Exact results for (un)safe QFT Francesco Sannino In collaboration - - PowerPoint PPT Presentation

exact results for un safe qft
SMART_READER_LITE
LIVE PREVIEW

Exact results for (un)safe QFT Francesco Sannino In collaboration - - PowerPoint PPT Presentation

Exact results for (un)safe QFT Francesco Sannino In collaboration with: Litim, 1406.2337 Intriligator 1508.07411 Bajc 1610.09681 Pelaggi, Strumia, Vigiani


slide-1
SLIDE 1

Francesco Sannino

Exact results for (un)safe QFT

In collaboration with: Litim, 1406.2337 Intriligator 1508.07411 Bajc 1610.09681 Pelaggi, Strumia, Vigiani 1701.01453

slide-2
SLIDE 2
slide-3
SLIDE 3

Gauge: SU(3) x SU(2) x U(1) at EW scale

Standard Model

Interactions: Gauge fields + fermions + scalars Yukawa: Fermion masses/Flavour Scalar self-interaction Fields: Culprit: Higgs

slide-4
SLIDE 4

Gauge - Yukawa theories

L = −1 2F 2 + iQγµDµQ + y(QLHQR + h.c.) Tr ⇥ DH†DH ⇤ − λuTr ⇥ (H†H)2⇤ − λvTr ⇥ (H†H) ⇤2

4D: standard model, dark matter, … Lower D: condensed matter, phase transitions, graphene 4D plus: extra dimensions, string theory, …

Gauge Yukawa Scalar selfinteractions

Universal description of physical phenomena

slide-5
SLIDE 5

Standard Model (blind spots)

L = −1 2F 2 + iQγµDµQ + y(QLHQR + h.c.) Tr ⇥ DH†DH ⇤ − λuTr ⇥ (H†H)2⇤ − λvTr ⇥ (H†H) ⇤2

Gauge Yukawa Scalar selfinteractions

Gauge structure is established Yukawa structure partially constrained Higgs self-coupling is not directly constrained Unsafe field theory But it does work well, so far!

slide-6
SLIDE 6

Asymptotic safety

  • 0.0

0.1 0.2 0.3 0.4 μ μ α μ

  • 0.0

0.1 0.2 0.3 0.4 μ μ α μ

ChSB/Confinement 1 GeV ~ TeV Before Planck

αs µ

Light quarks Top partners Colorons Gluino-like Unexpected

Can QCD be safe?

Sannino, 1511.09022

Pica & Sannino,1011.5917 PRD New coloured states Higgs mechanism Top

slide-7
SLIDE 7

Cosmology Cosmic rays LHC

Asymptotic safety

  • 0.0

0.1 0.2 0.3 0.4 μ μ α μ

  • 0.0

0.1 0.2 0.3 0.4 μ μ α μ

ChSB/Confinement 1 GeV ~ TeV Before Planck

αs µ

Is the safe QCD scenario testable?

Sannino, 1511.09022

Asymptotic freedom is not a must for UV complete theories

Bond, Hiller, Kowalska, Litim 1702.01727 Pelaggi, Sannino, Strumia, Vigiani 1701.01453

Model independent tests of new coloured states at the LHC Becciolini, Gillioz, Nardecchia, Sannino, Spannowsky 1403.7411, PRD

slide-8
SLIDE 8

Is the Standard Model safe?

Pelaggi, Sannino, Strumia, Vigiani 1701.01453

slide-9
SLIDE 9

Do theory like these exist?

Precise and/or nonperturbative exact results for UV interacting fixed points

slide-10
SLIDE 10

Exact 4D Interacting UV Fixed Point

Litim and Sannino, 1406.2337, JHEP

Tr ⇥ ∂H†∂H ⇤ − uTr ⇥ (H†H)2⇤ − vTr ⇥ (H†H) ⇤2

L = −F 2 + iQγ · DQ + y(QLHQR + h.c.)+

Antipin, Gillioz, Mølgaard, Sannino 1303.1525 PRD Litim, Mojaza, Sannino, 1501.03061, JHEP

slide-11
SLIDE 11

Veneziano Limit

Normalised couplings

At large N

NF NC 2 <+

v u = αv αhNF

Litim and Sannino, 1406.2337, JHEP Litim, Mojaza, Sannino, 1501.03061, JHEP

ϵ

αg βg

✏ = NF NC − 11 2

Impossible in Gauge Theories with Fermions alone Caswell, PRL 1974

slide-12
SLIDE 12

Complete asymptotic safety

Scalars are needed to make the theory fundamental

Gauge + fermion + scalars theories can be fund. at any energy scale

Litim and Sannino, 1406.2337, JHEP

Λ

slide-13
SLIDE 13

Violation of the thermal d.o.f. count

Rischke & Sannino 1505.07828, PRD

Thermal d.o.f. is violated Thermal d.o.f. conjecture

Appelquist, Cohen, Schmaltz, th/9901109 PRD

Although the thermal d.o.f. count is violated the a-theorem works!

