probing kinetic mixing term of dark gauge boson at the lhc · 2019. 6. 4. · probing kinetic...

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Teruki Kamon Mitchell Institute for Fundamental Physics and Astronomy Texas A&M University Searching for Long-Lived Particles at the LHC: Fifth workshop on the LHC Long-Lived Particle (LLP) Community, (https://indico.cern.ch/event/792346/overview) CERN, 27-29 May 2019 1 May 27, 2019 Kinetic Mixing [Credits] Images of Baryon Acoustic Bscillations with Cosmic Microwave Background by E.M. Huff, the SDSS-III team, and the South Pole Telescope team. Graphic by Zosia Rostomian (Lawrence Berkeley National Laboratory) Image of Neutrino Astrophysics, taken from https://astro.desy.de/ Image of the LHC by CERN Photo Image of Bullet Cluster by NASA/ Chandra X-ray Center Probing Kinetic Mixing Term of Dark Gauge Boson at the LHC Collaboration: Mohammad Abdullah (Mitchell Institute) Bhaskar Dutta (Mitchell Institute) Teruki Kamon (CMS/Mitchell Institute) Marcus Hohlmann (CMS/FIT) Adrian Thompson (CMS/Mitchell Institute)

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  • Teruki Kamon Mitchell Institute for Fundamental Physics and Astronomy

    Texas A&M University

    Searching for Long-Lived Particles at the LHC:

    Fifth workshop on the LHC Long-Lived Particle (LLP) Community,

    (https://indico.cern.ch/event/792346/overview)

    CERN, 27-29 May 2019

    1May 27, 2019 Kinetic Mixing

    [Credits]

    Images of Baryon Acoustic Bscillations with Cosmic Microwave Background

    by E.M. Huff, the SDSS-III team, and the South Pole Telescope team. Graphic

    by Zosia Rostomian (Lawrence Berkeley National Laboratory)

    Image of Neutrino Astrophysics, taken from https://astro.desy.de/

    Image of the LHC by CERN Photo

    Image of Bullet Cluster by NASA/ Chandra X-ray Center

    Probing Kinetic Mixing Term

    of Dark Gauge Boson

    at the LHCCollaboration:

    Mohammad Abdullah (Mitchell Institute)

    Bhaskar Dutta (Mitchell Institute)

    Teruki Kamon (CMS/Mitchell Institute)

    Marcus Hohlmann (CMS/FIT)

    Adrian Thompson (CMS/Mitchell Institute)

  • A simple extension of the standard model involves adding a "dark" U(1) gauge group

    that is broken by a dark Higgs vev. The "dark vector" 𝑍𝐷 can then kinetically mix withthe 𝑈(1)𝐵 gauge boson, and the "dark Higgs" 𝑆 (or ℎ𝑆) can mix with the SM doubletHiggs via the Higgs portal |H|2|S|2 operator. This can induce a variety of exotic Higgs

    decays like:

    ℎ → 𝑍𝑍𝐷 (if kinetic mixing dominates)ℎ → 𝑍𝐷𝑍𝐷 (if higgs mixing dominates)ℎ → 𝑆𝑆 (if higgs mixing dominates)

    http://insti.physics.sunysb.edu/~curtin/hahm_mg.html

    2

    Kinetic Mixing with Dark Gauge Boson

    Note: this is not Feynman diagram

  • Kinetic Mixing by ATLAS and CMS

    3

    MC samples m(𝜸𝑫) = 0.25 –58 GeV 𝑐𝜏 = 0 –100 mm m(𝑵𝟏) = 10, 60 GeV, m(𝒏𝑫) = 1 GeV

    Unknown

    branching

    fractions

    Unknown

    branching

    fractions

  • 4

    𝑝𝑝 → ℎ → 𝑍𝑍𝑑(or 𝑎𝑎) → 4𝓁 ; 𝑝𝑝 → 𝑍𝑑 → 𝓁𝓁; 𝑝𝑝 → 𝑍 → 𝜇𝜇; 𝑍𝑑 → 4𝓁

    Other Representative Processes

    Independent of the Higgs portal

    |H|2|S|2 operator

  • 𝒁′ as ”𝜸𝒅 or 𝒁𝒅” Search FrameworkPhysics of dark gauge boson (𝜸𝑑 or 𝑍𝑑) can be studied via a framework of aspin-1 particle (𝒁′) which couples to first- and second-generation fermions.

