/"
d"
/ d
!
! = m2/(pt2 R2)
LO v. Pythia showers (quark jets)
m [GeV], for pt = 3 TeV, R = 1
mMDT (ycut = 0.13)
pt,jet > 3 TeV
v6.425 (DW) virtuality orderedv6.425 (P11) pt ordered
v6.428pre (P11) pt ordered
v8.165 (4C) pt ordered
Leading Order
0
0.1
10-6 10-4 0.01 0.1 1
10 100 1000
!/"
d"
/ d
!
! = m2/(pt2 R2)
LO v. NLO v. resummation (quark jets)
m [GeV], for pt = 3 TeV, R = 1
mMDT (ycut = 0.13)
pt,jet > 3 TeV
Leading Order
Next-to-Leading Order
Resummed
0
0.1
10-6 10-4 0.01 0.1 1
10 100 1000
Gavin Salam (CERN) Towards an understanding of jet substructure Boost 2013, Flagstaff, August 2013
Performance for finding signals
70
0
0.2
0.4
0.6
0.8
1
300 500 1000 3000
tagg
ing
effic
ienc
y ε
pt,min [GeV]
W tagging efficiencies
hadron level with UE
mMDT (ycut = 0.11)
pruning (zcut=0.1)
Y-pruning (zcut=0.1)
trimming (Rsub=0.3, zcut=0.05)
Figure 17. E!ciencies for tagging hadronically-decaying W ’s, for a range of taggers/groomers,shown as a function of the W transverse momen-tum generation cut in the Monte Carlo samples(Pythia 6, DW tune). Further details are givenin the text.
It receives O (!s) corrections from gluon radiation o" the W ! qq̄! system. Monte Carlo
simulation suggests these e"ects are responsible, roughly, for a 10% reduction in the tagging
e!ciencies. Secondly, Eq. (8.9) was for unpolarized decays. By studying leptonic decays of
the W in the pp ! WZ process, one finds that the degree of polarization is pt dependent,
and the expected tree-level tagging-e!ciency ranges from about 76% at low pt to 84%
at high pt. These two e"ects explain the bulk of the modest di"erences between Fig. 17
and the result of Eq. (8.9). However, the main conclusion that one draws from Fig. 17
is that the ultimate performance of the di"erent taggers will be driven by their e"ect on
the background rather than by the fine details of their interplay with signal events. This
provides an a posteriori justification of our choice to concentrate our study on background
jets.
2
3
4
5
300 500 1000 3000
ε S / √ε
B
pt,min [GeV]
signal significance with quark bkgds
hadron level with UE
(Rsub=0.3, zcut=0.05)
mMDT (ycut = 0.11)
pruning (zcut=0.1)
Y-pruning (zcut=0.1)
trimming
2
3
4
5
300 500 1000 3000ε S
/ √ε
B
pt,min [GeV]
signal significance with gluon bkgds
hadron level with UE
(Rsub=0.3, zcut=0.05)
mMDT (ycut = 0.11)
pruning (zcut=0.1)
Y-pruning (zcut=0.1)
trimming
Figure 18. The significance obtained for tagging signal (W ’s) versus background, defined as"S/
""B, for a range of taggers/groomers, shown as a function of the transverse momentum gen-
eration cut in the Monte Carlo samples (Pythia 6, DW tune) Further details are given in thetext.
– 43 –