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objective minimal realization of light composite higgs
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objective: minimal realization of light composite Higgs USQCD 2015 - - PowerPoint PPT Presentation

objective: minimal realization of light composite Higgs USQCD 2015 Lattice Higgs Collaboration (L at HC) Zoltan Fodor, Kieran Holland, JK, Santanu Mondal, Daniel Nogradi, Chik Him Wong Julius Kuti University of California, San Diego USQCD


slide-1
SLIDE 1

USQCD 2015

  • bjective: minimal realization of light composite Higgs

1

Lattice Higgs Collaboration (LatHC)

Zoltan Fodor, Kieran Holland, JK, Santanu Mondal, Daniel Nogradi, Chik Him Wong

Julius Kuti University of California, San Diego

USQCD Collaboration Meeting May 1-2, 2015, Fermilab

slide-2
SLIDE 2

LHiggs → −1 4FµνFµν + i ¯ QγµDµQ + . . .

R

e-writing the Higgs doublet field H = 1 ⌦ 2 ⇤ ⇤2 + i ⇤1 ⌅ i ⇤3 ⌅

1 ⌦ 2 ⌅ + i⌦ ⇧ · ⌦ ⇤⇥ ⇧ M .

DµM = µM i g WµM + i g⌥M Bµ , with Wµ = Wa

µ

⇧a 2 , Bµ = Bµ ⇧3 2

The Higgs Lagrangian is L = 1 2Tr ⇧ DµM†DµM ⌃

  • m2

M

2 Tr ⇧ M†M ⌃ 4 Tr ⇧ M†M ⌃2

strongly coupled gauge theory Nf fermions in gauge group reps needle in the haystack?

  • r, just one of the haystacks?

spontaneous symmetry breaking Higgs mechanism

What is our composite Higgs terminology?

slide-3
SLIDE 3

Outline

Near-conformal SCGT?

light scalar close to conformal window effective theory? scale setting and spectroscopy systematics and mixed action

Chiral Higgs condensate

GMOR and mode number epsilon regime and RMT large mass anomalous dimension?

Scale dependent renormalized coupling

matching scale dependent coupling from form UV to IR with chiSB

Early universe

EW phase transition, sextet baryon, and dark matter

Summary

SCGT Theory Space close to scale invariance? nf=2 sextet rep massless fermions SU(2) doublet 3 Goldstones morph into weak bosons minimal realization

sextet rep near-conformal?

QCD intuition for near-conformal compositeness is just plain wrong Technicolor thought to be scaled up QCD motivation of the project: composite Higgs-like scalar close to the conformal window

u(+e/2 d(-e/2) ⎡ ⎣ ⎢ ⎤ ⎦ ⎥

minimal EW embedding QCD far from scale invariance

haystack

slide-4
SLIDE 4

5 10 15 20 25 −1 1 2 3 4 5 6 7 8 9 x 10

−5

t

Csinglet(t) ~ exp(-M0++·t) fitting function: Nf=12

Nf=12

Lowest 0++ scalar state from singlet correlator aM0++=0.304(18) 243x48 lattice simulation 200 gauge configs β=2.2 am=0.025

+

6 8 10 12 14 16 18 20 22 24 26 −0.5 0.5 1 1.5 2 2.5 3 x 10

−7

t

Cnon-singlet(t): Nf=12 Lowest non-singlet scalar from connected correlator aMnon-singlet = 0.420(2) !=2.2 am=0.025

C(t) = ⇤

n

  • Ane−mn(ΓS⊗ΓT)t + (−1)tBne−mn(γ4γ5ΓS⊗γ4γ5ΓT)t⇥

staggered correlator

test of scalar technology:

LatHC and LatKMI Nf=12 fundamental rep

light 0++ scalar and spectrum 2013-14 testing

slide-5
SLIDE 5

0.005 0.01 0.015 0.1 0.2 0.3 0.4 0.5 0.6

fermion mass m

triplet and singlet masses

0++ triplet state (connected) 0++ singlet state (disconnected)

From the composite Higgs mechanism: Goldstone decay constant F is setting the EWSB scale MH/F ~ 1−3 range

Triplet and singlet masses from 0

++ correlators

light 0++ scalar and spectrum sextet model LatHC

β=3.20 283x56, 323x64 m fit range 0.003 - 0.008

LatHC

circa Lattice 2013

1 TeV a1 rho

light scalar at few hundred GeV?