Corrected SU(2) GB count in Sannino 0902.3494 PRD

slide-14
SLIDE 14

Gauged Higgs UV Fixed Point

Pelaggi, Sannino, Strumia, Vigiani, 1701.01453

Controllably safe in all couplings

slide-15
SLIDE 15

Supersymmetric (un)safety

Intriligator and Sannino, 1508.07413, JHEP

Exact results beyond perturbation theory

Bajc and Sannino, 1610.09681, JHEP

slide-16
SLIDE 16

Unitarity constraints

Operators belong to unitary representations of the superconf. group Dimensions have different lower bounds Gauge invariant spin zero operators Chiral primary operators have dim. D and U(1)R charge R

slide-17
SLIDE 17

Central charges

Positivity of coefficients related to the stress-energy trace anomaly ‘a(R)’ Conformal anomaly of SCFT = U(1)R ’t Hooft anomalies [proportional to the square of the dual of the Rieman Curvature] ‘c(R)’ [proportional to the square of the Weyl tensor] ‘b(R)’ [proportional to the square of the flavor symmetry field strength]

slide-18
SLIDE 18

a-theorem

For any super CFT besides positivity we also have, following Cardy ri = dim. of matter rep. +(-) for asymptotic safety (freedom) Stronger constraint for asymp. safety, since at least one large R > 5/3

slide-19
SLIDE 19

SQCD with H

W = y Tr QHe Q Nf > 3Nc

AF is lost No perturbative UV fixed point

slide-20
SLIDE 20

SQCD with H

Assume a nonperturbative fixed point, however

D(H) = 3 2R(H) = 3 Nc Nf < 1 for Nf > 3Nc

Violates the unitarity bound

D(O) ≥ 1

Potential loophole: H is free and decouples at the fixed point Check if SQCD without H has an UV fixed point

slide-21
SLIDE 21

SQCD

Unitarity bound is not sufficient

Non-abelian SQED with(out) H cannot be asymptotically safe

Can be ruled out via a-theorem

aUV−safe − aIR−safe < 0

Generalisation to several susy theories using a-maximisation*

slide-22
SLIDE 22

Super safe GUTs

Exact results

Bajc and Sannino, 1610.09681, JHEP

slide-23
SLIDE 23

Gaining R parity… but

R-symmetry from SO(10) Cartan subalgebra generator B-L M = matter parity Elegant breaking of SO(10) preserving R-parity: Introduce 126 + 126* Higgs in SO(10) 126(126*) SM and SU(5) singlet has B-L=-2(2) preserving R-parity

slide-24
SLIDE 24
  • asymp. freedom is lost

To fully break SO(10) to SM add 210 of SO(10)

In summary: 3 x 16 + 126 + 126* + 10 + 210 contributes

β1−loop = −109

Asymptotic freedom is badly lost! a, b run over generations

slide-25
SLIDE 25

Exact results

Minimal SO(10) without super potential 3 x 16 + 126 + 126* + 10 + 210 is unsafe. Minimal SO(10) with general 3-linear super potential

  • All trilinear present then: R=2/3 for all fields and no NSVZ UV fixed point
  • Eliminate one 16 from super potential passes the constraints

Exotic examples exist requiring thousands of generations! Super GUTs with R-charge are challenging!

slide-26
SLIDE 26

Higgs as shoelace

slide-27
SLIDE 27

Outlook

Extend to other (chiral) gauge theories/space-time dim

[Ebensen, Ryttov, Sannino,1512.04402 PRD, Codello, Langaeble, Litim, Sannino, JHEP 1603.03462, Mølgaard and Sannino 1610.03130]

N=1 Susy GUTs with R-parity are unlikely Go beyond P .T. [Lattice, dualities, holography, truncations] New ways to unify flavour? Models of DM and/or Inflation Challenging QCD asymptotic freedom Is there a 4D alternative to asymptotically safe gravity ?

