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Beyond the Higgs Boson Particle Physics at the Verge of More - PowerPoint PPT Presentation

Cluster of Excellence Precision Physics, Fundamental Interactions and Structure of Matter Beyond the Higgs Boson Particle Physics at the Verge of More Discoveries? Matthias Neubert Mainz Institute for Theoretical Physics (MITP) and PRISMA


  1. Cluster of Excellence Precision Physics, Fundamental Interactions and Structure of Matter Beyond the Higgs Boson Particle Physics at the Verge of More Discoveries? Matthias Neubert — Mainz Institute for Theoretical Physics (MITP) and PRISMA Cluster of Excellence Johannes Gutenberg University, Mainz 25 January 2016 — 54 th International Winter Meeting on Nuclear Physics, Bormio Based on collaborations with Martin Bauer (arXiv:1511:01900, 1512:06828) ERC Advanced Grant (EFT4LHC) An E ff ective Field Theory Assault on the Zeptometer Scale: Exploring the Origins of Flavor and Electroweak Symmetry Breaking

  2. Overview 1 2 3 4 Discovery of the Higgs Hints for New Physics One Leptoquark to Rule One Leptoquark to Rule Boson Them All Them All Dark matter, flavor anomalies and diboson resonances A new kind of particle Part I: Flavor anomalies Part II: Diphoton resonance S(750) 5 Outlook Matthias Neubert: Beyond the Higgs Boson 2

  3. Discovery of the Higgs boson: A new kind of particle 4 July 2012: A milestone in the history of physics Matthias Neubert: Beyond the Higgs Boson 3

  4. Discovery of the Higgs boson: A new kind of particle The Standard Model of particle physics is complete! The Higgs mechanism predicts the existence of a medium penetrating all of spacetime (like an ether) In any relativistic quantum theory a field can be excited to vibrate — the vibrations of the Higgs medium consist of Higgs bosons The Higgs discovery provides an experimental proof for the existence of the Higgs medium Matthias Neubert: Beyond the Higgs Boson 4

  5. Is it the Higgs boson of the Standard Model? Properties of the Higgs bosons: -1 -1 19.7 fb (8 TeV) + 5.1 fb (7 TeV) (stat.) σ Total uncertainty ATLAS Preliminary sys inc. ( ) m = 125 GeV σ CMS theory Combined H 1 on m = 125.36 GeV ± σ µ H = 1.00 0.14 (theory) µ ± σ p = 0.96 SM + 0.23 H → γ γ - 0.23 H tagged + 0.16 → γ γ 0.28 + - 0.11 = 1.17 µ + 0.12 = 1.12 0.24 µ ± 0.26 - - 0.08 + 0.35 H ZZ* → - 0.31 H ZZ tagged + 0.19 → + 0.40 - 0.13 = 1.46 µ 0.18 + = 1.00 0.29 µ ± - 0.34 0.11 - + 0.16 H WW* → - 0.16 + 0.17 H WW tagged → + 0.24 - 0.14 = 1.18 µ + 0.13 = 0.83 0.21 µ ± - 0.21 - 0.09 0.31 + 0.30 H b b - → + 0.24 H tagged → τ τ + 0.39 - 0.23 = 0.63 µ + 0.09 = 0.91 0.28 µ ± - 0.37 - 0.07 + 0.30 H → τ τ - 0.29 0.29 + H bb tagged → + 0.42 0.23 - = 1.44 µ + 0.16 = 0.84 0.44 µ ± - 0.37 - 0.10 + 3.6 H → µ µ - 3.6 0 0.5 1 1.5 2 + 0.5 + 3.7 - 0.7 Best fit / σ σ = -0.7 µ + 0.4 SM - 3.7 - 0.4 + 4.3 H Z → γ - 4.2 + 1.7 + 4.6 - 1.3 = 2.7 µ + 1.1 - 4.5 - 0.3 + 0.10 σ ( pp → H ) · BR( H → X ) Combined - 0.10 µ = + 0.11 + 0.15 - 0.10 = 1.18 µ 0.08 σ ( pp → H ) SM · BR( H → X ) SM + - 0.14 0.07 - Higgs couplings are Standard Model-like 1 0 1 2 3 − -1 s = 7 TeV, 4.5-4.7 fb within present experimental accuracy! Signal strength ( ) µ -1 s = 8 TeV, 20.3 fb Matthias Neubert: Beyond the Higgs Boson 5