  • bserved Higgs-like?

EW self-energy shift

within reach of LHC Run 2 ?

t W Z

then δM2

H ⌅ 12κ2r2 t m2 t ⌅

κ2r2

t (600 GeV)2.

a0 B

near-conformal resonance spectrum separated from light scalar moving up to 2-3 TeV with refined scale setting

3 TeV

slide-6
SLIDE 6

0.005 0.01 0.015 0.1 0.2 0.3 0.4 0.5 0.6

fermion mass m

triplet and singlet masses

0++ triplet state (connected) 0++ singlet state (disconnected)

From the composite Higgs mechanism: Goldstone decay constant F is setting the EWSB scale MH/F ~ 1−3 range

Triplet and singlet masses from 0

++ correlators

light 0++ scalar and spectrum sextet model LatHC

β=3.20 283x56, 323x64 m fit range 0.003 - 0.008

LatHC

circa Lattice 2013

1 TeV a1 rho

light scalar at few hundred GeV?

  • bserved Higgs-like?

EW self-energy shift

within reach of LHC Run 2 ?

t W Z

then δM2

H ⌅ 12κ2r2 t m2 t ⌅

κ2r2

t (600 GeV)2.

a0 B

near-conformal resonance spectrum separated from light scalar moving up to 2-3 TeV with refined scale setting

3 TeV

2 4 6 8 10 12 14 −0.1 −0.05 0.05 0.1 0.15 0.2 0.25

=3.20 (with PCA analysis) 483x96 m=0.002 t effective mass of D(t) − D(T/2) MHiggs = 0.0548 ± 0.0175 2 = 0.019 Q = 1

number of blocks = 16 block size = 4 eigenvalue threshold of PCA = 0.004 error threshold of PCA = 2 fitted range = 5 − 10

2 4 6 8 10 12 14 16 −0.1 −0.05 0.05 0.1 0.15 0.2 0.25 0.3

=3.20 (with PCA analysis) 403x80 m=0.002 t effective mass of D(t) − D(T/2) MHiggs = 0.0494 ! 0.0147 2 = 0.11 Q = 0.99

number of blocks = 17 block size = 5 eigenvalue threshold of PCA = 0.004 error threshold of PCA = 2 fitted range = 4 − 10

− −

− −

− −

− −

new, preliminary new, preliminary

LatHC LatHC

slide-7
SLIDE 7

0.005 0.01 0.015 0.1 0.2 0.3 0.4 0.5 0.6

fermion mass m

triplet and singlet masses

0++ triplet state (connected) 0++ singlet state (disconnected)

From the composite Higgs mechanism: Goldstone decay constant F is setting the EWSB scale MH/F ~ 1−3 range

Triplet and singlet masses from 0

++ correlators

light 0++ scalar and spectrum sextet model LatHC

β=3.20 283x56, 323x64 m fit range 0.003 - 0.008

LatHC

circa Lattice 2013

1 TeV a1 rho

light scalar at few hundred GeV?

  • bserved Higgs-like?

EW self-energy shift

within reach of LHC Run 2 ?

t W Z

then δM2

H ⌅ 12κ2r2 t m2 t ⌅

κ2r2

t (600 GeV)2.

a0 B

near-conformal resonance spectrum separated from light scalar moving up to 2-3 TeV with refined scale setting

3 TeV

2 4 6 8 10 12 14 −0.1 −0.05 0.05 0.1 0.15 0.2 0.25

=3.20 (with PCA analysis) 483x96 m=0.002 t effective mass of D(t) − D(T/2) MHiggs = 0.0548 ± 0.0175 2 = 0.019 Q = 1

number of blocks = 16 block size = 4 eigenvalue threshold of PCA = 0.004 error threshold of PCA = 2 fitted range = 5 − 10

