Revealing the Jet Substructure in a Compressed Spectrum

Revealing the Jet Substructure in a Compressed Spectrum

APCTP-Pre2015-021 IPMU15-0120 CTPU-16-09 Revealing the jet substructure in a compressed spectrum 1, 2, 1, 2, 3, Chengcheng Han ∗ and Myeonghun Park y 1Asia Pacific Center for Theoretical Physics, Pohang, 790-784, Korea 2Kavli IPMU (WPI), The University of Tokyo, Kashiwa, Chiba 277-8583, Japan 3Center for Theoretical Physics of the Universe, Institute for Basic Science (IBS), Daejeon, 34051, Korea (Dated: March 28, 2016) The physics beyond the Standard Model with parameters of the compressed spectrum is well motivated both in a theory side and with phenomenological reasons, especially related to dark matter phenomenology. In this letter, we propose a method to tag soft final state particles from a decaying process of a new particle in this parameter space. By taking a supersymmetric gluino search as an example, we demonstrate how the Large Hadron Collider experimental collaborations can improve a sensitivity in these non-trivial search regions. Introduction.|After discovering the Higgs boson at with a case of compressed mass spectrum, the Large Hadron Collider (LHC), the most important question is whether the scale of the physics beyond the ∆m ≡ mA − mB mA: (2) Standard Model (BSM) is within the coverage of the LHC. As current LHC searches have been pushing away When the mass splitting is negligible compared to the a possible energy scale of the BSM, most part of param- mass of A, most of the energy from this decay flows into eter space around O(1) TeV mass scale in various models B making each quark q; q0 too soft to be tagged as an of BSM have been ruled out. But so far existing LHC isolated jet. This type of a decay is very common in analyses lose sensitivities in the compressed spectrum re- BSM, some examples in SUSY with a gluino decaying gion where the difference of masses among new parti- into a neutralino or a heavier chargino/neutralino de- cles are negligible compared to their mass scale. Major caying into the lighter neutralino when a mass splitting difficulties in those analyses are from tagging soft par- is less than W=Z=H bosons. We should note that cur- ticles over Standard Model Quantum Chromodynamics rent collider searches do not provide satisfactory results (QCD) backgrounds. The parameter space of compresses in this case, especially in search channels of multi-jet [7] spectrum is common in various new physics scenarios. and of mono-jet+missing transverse energy (E6 T ) chan- In a supersymmetric framework (SUSY), the compressed nel [9] that barely provides limits on neutralino mass spectrum is naturally predicted by various SUSY break- around 600 GeV. Thus we introduce a method to tag ing models [1,2]. For the extra dimension models like jets from A decay with suppressing the Standard Model the Universal extra dimensional one (UED), the degen- backgrounds. To identify quarks in the above process, erate spectrum in Kaluza Klein (KK) modes is usually we propose a \fat-jet (FJ)" to capture quarks (q; q0) as a predicted and only radiative correction can give limited single clustered object. The cone size of a fat-jet will be mass difference between different KK particles [3]. From determined purely by the kinematics of a decaying pro- the phenomenological point of view, BSM with the com- cess at the leading order QCD. A distance ∆R between pressed spectrum is favored. Dark matter annihilate pro- two quarks would be, cesses in this parameter space case can easily satisfy a 1 Mqq0 relic density compatible to current observations through ∆R ≈ p ; (3) the co-annihilation process as in the bino-wino or bino- z(1 − z) pT (FJ) gluino co-annihilation region [4,5]. Due to the impor- where pT (FJ) is the total transverse momentum of (q; q0) arXiv:1507.07729v2 [hep-ph] 26 Jun 2016 tance of compressed spectrum, there have been lots of studies [6]. Unlike previously suggested analyses, we pro- (a fat-jet), z is a pT fraction of A that q obtains. In a pose a method to tag soft jets from decays of BSM par- case of a three body decay, due to a symmetric feature ticles. of (q $ q0), z ' 1=2. Mqq0 denotes an invariant mass of A fat-jet for compressed spectrum.| The event topol- q; q0. With limited data, Mqq0 will be localised around ogy of our consideration is a three-body decay channel the peak Pqq0 of an invariant mass distribution [10], where a BSM particle A decays into two quarks and an- 1 s 2 other BSM particle B, " 2 2 2 2 !