  6. Is it the Higgs boson of the Standard Model? H “This could be the discovery of the century. Depending, of course, on how far down it goes.” Matthias Neubert: Beyond the Higgs Boson 6

  7. Is Nature natural? Matthias Neubert: Beyond the Higgs Boson 7

  8. Is Nature natural? Hierarchie problem suggested that a “natural” theory ie & of electroweak symmetry breaking should contain en& new colored particle near the weak scale & Existence of dark matter suggested that there should be new weakly interacting particles near the weak scale (WIMP miracle) Where are they? Matthias Neubert: Beyond the Higgs Boson 8

  9. Is Nature natural? Where are they? Matthias Neubert: Beyond the Higgs Boson 9

  10. Hints for New Physics Dark matter, flavor anomalies and diboson resonances

  11. On the verge of another discovery? While we have not observed any of the expected faces of new physics, there exist several tantalizing hints of effects which cannot be explained by the Standard Model • Dark matter • Neutrino masses and mixings + ??? • Anomalous magnetic moment of the muon • Various anomalies in the flavor sector • Hints for new heavy resonances from the LHC Matthias Neubert: Beyond the Higgs Boson 11

  12. Anomalies in the flavor sector ∼ 3 . 5 � ( g − 2 ) µ anomaly ∼ 3 . 5 � non-standard like-sign dimuon charge asymmetry enhanced B → D ( ⇤ ) ⌧⌫ rates ∼ 3 . 5 � suppressed branching ratio of B s → � µ + µ � ∼ 3 . 5 � ∼ 3 � tension between inclusive and exclusive determination of | V ub | ∼ 3 � tension between inclusive and exclusive determination of | V cb | anomaly in B → K ⇤ µ + µ � angular distributions 2 − 3 � SM prediction for ✏ 0 / ✏ below experimental result 2 − 3 � lepton flavor non-universality in B → K µ + µ � vs. B → Ke + e � ∼ 2 . 5 � ∼ 2 . 5 � non-zero h → ⌧ µ Wolfgang Altmannshofer (UC) Theoretical Advances in Flavor Physics January 14, 2016 18 / 34 (Wolfgang Altmannshofer, Aspen Winter Conference on Particle Physics 2016) 12

  13. Flavor anomalies: Enhanced B → D (*) τν rates 0.5 R(D*) 2 BaBar, PRL109,101802(2012) = 1.0 ∆ χ Belle, arXiv:1507.03233 0.45 LHCb, arXiv:1506.08614 Average 0.4 0.35 0.3 HFAG 0.25 Prel. EPS2015 SM prediction 2 P( ) = 55% χ 0.2 0.2 0.3 0.4 0.5 0.6 e. R(D) Semileptonic decays with tau leptons are 3.5σ higher than SM predicRon! Matthias Neubert: Beyond the Higgs Boson 13

  14. Flavor anomalies: Suppressed B s → Φ μ + μ - branching ratio LHCb 1506.08777 Branching raRo in region 1 GeV 2 < q 2 < 6 GeV 2 is 3.5σ lower than SM predicRon! Matthias Neubert: Beyond the Higgs Boson 14