2 4 6 8 10 12 14 16 −0.1 −0.05 0.05 0.1 0.15 0.2 0.25 0.3

=3.20 (with PCA analysis) 403x80 m=0.002 t effective mass of D(t) − D(T/2) MHiggs = 0.0494 ! 0.0147 2 = 0.11 Q = 0.99

number of blocks = 17 block size = 5 eigenvalue threshold of PCA = 0.004 error threshold of PCA = 2 fitted range = 4 − 10

− −

− −

− −

− −

new, preliminary new, preliminary

LatHC LatHC

slide-8
SLIDE 8

0.005 0.01 0.015 0.1 0.2 0.3 0.4 0.5 0.6

fermion mass m

triplet and singlet masses

0++ triplet state (connected) 0++ singlet state (disconnected)

From the composite Higgs mechanism: Goldstone decay constant F is setting the EWSB scale MH/F ~ 1−3 range

Triplet and singlet masses from 0

++ correlators

light 0++ scalar and spectrum sextet model LatHC

β=3.20 283x56, 323x64 m fit range 0.003 - 0.008

LatHC

circa Lattice 2013

1 TeV a1 rho

light scalar at few hundred GeV?

  • bserved Higgs-like?

EW self-energy shift

within reach of LHC Run 2 ?

t W Z

then δM2

H ⌅ 12κ2r2 t m2 t ⌅

κ2r2

t (600 GeV)2.

a0 B

near-conformal resonance spectrum separated from light scalar moving up to 2-3 TeV with refined scale setting

3 TeV

2 4 6 8 10 12 14 −0.1 −0.05 0.05 0.1 0.15 0.2 0.25

=3.20 (with PCA analysis) 483x96 m=0.002 t effective mass of D(t) − D(T/2) MHiggs = 0.0548 ± 0.0175 2 = 0.019 Q = 1

number of blocks = 16 block size = 4 eigenvalue threshold of PCA = 0.004 error threshold of PCA = 2 fitted range = 5 − 10

2 4 6 8 10 12 14 16 −0.1 −0.05 0.05 0.1 0.15 0.2 0.25 0.3

=3.20 (with PCA analysis) 403x80 m=0.002 t effective mass of D(t) − D(T/2) MHiggs = 0.0494 ! 0.0147 2 = 0.11 Q = 0.99

number of blocks = 17 block size = 5 eigenvalue threshold of PCA = 0.004 error threshold of PCA = 2 fitted range = 4 − 10

− −

− −

− −

− −

new, preliminary new, preliminary

LatHC LatHC

running large volumes m fit range 0.001 - 0.002

slide-9
SLIDE 9

3.2 β 2 4 6 8 10 12 14 16 18 20 22 M / F 0.5 1 1.5 2 2.5 3 3.5 4 4.5 5 M / TeV MN Ma1 Mρ

0++ scalar Higgs?

a0 scalar isovector?

light 0++ scalar and spectrum sextet model LatHC

strong gauge dynamics

coupling to SM?

slide-10
SLIDE 10

3.2 β 2 4 6 8 10 12 14 16 18 20 22 M / F 0.5 1 1.5 2 2.5 3 3.5 4 4.5 5 M / TeV MN Ma1 Mρ

0++ scalar Higgs?

a0 scalar isovector?

light 0++ scalar and spectrum sextet model LatHC

strong gauge dynamics

partial compositeness ETC

?

coupling to SM?

slide-11
SLIDE 11

3.2 β 2 4 6 8 10 12 14 16 18 20 22 M / F 0.5 1 1.5 2 2.5 3 3.5 4 4.5 5 M / TeV MN Ma1 Mρ

0++ scalar Higgs?

a0 scalar isovector?

light 0++ scalar and spectrum sextet model LatHC

strong gauge dynamics

partial compositeness ETC

?

coupling to SM?

extended linear sigma model dilaton

}

effective theories

slide-12
SLIDE 12

EUROPEAN ORGANISATION FOR NUCLEAR RESEARCH (CERN)

