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  • Open Access

Determining the spacetime structure of bottom-quark couplings to spin-zero particles

Tathagata Ghosh, Rohini Godbole, and Xerxes Tata
Phys. Rev. D 100, 015026 – Published 18 July 2019

Abstract

We present a general argument that highlights the difficulty of determining the spacetime structure of the renormalizable bottom-quark Yukawa interactions of the Standard Model Higgs boson, or for that matter of any hypothetical spin-zero particle, at high energy colliders. The essence of the argument is that, it is always possible, by chiral rotations, to transform between scalar and pseudoscalar Yukawa interactions without affecting the interactions of bottom quarks with SM gauge bosons. Since these rotations affect only the b-quark mass terms in the Standard Model Lagrangian, any differences in observables for scalar versus pseudoscalar couplings vanish when mb0, and are strongly suppressed in high energy processes involving the heavy spin-zero particle where the b quarks are typically relativistic. We show, however, that the energy dependence of, for instance, e+ebb¯X (here X denotes the spin-zero particle) close to the reaction threshold may serve to provide a distinction between the scalar versus pseudoscalar coupling at electron-positron colliders that are being proposed, provided that the Xbb¯ coupling is sizeable. We also note that while various kinematic distributions for tt¯h are indeed sensitive to the spacetime structure of the top-Yukawa coupling, for a spin-zero particle X of an arbitrary mass, the said sensitivity is lost if mXmt.

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  • Received 27 April 2019

DOI:https://doi.org/10.1103/PhysRevD.100.015026

Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. Funded by SCOAP3.

Published by the American Physical Society

Physics Subject Headings (PhySH)

Particles & Fields

Authors & Affiliations

Tathagata Ghosh1,*, Rohini Godbole2,†, and Xerxes Tata1,‡

  • 1Department of Physics and Astronomy, University of Hawaii, Honolulu, Hawaii 96822, USA
  • 2Centre for High Energy Physics, Indian Institute of Science, Bangalore, 560012, India

  • *tghosh@hawaii.edu
  • rohini@iisc.ac.in
  • tata@phys.hawaii.edu

Article Text

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Issue

Vol. 100, Iss. 1 — 1 July 2019

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  • Figure 1
    Figure 1

    Left panel: The distribution of pTh in pptt¯h production at the LHC with s=14TeV, assuming that the Lagrangian Yukawa coupling is given by its SM value for both αt=0 as well as αt=π/2. Right panel: The same distribution normalized to unity. The total cross sections for the two cases are 480.6 and 219.6 fb, respectively.

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  • Figure 2
    Figure 2

    Left panel: The distribution of pTh in ppbb¯h production at the LHC with s=14TeV, assuming that the Lagrangian Yukawa coupling is given by its SM value for both αb=0 as well as αb=π/2. Right panel: The same distribution normalized to unity. The purely electroweak contribution where the h is radiated off the virtual Z boson is significant in this case. After the ET(b)>30GeV and |η(b)|<2.5 cuts, the cross section for the case cosαb=1 and yb=0 is 37.1 fb while the corresponding total cross section is 51.4 fb. The impact of the ZZh coupling, which we assume is absent for the αb=π/2 case, is illustrated by the three histograms shown.

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  • Figure 3
    Figure 3

    The left panel shows the differential distribution of pTh produced via e+ebb¯h at an electron-positron collider with s=161GeV for αb=0 and αb=π/2. As in Fig. 2, we show three histograms for αb=0 and one for αb=π/2. The dot-dashed green histogram for αb=π/2 and the dashed red histogram for αb=0 are to be read on the right-hand scale. The same distributions, but normalized to unity, are shown in the right panel. The total cross sections for cosαb=1 and sinαb=1 cases are 17.2 and 9.75×103ab, respectively.

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  • Figure 4
    Figure 4

    Differential distributions for kinematic variables, pTX (upper left), EX (upper right), ϕ* (lower left), θbb¯ (lower right) for the process e+ebb¯X for (unpolarized initial beams) at a center-of-mass energy s=161GeV, where X is a spin-zero particle. All distributions are normalized to unity. We take mX=100GeV and the Yukawa coupling to bottom quarks ybbX=0.7.

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  • Figure 5
    Figure 5

    Cross section for e+ebb¯X process (with unpolarized beams) for cosαb=1 and sinαb=1, taking mX=100GeV and ybbX=0.7 versus x=smX2mb, including beamstrahlung effects on a linear scale (left frame). We also show the same cross section using a log scale (right frame) to show the behavior close to the threshold, x=0, along with straight lines that illustrate quadratic and cubic rise of the cross section. The inset on the left frame shows the same cross section with (solid) and without (dashed) beamstrahlung in linear scale.

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  • Figure 6
    Figure 6

    In the top panel we show the invariant mass distributions for tt¯h production at the LHC, for mh=125GeV. In the two lower panels we show invariant mass distributions for mh=250 and 400 GeV.

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