    o Associated production with ISR jet/photon or the SM weak

    gauge boson (V = W or Z) will probe the mixing term

    independently of the Higgs portal |H|2|S|2 operator.

    o Larger signal cross sections, compared to processes with

    the Higgs boson decays.

    o [Trigger] A standard mono-jet or mono-photon or mutilepton

    trigger (w/o vertex constraint on leptons).

    o [Main backgrounds] g(photon)+𝛾∗ (𝑝𝑇(𝑔 𝑜𝑟 𝛾) > 200 GeV) or V+𝛾∗ (𝑝𝑇(𝑉) >

    20 GeV), followed by 𝛾∗ → 𝜇𝜇. But they should be suppressed by a lifetime cut. Also 𝑔∗ → 𝑏𝑏 → 𝜇𝜇 + 𝑋 (we need an isolation study.)

    5

    A basic idea on direct production is stated in “Non-Abelian

    Dark Sectors and Their Collider Signatures”, Matthew

    Baumgart, Clifford Cheung, Joshua T. Ruderman, Lian-Tao

    Wang, and Itay Yavin, JHEP 04 (2009) 014, 10.1088/1126-

    6708/2009/04/014 [arXiv:0901.0283]. See Fig. 11.

    https://arxiv.org/ct?url=https%3A%2F%2Fdx.doi.org%2F10.1088%2F1126-6708%2F2009%2F04%2F014&v=50ff5ccehttps://arxiv.org/abs/0901.0283

  • 6

    𝒁′ Associate Production Processes

    𝑝𝑇(𝑔) > 200 GeV

    𝑝𝑇(𝛾) > 200 GeV

    𝑝𝑇(𝑉) > 20 GeV

    𝑝𝑇(𝑉) > 20 GeV

    Low mass 𝑍′ could be probed by V+𝑍′, as an angular separation of leptons in highlyboosted lighter dark gauge boson may be a problem in high 𝑝𝑇(𝑔 𝑜𝑟 𝛾) trigger. For𝑝𝑇 ≳ 200 GeV, an opening angle of approximately 𝜃~ Τ𝑚𝛾′ 𝑝𝑇 < 0.00125 for M = 0.25

    GeV.

  • 7

    Kinematics in 𝒁′ Associate Production𝒑𝑻(j,𝜸) > 200 GeV or 𝒑𝑻(𝝁 from W, Z) > 20 GeV

    M = 1 GeV M = 10 GeV

    𝒑𝑻(𝝁𝝁)

    ∆𝝋(𝝁𝝁)

    𝒑𝑻(𝝁𝝁)

    ∆𝝋(𝝁𝝁)

    MadGraph+Delphes

    Adrian Thompson

    Mohammad Abdullah

    𝜃~ Τ𝑚𝛾′ 𝑝𝑇 < 0.005

    for 1 GeV mass

    𝝈∙𝑨∙ℒ

    𝝈∙𝑨∙ℒ

    𝝈∙𝑨∙ℒ

    𝝈∙𝑨∙ℒ

  • [U(1)𝐿𝜇 − 𝐿𝜏 gauge bosons] A search for Z′ in 4μ final state, PLB 792 (2019) 345, EXO

    18-008, CMS AN-17/321, arXiv:1808.03684

    [Refs: arxiv:1808.03647, arxiv:1712.10022]

    70 GeV

    Complementary Search

    + quark sectors?

    ?

    [CMS, PLB 792 (2019) 345; 1808.03684] The

    4μ analysis can set limits on 𝑔𝜇 for masses

    down to 10 GeV.

    𝒈

    The limits will depend on how many decay

    channels the Z‘ has in our model.

    There are some limits from related searches,

    but not on the same process directly.

    8

  • 9

    Summary[Complementary] The mixing term can

    be probed via associate production with

    ISR jet/photon or the SM weak gauge

    boson (V = W or Z), independently of

    the Higgs portal |H|2|S|2 operator.