Submitted to: Eur. Phys. J. C. CERN-PH-EP-2015-052 30th March 2015

Search for a new resonance decaying to a W or Z boson and a Higgs boson in the ``/`⌫/⌫⌫ + b¯ b final states with the ATLAS Detector

The ATLAS Collaboration Abstract

A search for a new resonance decaying to a W or Z boson and a Higgs boson in the ``/`⌫/⌫⌫+ b¯ b final states is performed using 20.3 fb1 of pp collision data recorded at ps = 8 TeV with the ATLAS detector at the Large Hadron Collider. The search is conducted by examining the WH/ZH invariant mass distribution for a localized excess. No significant deviation from the Standard Model background prediction is observed. The results are interpreted in terms of constraints on the Minimal Walking Technicolor model and on a simplified approach based

  • n a phenomenological Lagrangian of Heavy Vector Triplets.

light 0++ scalar and spectrum sextet model LatHC

3.2 β 2 4 6 8 10 12 14 16 18 20 22 M / F 0.5 1 1.5 2 2.5 3 3.5 4 4.5 5 M / TeV MN Ma1 Mρ

0++ scalar Higgs?

a0 scalar isovector?

slide-13
SLIDE 13

[GeV]

R1

m 400 600 800 1000 1200 1400 1600 1800 bb) [pb] → (H × ZH) →

1

BR (R × σ

  • 3

10

  • 2

10

  • 1

10 1 10

ATLAS

  • 1

L dt = 20.3 fb

= 8 TeV s

=2 g ~ ZH →

2

,R

1

MWT R =1

v

’ HVT Benchmark model A g V Observed 95% Upper Limit Expected 95% Upper Limit 1 Sigma Uncertainty ± 2 Sigma Uncertainty ±

(a) R0

1(V00) ! ZH, H ! b¯

b

[GeV]

±

R1

m 400 600 800 1000 1200 1400 1600 1800 bb) [pb] → (H × WH) →

± 1

BR (R × σ

  • 3

10

  • 2

10

  • 1

10 1 10

ATLAS

  • 1

L dt = 20.3 fb

= 8 TeV s

=2 g ~ WH →

± 2

,R

± 1

MWT R =1

v

HVT Benchmark model A g

±

V’ Observed 95% Upper Limit Expected 95% Upper Limit 1 Sigma Uncertainty ± 2 Sigma Uncertainty ±

(b) R±

1(V0±) ! WH, H ! b¯

b

[TeV]

A

m

0.5 1 1.5 2 2.5

g ~

1 2 3 4 5 6 7 8 9 10

95% CL Observed Exclusion 95% CL Expected limit Dilepton resonances 95% Exclusion Theory Inconsistent Running regime EW precision test

ATLAS

= 8 TeV s W/Z+H →

2

, R

1

R

  • 1

L dt = 20.3 fb

∫ R1 and R2 couplings: ĝ is the coupling in SU(4) vector boson g/ĝ is the coupling to fermions

light 0++ scalar and spectrum sextet model LatHC

slide-14
SLIDE 14

0.002 0.004 0.006 0.008 0.01 0.012 0.01 0.02 0.03 0.04 0.05 0.06 0.07 0.08 0.09 0.1

m M2

linear fit range: m= 0.003 − 0.007 input from 323× 64 and 483× 96 volumes M2 = csc m +sc linear fit sc = 0.0047 ± 0.0009 csc = 8.45 ± 0.17 2/dof= 0.56

=3.20 non−Goldstone scPion spectrum

scPion ijPion Goldstone fitted not fitted

systematics and mixed action taste breaking to improve

0.002 0.004 0.006 0.008 0.01 0.012 0.01 0.02 0.03 0.04 0.05 0.06 0.07 0.08 0.09 0.1

m M2

linear fit range: m= 0.002 − 0.006 input from 323× 64 and 483× 96 volumes M2 = csc m +sc linear fit sc = 0.0016 ± 0.0009 csc = 6.68 ± 0.22 2/dof= 1.6