slide-28
SLIDE 28

Backup slides

slide-29
SLIDE 29

Phenomenological Applications

slide-30
SLIDE 30

Safe QCD

slide-31
SLIDE 31

QCD

QCD is not IR conformal because Asymptotic freedom verified < TeV

Hadronic spectrum/dyn. mass Pions <-> Spont. ChSB

If above TeV asymptotic freedom is lost, then what?

slide-32
SLIDE 32

Asymptotic safety

  • 0.0

0.1 0.2 0.3 0.4 μ μ α μ

  • 0.0

0.1 0.2 0.3 0.4 μ μ α μ

ChSB/Confinement 1 GeV ~ TeV Before Planck

αs µ

New coloured states Higgs mechanism Light quarks Top Top partners Colorons Gluino-like Unexpected

Safe QCD scenario

Sannino, 1511.09022

slide-33
SLIDE 33

Cosmology Cosmic rays LHC

Asymptotic safety

  • 0.0

0.1 0.2 0.3 0.4 μ μ α μ

  • 0.0

0.1 0.2 0.3 0.4 μ μ α μ

ChSB/Confinement 1 GeV ~ TeV Before Planck

αs µ

Is the safe QCD scenario testable?

Sannino, 1511.09022

Asymptotic freedom is not a must for UV complete theories

Large Nf, QCD, Holdom 1006.2119 PLB & Pica & Sannino,1011.5917 PRD

slide-34
SLIDE 34

Safe Dark Matter

slide-35
SLIDE 35

Safe DM

σ ∝ αqαX m4

V

µ2

X X SM SM V

hσannvi / αqαX m4

V

m2

X

X X SM SM

V

Offset direct detection

Sannino & Shoemaker, 1412.8034, PRD

slide-36
SLIDE 36

Anomalous dimensions

HB = Z

1 2

HH

∆H = 1 + γH

γH = −1 2 d ln ZH d ln µ H = 4✏ 19 + 14567 − 2376 √ 23 6859 ✏2 + O(✏3)

slide-37
SLIDE 37

Mass dimensions

∆F = 3 − γF γF = d ln M d ln µ

F = 4 19✏ + 4048 √ 23 − 59711 6859 ✏2 + O(✏3)

MQQ Fermion

slide-38
SLIDE 38

Mass dimensions

Small perturb., hence m2= 0 at the UV-FP Scalar m2Tr ⇥ H†H ⇤ γ(1)

m = 2αy + 4αh + 2αv

γm = 1 2 d ln m2 d ln µ

slide-39
SLIDE 39

UV critical surface

(Ir)relevant directions implies UV lower dim. critical

`

Near the fixed point

slide-40
SLIDE 40

Double - trace and stability

Is the potential stable at FP? Which FP survives?

slide-41
SLIDE 41

Moduli

Classical moduli space Use U(Nf)xU(Nf) symmetry If V vanishes on Hc it will vanish for any multiple of it

Litim, Mojaza, Sannino 1501.03061 JHEP

slide-42
SLIDE 42

Ground state conditions at any Nf

Hc ∝ δij Hc ∝ δi1

α∗

h + α∗ v2 < 0 < α∗ h + α∗ v1

Stability for α∗

v1

slide-43
SLIDE 43

Quantum Potential

The QP obeys an exact RG equation

Hc = φcδij

γ = −1 2d ln Z/d ln µ

Litim, Mojaza, Sannino 1501.03061, JHEP

slide-44
SLIDE 44

Resumming logs

Dimensional analysis

slide-45
SLIDE 45

The Potential

Lambert Function

Effective gauge coupling

slide-46
SLIDE 46

Visualisation

0.0 0.2 0.4 0.6 0.8 1.0 1.00 1.05 1.10 1.15 ϕ/μ (ϕ) (ϕ)

NLO NNLO

0.0 0.2 0.4 0.6 0.8 1.0 0.0 0.2 0.4 0.6 0.8 1.0 ϕ/μ (ϕ) (μ)

QFT is controllably defined to arbitrary short scales

slide-47
SLIDE 47

Gauge - Yukawa theories/Gradient Flow

Relations among the modified β of different couplings Precise prescription for expanding beta functions in perturb. theory

∂˜ a ∂gi = ✓ −χij + ∂wi ∂gj − ∂wj ∂gi ◆ βj ⇒ ∂˜ a ∂gi = −βi , βi ≡ χijβj

∂βj ∂gi = ∂βi ∂gj ,

Gradient flow fundamental relation

Antipin, Gillioz, Mølgaard, Sannino 13

  • mega is an exact form

Osborn 89 & 91, Jack & Osborn 90 Jack and Poole 15