CONFORMAL SYMMETRY IN STANDARD MODEL AND GRAVITY Tomislav Prokopec, - - PowerPoint PPT Presentation

conformal symmetry in standard model and gravity
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CONFORMAL SYMMETRY IN STANDARD MODEL AND GRAVITY Tomislav Prokopec, - - PowerPoint PPT Presentation

1 CONFORMAL SYMMETRY IN STANDARD MODEL AND GRAVITY Tomislav Prokopec, ITP, Utrecht University Stefano Lucat and T. Prokopec, arXiv:1705.00889 [gr-qc]; 1709.00330 [gr-qc];1606.02677 [hep-th] T. Prokopec, Leonardo da Rocha, Michael Schmidt,


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Stefano Lucat and T. Prokopec, arXiv:1705.00889 [gr-qc]; 1709.00330 [gr-qc];1606.02677 [hep-th]

  • T. Prokopec, Leonardo da Rocha, Michael Schmidt, Bogumila Swiezewskae-Print: arXiv:1801.05258 [hep-ph] +

CONFORMAL SYMMETRY IN STANDARD MODEL AND GRAVITY

Tomislav Prokopec, ITP, Utrecht University

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Kyoto, 26-02-2018

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CONTENTS

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(7) CONCLUSIONS AND OUTLOOK (2) THEORETICAL MOTIVATION (3) WEYL SYMMETRY IN CLASSICAL GRAVITY (+ MATTER) (1) PHYSICAL MOTIVATION (4) CONFRONTING THE THEORY WITH OBSERVATIONS?

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PHYSICAL MOTIVATION

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PHYSICAL MOTIVATION

  • AT LARGE ENERGIES THE STANDARD MODEL IS

ALMOST CONFORMALLY INVARIANT.

  • OBSERVED HIGGS MASS: 𝑛𝐼 = 125.3GeV is close to the stability bound
  • HIGGS MASS AND KINETIC TERMS BREAK THE SYMMETRY
  • STABILITY BOUND: 𝑛𝐼130GeV: CAN BE ATTAINED BY ADDING SCALAR

Degrassi, Di Vita, Elias-Miro, Espinosa, Giudice, Isidori, Strumia, 1205.6497 [hep-ph]

Oleg Lebedev, e-Print: arXiv:1203.0156 [hep-ph]

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SLIDE 5

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THEORETICAL MOTIVATION

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SLIDE 6

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THEORETICAL MOTIVATION IN SM

  • HIGGS MASS TERM RESPONSIBLE FOR GAUGE HIERARCHY PROBLEM
  • IF WE COULD FORBID IT BY SYMMETRY, THE GHP WOULD BE SOLVED
  • THIS SYMMETRY COULD BE WEYL SYMMETRY IMPOSED CLASSICALLY
  • HIGGS MASS COULD BE GENERATED DYNAMICALLY BY

THE COLEMAN-WEINBERG (CW) MECHANISM

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SLIDE 7

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THEORETICAL MOTIVATION IN GRAVITY

  • THE SYMMETRY IS BROKEN BY THE NEWTON CONSTANT

AND COSMOLOGICAL TERM, G & .

  • SCALAR DILATON & CARTAN TORSION CAN RESTORE

WEYL SYMMETRY IN CLASSICAL GRAVITY.

  • G &  CAN BE GENERATED BY DILATON CONDENSATION INDUCED

BY QUANTUM EFFECTS akin to THE COLEMAN-WEINBERG MECHANISM.

  • G &  ARE RESPONSIBLE FOR GRAVITATIONAL HIERARCHY PROBLEM.
  • IF GRAVITY IS CONFORMAL IN UV, IT MAY BE FREE OF SINGULARITIES

(BOTH COSMOLOGICAL AND BLACK HOLE).

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WEYL SYMMETRY IN CLASSICAL GRAVITY

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CARTAN EINSTEIN THEORY

  • POSITS THAT FERMIONS (& SCALARS) SOURCE SPACETIME TORSION.
  • TORSION IS CLASSICALLY A CONSTRAINT FIELD

(NOT DYNAMICAL, DOES NOT PROPAGATE)  CARTAN EQUATION CAN BE INTEGRATED OUT, RESULTING IN THE KIBBLE-SCIAMA THEORY

Lucat, Prokopec, e-Print: arXiv:1512.06074 [gr-qc]

 THIS THEORY PROVIDES ADDITIONAL SOURCE TO STRESS-ENERGY, WHICH CAN CHANGE BIG-BANG SINGULARITY TO A BOUNCE.

  • CARTAN-EINSTEIN THEORY CAN BE MADE CLASSICALLY CONFORMAL!

Lucat & Prokopec, arxiv:1606.02677 [hep-th]

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SLIDE 10

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CLASSICAL WEYL SYMMETRY

  • WEYL TRANSFORMATION ON THE METRIC TENSOR
  • GENERAL CONNECTION , TORSION TENSOR T, CHRISTOFFEL CON
  • RIEMANN TENSOR IS INVARIANT: 𝜀𝑆𝛽

𝛾𝛿𝜀 = 0

  • THIS IMPLIES THAT THE VACUUM EINSTEIN EQUATION IS WEYL INV:

𝐻𝜈𝜉 = 0, 𝜀𝐻𝜈𝜉 = 0 𝜀Γ𝜈𝛽𝛾= 𝜀𝜈(𝛽𝜖𝛾)𝜄, ASSUME: ∘ 𝜀Γ𝜈𝛽𝛾= 𝜀𝜈𝛽𝜖𝛾𝜄 ⇒ 𝜀𝑈𝜈𝛽𝛾= 𝜀𝜈[𝛽𝜖𝛾]𝜄

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SLIDE 11

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GEOMETRIC VIEW OF TORSION

  • (VECTORIAL) TORSION TRACE 1-FORM:
  • WHEN A VECTOR IS PARALLEL-

TRANSPORTED, TORSION TRACE INDUCES A LENGTH CHANGE: CRUCIAL IN WHAT FOLLOWS

  • TRANSFORMS AS A VECTOR FIELD:
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PARALLEL TRANSPORT AND JACOBI EQUATION

  • JACOBI EQUATION (JACOBI FIELDS J ⊥ ሶ

𝛿) AND RAYCHAUDHURI EQ:

  • GEODESIC EQUATION:

𝛼 ሶ

𝛿 𝑒𝑦𝜈 𝑒𝜐 ≡ 𝑒𝑦𝜇 𝑒𝜐 𝛼λ 𝑒𝑦𝜈 𝑒𝜐 = 0

 TRANSFORMS MULTIPLICATIVELY (as 1/𝑒𝜐2)

𝛼 ሶ

𝛿 𝑒𝑦𝜈 𝑒𝜐 = 0 𝑓−2𝜄(𝑦)𝛼 ሶ 𝛿 𝑒𝑦𝜈 𝑒𝜐 = 0 NB: TRANSFORMATION OF 𝑒𝜐 COMPENSATED BY TRANSFORMATION OF  !

= LEVI-CIVITA

 ALSO TRANSFORMS MULTIPLICATIVELY (as 1/𝑒𝜐2) UNDER WEYL TR

  • SUGGESTS TO DEFINE A GAUGE INVARIANT PROPER TIME:

PHYSICAL TIME OF COMOVING OBSERVERS!

(𝑒𝜐)𝑕.𝑗.= exp − ׬

𝑦0 𝑦 𝑈 𝜈𝑒𝑦𝜈 𝑒𝜐 ≔

  • T. Prokopec, het Lam, e-Print: arXiv:1606.01147
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CONFORMAL SYMMETRY AND OBSERVATIONS

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CONFRONTING OBSERVATIONS

Γ

𝐹𝐺𝐺 ⊃ − ׬ 𝑒4𝑦 −𝑕 { 𝛽 𝜈 ത

𝑆2 + 𝛾(𝜈)𝜚2𝑆 +𝛿 𝜈 𝑈

𝛽𝛾 𝑈𝛽𝛾}

  • INFLATIONARY MODELS GENERATED BY CONDENSATION OF SCALARON,

DILATON OR TORSION TRACE MAY HAVE SPECIFIC FEATURES. EARLY COSMOLOGY LATE COSMOLOGY

  • PRELIMINARY RESULTS: CAN GET (quasi)de SITTER UNIVERSE AND

NEARLY SCALE INVARIANT SCALAR SPECTRUM.

  • CAN BE TESTED BY STUDYING e.g. DARK ENERGY AND STRUCTURE

FORMATION, POSSIBLY DARK MATTER CANDIDATE.

  • TORSION TRACE (AND MIXED TORSION) CAN BE DETECTED BY

CONVENTIONAL GRAVITATIONAL WAVE DETECTORS Stefano Lucat and T. Prokopec, arXiv:1705.00889 [gr-qc]

► 𝑈𝛽𝛾=TORSION (TRACE) FIELD STRENGTH

  • STRONG 1st ORDER EW PT  GW PRODUCTION & BARYOGENESIS
  • J. REZACEK, B. SWIEZEWSKA and T. PROKOPEC, in progress
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GRAVITATIONAL DETECTORS

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GRAVITATIONAL WAVES

  • GRAVITATIONAL WAVES
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DETECTORS FOR TORSION WAVES

  • TORSION TRACE

► LONGITUDINAL ► TRANSVERSE ○ DETECTOR RESPONSE ○ DETECTOR RESPONSE

  • GRAVITATIONAL WAVES vs TORSION WAVES: a comparsion

► PHASE SHIFT ¼ PERIOD ► FREQUENCY DEPENDENCE ►TORSION TRACE (L) COUPLES TO ► GW INTEFEROMETERS such as aLIGO/VIRGO

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SLIDE 18

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TORSION SOURCES

  • E.G.: TORSION TRACE: LONGITUDINAL MODE

► ITS MASS IS PROTECTED BY THE CONFORMAL WARD=TAKAHASHI, (see talk of Stefano Lucat) ► THIS IMPLIES ABOUT 1 order of magnitude suppression when compared with the amplitude of gravitational waves, i.e. ○ e=sources excentricity (can be 0.5) ► DETECTABLE BY THE NEXT GENERATION OF OBSERVATORIES such as EINSTEIN TELESCOPE.

 ℎ𝑗𝑘 ~ 𝑓2 2

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CONCLUSIONS AND OUTLOOK

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CONCLUSIONS AND OUTLOOK

  • CHALLENGE 1: USE FRG METHODS TO STUDY HOW THIS THEORY

DIFFERS FROM THE USUAL GRAVITY, i.e. WHETHER IT IS ASYMPTOTICALLY SAFE/ADMITS UV COMPLETION.

  • CHALLENGE 2: CONFRONT THIS THEORY AS MUCH AS POSSIBLE

WITH OBSERVATIONS

(𝑒𝜐)𝑕.𝑗.= exp − ׬

𝑦0 𝑦 𝑈 𝜈𝑒𝑦𝜈 𝑒𝜐 ≔

  • CHALLENGE 3: CAN WE GET RID OF (COSMOLOGICAL AND BLACK HOLE)

SINGULARITIES? HINT: RECALL: PHYSICAL TIME OF COMOVING OBSERVERS