=3.25 non−Goldstone scPion spectrum

scPion ijPion Goldstone fitted not fitted

chiSB in Goldstone spectrum vanishes only at zero lattice spacing decreasing lattice spacing

0.005 0.01 0.015 0.02

m at

0.01 0.02 0.03 0.04 0.05 0.06 0.07

M

2 at 2 Mij Mi5 Msc M

=3.3 L^3xT = 32^3x64

M 2 ij=c0 + c1 m c0=-3.753e-04 +/- 5.33e-03 c1=6.310e+00 +/- 7.25e-01
  • 2/dof=9.519e+00
M 2 i5=c0 + c1 m c0=-1.777e-05 +/- 3.29e-03 c1=5.796e+00 +/- 4.50e-01
  • 2/dof=7.432e+00
M 2 sc=c0 + c1 m c0=1.477e-03 +/- 6.09e-03 c1=5.644e+00 +/- 8.74e-01
  • 2/dof=9.767e+00
M 2 =2B m 2B=4.842e+00 +/- 4.78e-02
  • 2/dof=3.829e+00

new runs here

slide-15
SLIDE 15

0.002 0.004 0.006 0.008 0.01 0.012 0.01 0.02 0.03 0.04 0.05 0.06 0.07 0.08 0.09 0.1

m M2

linear fit range: m= 0.003 − 0.007 input from 323× 64 and 483× 96 volumes M2 = csc m +sc linear fit sc = 0.0047 ± 0.0009 csc = 8.45 ± 0.17 2/dof= 0.56

=3.20 non−Goldstone scPion spectrum

scPion ijPion Goldstone fitted not fitted

idea:

  • use the gauge configurations

generated with sea fermions

  • taste breaking makes chiPT analysis

unnecessarily complicated

  • in the analysis use valence Dirac
  • perator with gauge links on the

gradient flow

  • taste symmetry is restored in

valence spectrum

  • Mixed Action analysis should agree

with original standard analysis when cutoff is removed: cross check

0.002 0.004 0.006 0.008 0.01 0.012 0.01 0.02 0.03 0.04 0.05 0.06 0.07 0.08 0.09 0.1

m M2

linear fit range: m= 0.002 − 0.006 input from 323× 64 and 483× 96 volumes M2 = csc m +sc linear fit sc = 0.0016 ± 0.0009 csc = 6.68 ± 0.22 2/dof= 1.6

=3.25 non−Goldstone scPion spectrum

scPion ijPion Goldstone fitted not fitted

chiSB in Goldstone spectrum vanishes only at zero lattice spacing decreasing lattice spacing

systematics and mixed action taste breaking to improve

slide-16
SLIDE 16

0.002 0.004 0.006 0.008 0.01 0.012 0.01 0.02 0.03 0.04 0.05 0.06 0.07 0.08 0.09 0.1

m M2

linear fit range: m= 0.003 − 0.007 input from 323× 64 and 483× 96 volumes M2 = csc m +sc linear fit sc = 0.0047 ± 0.0009 csc = 8.45 ± 0.17 2/dof= 0.56

=3.20 non−Goldstone scPion spectrum

scPion ijPion Goldstone fitted not fitted

idea:

  • use the gauge configurations

generated with sea fermions

  • taste breaking makes chiPT analysis

unnecessarily complicated

  • in the analysis use valence Dirac
  • perator with gauge links on the

gradient flow

  • taste symmetry is restored in

valence spectrum

  • Mixed Action analysis should agree

with original standard analysis when cutoff is removed: cross check

0.002 0.004 0.006 0.008 0.01 0.012 0.01 0.02 0.03 0.04 0.05 0.06 0.07 0.08 0.09 0.1

m M2

linear fit range: m= 0.002 − 0.006 input from 323× 64 and 483× 96 volumes M2 = csc m +sc linear fit sc = 0.0016 ± 0.0009 csc = 6.68 ± 0.22 2/dof= 1.6