  15. Flavor anomalies: B → K * μ + μ - angular distributions LHCb 1512.04442 q 2 bin Decay obs. SM pred. measurement pull B 0 → ¯ ¯ K ⇤ 0 µ + µ � [2 , 4 . 3] 0 . 81 ± 0 . 02 0 . 26 ± 0 . 19 ATLAS +2 . 9 F L B 0 → ¯ ¯ K ⇤ 0 µ + µ � [4 , 6] 0 . 74 ± 0 . 04 0 . 61 ± 0 . 06 LHCb +1 . 9 F L B 0 → ¯ ¯ K ⇤ 0 µ + µ � [4 , 6] − 0 . 33 ± 0 . 03 − 0 . 15 ± 0 . 08 LHCb − 2 . 2 S 5 B 0 → ¯ ¯ K ⇤ 0 µ + µ � P 0 [1 . 1 , 6] − 0 . 44 ± 0 . 08 − 0 . 05 ± 0 . 11 LHCb − 2 . 9 5 B 0 → ¯ ¯ K ⇤ 0 µ + µ � P 0 [4 , 6] − 0 . 77 ± 0 . 06 − 0 . 30 ± 0 . 16 LHCb − 2 . 8 5 10 7 d BR B � → K ⇤� µ + µ � [4 , 6] 0 . 54 ± 0 . 08 0 . 26 ± 0 . 10 LHCb +2 . 1 dq 2 B 0 → ¯ ¯ 10 8 d BR K 0 µ + µ � [0 . 1 , 2] 2 . 71 ± 0 . 50 1 . 26 ± 0 . 56 LHCb +1 . 9 dq 2 B 0 → ¯ ¯ 10 8 d BR K 0 µ + µ � [16 , 23] 0 . 93 ± 0 . 12 0 . 37 ± 0 . 22 CDF +2 . 2 dq 2 10 7 d BR B s → � µ + µ � [1 , 6] 0 . 48 ± 0 . 06 0 . 23 ± 0 . 05 LHCb +3 . 1 dq 2 Altmannshofer, Sraub (arXiv:1503:06199) 2.8σ deviaRon in q 2 bin between [4, 6] GeV 2 (3.0σ in bin [6, 8] GeV 2 ) ! Matthias Neubert: Beyond the Higgs Boson 15

  16. Flavor anomalies: B → K μ + μ - vs. B → K e + e - LHCb 1406.6482 R K = Γ ( ¯ B ! ¯ Kµ + µ − ) Ke + e − ) = 0 . 745 +0 . 090 − 0 . 074 ± 0 . 036 Γ ( ¯ B ! ¯ 2.6σ hint for a violaRon of lepton flavor universality! Matthias Neubert: Beyond the Higgs Boson 16

  17. Flavor anomalies — reason for excitement The flavor anomalies in rare B -meson decays are: Coefficient Best fit 1 σ 3 σ Pull SM C NP − 0 . 02 [ − 0 . 04 , − 0 . 00] [ − 0 . 07 , 0 . 04] 1.1 7 • in many cases statistically significant C NP [ − 1 . 32 , − 0 . 89] [ − 1 . 71 , − 0 . 40] 4.5 − 1 . 11 9 C NP 0 . 58 [0 . 34 , 0 . 84] [ − 0 . 11 , 1 . 41] • seen by more than one experiment 2.5 10 C NP 0 . 02 [ − 0 . 01 , 0 . 04] [ − 0 . 05 , 0 . 09] 0.7 7 0 • provide a coherent picture when interpreted in C NP 0 . 49 [0 . 21 , 0 . 77] [ − 0 . 33 , 1 . 35] 1.8 9 0 terms of new physics contributions to one or two C NP − 0 . 27 [ − 0 . 46 , − 0 . 08] [ − 0 . 84 , 0 . 28] 1.4 10 0 operators in the effective weak Hamiltonian C NP = C NP − 0 . 21 [ − 0 . 40 , 0 . 00] [ − 0 . 74 , 0 . 55] 1.0 9 10 C NP = − C NP [ − 0 . 88 , − 0 . 51] [ − 1 . 27 , − 0 . 18] 4.1 − 0 . 69 9 10 C NP = − C NP [ − 1 . 28 , − 0 . 88] [ − 1 . 62 , − 0 . 42] 4.8 − 1 . 09 H e ff = � 4 G F 9 9 0 X 2 V tb V ⇤ C i O i p ts i Descotes-Genon, Hofer, Matias, Virto (arXiv:1510:04239) e 2 e 2 s � µ P L b )(¯ s � µ P R b )(¯ `� µ ` ) , `� µ ` ) , O 9 0 = O 9 = 16 ⇡ 2 (¯ 16 ⇡ 2 (¯ e 2 e 2 s � µ P L b )(¯ s � µ P R b )(¯ `� µ � 5 ` ) , `� µ � 5 ` ) O 10 0 = O 10 = 16 ⇡ 2 (¯ 16 ⇡ 2 (¯ Matthias Neubert: Beyond the Higgs Boson 17

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