# mA + mB 12mAmB 0 − Pqq = 2 1 + 2 2 2 3 (mA + mB) A ! q + q0 + B; (1) ∆m −! p ; (4) ∆m mA 2 ∗[email protected] To select signal events over backgrounds, we require a cut y [email protected] on a transverse momentum pT of a fat-jet. With pT (FJ) > 2 0.2 ∆ ∆ m= 40 0.2 m= 40 ∆ m= 100 ∆ m= 100 ∆ m= 40 (p > 40 ) ∆ m= 40 (p > 40 ) T 0.15 T 0.15 ∆ m= 100 (p > 100) ∆ m= 100 (p > 100) T Arb.Units T Arb.Units 0.1 0.1 0.05 0.05 0 0 0 0.5 1 1.5 2 2.5 3 3.5 4 0 20 40 60 80 100 120 M (GeV) ∆ R q,q' FIG. 1: We show distributions of a distance ∆R between two quarks from a gluino decay (a) and an invariant mass Mqq0 (b) using a parton level Monte Carlo (MC) simulation. Here we choose ∆m = 40; 100 GeV, solid lines with a requirement of pT (FJ) > ∆m and dotted lines without pT (FJ) requirement. p ∆m, we have ∆R . 2 from eq. (3). Thus we set a to the compressed spectrum in the region of moderate radius R of a fat-jet to 1:5 to capture two quarks from pT . To show the difference between signal fat-jets and A decay. In FIG. (1), we show a distance between two QCD fat-jets, we simulate supersymmetry gluino pair quarks from A decay and their invariant mass using a MC productions as in the previous section and Z+jet produc- simulation at a parton level. We generate SUSY gluino tions for backgrounds. Both signals and backgrounds are pair productions and their decays into two quarks and generated by Madgraph aMC@NLO [15] with PYTHIA a neutralino. The neutralino mass is fixed to 600 GeV 6.4.28 [16]. We apply ATLAS AUET2B [17, 18] tune with and gluino mass varies according to the mass difference PDF set CT6L[19]. For a detector simulation, we use ∆m. As we see, we can capture most of two quarks from Delphes v3 [20] interfaced with FastJet v3.0.6 [21] for a a gluino decay with a fat-jet radius R = 1:5 after a cut jet clustering with ATLAS detector parameters. Fat-jets on a fat-jet, pT (FJ) > ∆m. Our approach has a benefit are clustered according to Cambridge-Aachen(C/A) al- of statistical gain in a requirement on pT of an initial gorithm [22] with R = 1:5. state radiation (ISR) over mono-jet+E6 T searches. We To decontaminate a fat-jet from soft QCD corruptions, only require ISR pT as large enough for A to be boosted we implement the Mass Drop Tagger (MDT) [12] out of resulting in pT (FJ) > ∆m. various grooming techniques [12, 23, 24]. We choose a With introducing a large size jet, we have issues from parameters for MDT same as in BDRS Higgs tagger [12] soft QCD corruptions. A normal QCD jet (NLO) is ap- since our spectrums ∆m are about the similar order of proximately to the Higgs' mass. In FIG. (2) we show jet mass distribu- q tions of signal fat-jets and QCD fat-jets before and after 2 < MJ >NLO ≈ 0:2pJ R; (5) passing MDT. There is a huge overlapping in jet mass distributions between signal fat-jets and QCD fat-jets be- with a numerical factor 0.2 including colour charges [11]. fore MDT. However, after MDT procedure, the signal jet For an example with a mass splitting of ∆m = 100 GeV, clearly shows a peak around 60 GeV, and the distribution p 2 is similar to our parton level analysis in FIG. (1) while a normal QCD jet attains a mass of < MJ > ∼ 30 GeV with pT (FJ) > ∆m. But as we show in FIG. (2), due to QCD fat-jet becomes lighter. In short, our result shows underlying events, background jets become more mas- that MDT method effectively removes soft-QCD corrup- sive. To remove these additional contributions on a jet tions in \non-boosted" pT region. In addition to this dif- mass and to sort out background QCD fat-jet1, we utilize ferent shape in jet mass distributions between the signal a grooming technique and a jet substructure variable. and the background, QCD fat-jets easily fail the MDT Signal fat-jet v.s. QCD fat-jets.|We note that a sig- procedure since QCD fat-jet is characterized primarily nal fat-jet is a two-prong jet while QCD fat-jet gets most by a single dense core of energy deposits surrounded by of its energy from a single prong and obtains a volume soft radiations that is not compatible to symmetric con- by soft QCD radiations. A lot of studies have been ditions. Thus MDT itself can act as a good analysis cut. performed to distinguish two-prong jets from the nor- To increase a tagging efficiency, we use a dimensionless 2 2 2 mal jets [12{14] with focusing on large pT regions where parameter ρ = mj = pT jR to impose a cut on fat-jets.

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