=3.25 non−Goldstone scPion spectrum

scPion ijPion Goldstone fitted not fitted

chiSB in Goldstone spectrum vanishes only at zero lattice spacing decreasing lattice spacing

systematics and mixed action taste breaking to improve

0.005 0.01 0.015 0.02 0.025 0.03 0.035 0.04 0.005 0.01 0.015 0.02 0.025 0.03 0.035 0.04 0.045 0.05

m M2

  • m fit range: 0.01 − 0.028

inputs from volume 403! 80 flow time t=2 linear fit =3.2 M2

= 2B m

2B = 1.243 " 0.0041 2/dof = 0.126

sextet model Goldstone pion corner pion channel flow time t=2

cyan: scPion overlay

fitted linear fit

chiral symmetry restored

20 40 60 80 100 120 0.05 0.1

=3.20 323× 64 m=0.004 gradient flow time t=3 120 eigenvalues

Quartets of Q=−1 Dirac spectrum on gradient flow eigenvalue multiplets staggered quartet eigenvalue spectrum

degenerate quartets⇒valence chiral symmetry restored

0.005 0.01 0.015 0.02 0.025 0.03 0.005 0.01 0.015 0.02 0.025 0.03 0.035 0.04

valence mass m F

m fit range: 0.008 − 0.024 483× 96 NLO linear fit =3.20 m = 0.003 original ensemble F = F + pF m F = 0.0204 ± 7.5e−05 pF = 0.351 ± 0.0043 2/dof = 0.0197

sextet mixed action at flow time t=2 F (rwall pion channel)

m fit range: 0.008 − 0.024 483× 96 NLO linear fit =3.20 m = 0.003 original ensemble F = F + pF m F = 0.0204 ± 7.5e−05 pF = 0.351 ± 0.0043 2/dof = 0.0197

fitted linear fit

new range

slide-17
SLIDE 17

epsilon regime, p regime to epsilon regime crossover, valence pqChiPT with Mixed Action:

0.5 1 1.5 2 1 2 3 4 5 <q-

v qv> / !

MvvL Nf = 2, mu=10 MeV, L=2 fm new formula ("=0) p-expansion (#=0) $-expansion ("=0) 0.5 1 1.5 2 5 10 15 20 25 30 %&"(')/ ! '!V Nf = 2, L=2 fm, mu=10 MeV new formula ("=0) p-expansion (#=0) $-expansion ("=0)

Damgaard and Fukaya Damgaard and Fukaya

new analysis in crossover and RMT regime opens up with mixed action on gradient flow

taste breaking and mixed action

slide-18
SLIDE 18

epsilon regime, p regime to epsilon regime crossover, valence pqChiPT with Mixed Action:

0.001 0.002 0.003 0.004 0.005 0.006 0.007 0.008 0.009 0.01 0.2 0.4 0.6 0.8 1 1.2 1.4 1.6 1.8 2 x 10

−3

eigenvalue scale

spectral density (,m)

Vol=403! 80 =3.25 m=0.002 25 configurations with Q=0 300 eigenvalues

flow time t=3

spectral density (,m)

1 2 3 4 5 6 7 x 10

−3

0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 1 x 10

−3

eigenvalue scale

spectral density (,m)

Vol=483× 96 =3.25 m=0.002 37 configurations with Q=0 300 eigenvalues flow time t=3 spectral density (,m)

RMT regime

  • n gradient flow

RMT regime

  • n gradient flow

0.5 1 1.5 2 1 2 3 4 5 <q-

v qv> / !

MvvL Nf = 2, mu=10 MeV, L=2 fm new formula ("=0) p-expansion (#=0) $-expansion ("=0) 0.5 1 1.5 2 5 10 15 20 25 30 %&"(')/ ! '!V Nf = 2, L=2 fm, mu=10 MeV new formula ("=0) p-expansion (#=0) $-expansion ("=0)

Damgaard and Fukaya Damgaard and Fukaya

new analysis in crossover and RMT regime opens up with mixed action on gradient flow

taste breaking and mixed action

slide-19
SLIDE 19
  • B drops by large factor after matching, with some small decrease in F
  • GMOR implies large drop of order O(10) in the chiral condensate Σ