    [Wide mass range] Low mass 𝑍′ can besearched using V+𝑍′ (𝑝𝑇(𝑉) > 20 GeV),as angular separation of leptons in

    highly boosted lighter dark gauge boson

    may be a problem in 𝑝𝑇 𝑔 𝑜𝑟 𝛾 > 200 −500 GeV.

    “Hunting All the Hidden Photons”, Martin

    Bauer, Patrick Foldenauer, and Joerg Jaeckel,

    JHEP 07 (2018) 094

  • BACKUP

    10

  • 11

    Cross Section and AcceptanceMadGraph+Delphes

    Adrian Thompson

    Mohammad Abdullah

  • Thinking of Direct ProductionA basic idea on direct production is stated in “Non-Abelian Dark Sectors and

    Their Collider Signatures”, Matthew Baumgart, Clifford Cheung, Joshua T.

    Ruderman, Lian-Tao Wang, and Itay Yavin, JHEP 04 (2009) 014,

    10.1088/1126-6708/2009/04/014 [arXiv:0901.0283].

    See Fig. 11. X is not specified. They envisioned to trigger those events with

    single/dimuon triggers, referring to CMS Level 1 dimuon trigger (2 muons with 𝑝𝑇 > 3GeV in |η| < 2.4) or single muon trigger (1 muon with 𝑝𝑇 > 7 GeV and |η| < 2.4). Thus𝑝𝑇 ≳ 10 GeV, resulting in an opening angle of approximately 𝜃~ Τ𝑚𝛾′ 𝑝𝑇 < 0.025 for 10

    GeV 𝑝𝑇, 0.25 GeV mass.

    12

    https://arxiv.org/ct?url=https%3A%2F%2Fdx.doi.org%2F10.1088%2F1126-6708%2F2009%2F04%2F014&v=50ff5ccehttps://arxiv.org/abs/0901.0283

  • On Decay ModesIf Gd includes SU(2)d, the decay modes are more complex.

    See Fig. 9 of “Non-Abelian Dark Sectors and Their Collider Signatures”, Matthew

    Baumgart, Clifford Cheung, Joshua T. Ruderman, Lian-Tao Wang, and Itay Yavin,

    JHEP 04 (2009) 014, 10.1088/1126-6708/2009/04/014 [arXiv:0901.0283].

    13

    https://arxiv.org/ct?url=https%3A%2F%2Fdx.doi.org%2F10.1088%2F1126-6708%2F2009%2F04%2F014&v=50ff5ccehttps://arxiv.org/abs/0901.0283

  • Probing Kinetic Mixing Term at LHC“Hunting All the Hidden Photons”, Martin Bauer, Patrick Foldenauer, and

    Joerg Jaeckel, JHEP 07 (2018) 094

    14

    Can we search at ATLAS + CMS?𝝐𝒆

    𝑴𝑨′

    Physics of dark gauge boson (𝜸𝑑 or 𝑍𝑑) can be studied via a framework of a spin-1particle (𝒁′) which couples to first- and second-generation fermions.

  • [U(1)𝑳𝝁 − 𝑳𝝉 gauge bosons] A search for Z′ in 4μ final state, PLB 792 (2019)

    345, EXO 18-008, CMS AN-17/321, arXiv:1808.03684[Refs: arxiv:1808.03647, arxiv:1712.10022]

    70 GeV

    Example: Constraints on 𝒈𝝁 on 𝒁′

    [CMS, PLB 792 (2019) 345; 1808.03684] The

    4μ analysis can set limits on 𝑔𝜇 for masses

    down to 10 GeV.

    Also see [CMS, JHEP 01 (2018)

    097;1710.00159] Z’ with AK8 jet 𝑝𝑇 > 500 GeV (against another high 𝑝𝑇 ISR jet) for leptophobic Z' that can set limits on 𝑔𝑞 down

    to 𝑚(𝑍′) = 50 GeV.

    𝒈

    15

  • 16

    “Coherent elastic neutrino nucleus scattering as a probe of a Z′ through kinetic and mass mixing

    effects” Mohammad Abdullah, James B. Dent, Bhaskar Dutta, Gordon L. Kane, Shu Liao, and

    Louis E. Strigari, Phys.Rev. D98 (2018) 015005

    𝝐𝒁 𝝐𝑩

    Connection with CEvNS