Σ is not RG invariant, requires rescaling

  • in original analysis mΣV ~ O(100-200)

to reach RMT regime close to CW requires large resources

  • in Mixed Action analysis λΣV ~ O(10-20) RMT regime can be reached

epsilon regime, p regime to epsilon regime crossover, valence pqChiPT with Mixed Action:

0.001 0.002 0.003 0.004 0.005 0.006 0.007 0.008 0.009 0.01 0.2 0.4 0.6 0.8 1 1.2 1.4 1.6 1.8 2 x 10

−3

eigenvalue scale

spectral density (,m)

Vol=403! 80 =3.25 m=0.002 25 configurations with Q=0 300 eigenvalues

flow time t=3

spectral density (,m)

1 2 3 4 5 6 7 x 10

−3

0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 1 x 10

−3

eigenvalue scale

spectral density (,m)

Vol=483× 96 =3.25 m=0.002 37 configurations with Q=0 300 eigenvalues flow time t=3 spectral density (,m)

RMT regime

  • n gradient flow

RMT regime

  • n gradient flow

0.5 1 1.5 2 1 2 3 4 5 <q-

v qv> / !

MvvL Nf = 2, mu=10 MeV, L=2 fm new formula ("=0) p-expansion (#=0) $-expansion ("=0) 0.5 1 1.5 2 5 10 15 20 25 30 %&"(')/ ! '!V Nf = 2, L=2 fm, mu=10 MeV new formula ("=0) p-expansion (#=0) $-expansion ("=0)

Damgaard and Fukaya Damgaard and Fukaya

new analysis in crossover and RMT regime opens up with mixed action on gradient flow

taste breaking and mixed action

slide-20
SLIDE 20

0.5 1 1.5 2 1 2 3 4 5 6 7

eigenvalue scale

2() spectral density 483× 96 beta=3.20 m=0.002 LatHC

63,700,992 eigenvalues in D+D (Chebyshev expansion) = 2(0) Banks−Casher relation (nf=2)

topology: Q=0 spectral density of full Dirac spectrum (sextet rep)

0.5 1 1.5 2 1 2 3 4 5 6 7 x 10

7

scale of mode number count

(,m ) 483× 96 beta=3.20 m=0.002 LatHC

63,700,992 eigenvalues in D+D (,m ) = 2V

0 (,m ) mode number distribution

403× 80 data scaled with volume: blue dots

exact sum

mode number of full Dirac spectrum (sextet rep)

UV scale IR scale

  • nf=2 sextet example illustrates results from the Chebyshev expansion
  • full spectrum with 6,000 Chebyshev polynomials in the expansion
  • the integrated spectral density counts the sum of all eigenmodes correctly
  • Jackknife errors are so small that they are not visible in the plots.

The chiral condensate full spectrum new method

slide-21
SLIDE 21

The chiral condensate GMOR test in far IR

Improved determination of the chiral condensate Σ compared from Dirac spectra and the Chebyshev expansion. With the additive NLO cutoff term separated from B and new fit to F, the improved result on Σ eliminates previous discrepancies in the GMOR relation.

GMOR relation (nf=2): 2BF2 = Σ (Σ is the chiral condensate) F: decay constant of Goldstone pion Mπ

2 = 2B⋅m in LO χPT

Σeff Σ = 1+ Σ 32π3NFF4  2N2

F|Λ|arctan |Λ|

m 4π|Λ|N2

Fmlog Λ2 +m2

µ2 4mlog |Λ| µ

  • from chiral perturbation theory of the condensate in the p-regime:

0.5 1 1.5 2 2.5 3 x 10

−3

0.005 0.01 0.015

eigenvalue scale

spectral density (,m)

Vol=483! 96 =3.20 m=0.002 9 configurations with Q=0 171 eigenvalues Chebyshev expansion: cyan(1K) to green(4K) direct eigenvalue spectrum (red) spectral density (,m)

0.5 1 1.5 2 2.5 3 x 10

−3

0.005 0.01 0.015

eigenvalue scale

spectral density (,m)

Vol=483× 96 =3.20 m=0.002 9 configurations with Q=−1 180 eigenvalues Chebyshev expansion 3K:cyan, 6K:magenta direct eigenvalue spectrum (blue) spectral density (,m)

slide-22
SLIDE 22

0.2 0.4 0.6 0.8 1 1.2 1.4 0.2 0.4 0.6 0.8 1 1.2 1.4 1.6

scale of anomalous mass dimension

(,m) anomalous mass dimension 483× 96 (magenta) =3.20 m=0.003 LatHC −1 ~ footprint of gradient flow?

4−loop (RS)

483× 96 =3.20 m=0.002 data: blue circles

anomalous mass dimension from full Dirac spectrum (sextet rep)

0.5 1 1.5 2 1 2 3 4 5 6 7 x 10

7

scale of mode number count

(,m ) 483× 96 beta=3.20 m=0.002 LatHC

63,700,992 eigenvalues in D+D (,m ) = 2V

0 (,m ) mode number distribution

403× 80 data scaled with volume: blue dots

exact sum

mode number of full Dirac spectrum (sextet rep)

new, preliminary

The chiral condensate mass anomalous dimension

Boulder group pioneered fitting procedure

ν R(M R,mR) = ν(M,m) ≈ const ⋅ M

4 1+γ m (M ),

  • r equivalently, ν(M,m) ≈ const ⋅λ

4 1+γ m (λ) , with γ m(λ) fitted

How to match λ scale and g2 ?

slide-23
SLIDE 23

0.2 0.4 0.6 0.8 1 1.2 1.4 0.2 0.4 0.6 0.8 1 1.2 1.4 1.6

scale of anomalous mass dimension

(,m) anomalous mass dimension 483× 96 (magenta) =3.20 m=0.003 LatHC −1 ~ footprint of gradient flow?

4−loop (RS)

483× 96 =3.20 m=0.002 data: blue circles

anomalous mass dimension from full Dirac spectrum (sextet rep)

0.5 1 1.5 2 1 2 3 4 5 6 7 x 10

7

scale of mode number count

(,m ) 483× 96 beta=3.20 m=0.002 LatHC

63,700,992 eigenvalues in D+D (,m ) = 2V

0 (,m ) mode number distribution

403× 80 data scaled with volume: blue dots

exact sum

mode number of full Dirac spectrum (sextet rep)

new, preliminary

The chiral condensate mass anomalous dimension

Boulder group pioneered fitting procedure

ν R(M R,mR) = ν(M,m) ≈ const ⋅ M

4 1+γ m (M ),

  • r equivalently, ν(M,m) ≈ const ⋅λ

4 1+γ m (λ) , with γ m(λ) fitted

1 2 3 4 5 6 7 8 9 10 11 12

g

2

0.2 0.4 0.6 0.8

m

6 = 0 6 = 0.5

  • ne loop

DeGrand, Shamir, Svetitsky

How to match λ scale and g2 ?

slide-24
SLIDE 24

1 2 3 4 5 6 7 8 9 10 6.4 6.6 6.8 7 7.2 7.4 7.6 7.8 8

gradient flow time t g2(t,m2)

Wilson flow, Symanzik action 6/g0

2 = 3.25

483x96 m = 0.002−0.004 323x64 m = 0.005−0.006,0.008

scale−dependent running coupling on gradient flow

6.6 6.8 7 7.2 7.4 7.6 7.8 8 2 4 6 8 10 12 14 16

renormalized gauge coupling g2 t0 scale of g2 in chiral limit

6/g2

0=3.25

6/g2

0=3.20

cubic spline interpolation

renormalized gauge coupling in chiral limit

running coupling at fixed β

leading dependence of g2(t,m) on Mπ

2 is linear

based on gradient flow chiPT B ar and Golterman works better than expected chiral logs are not detectable

scale change at fixed renormalized g2 a → 0 needed

scale-dependent coupling matching IR to UV

nstructed at flow time 0 depend on t

0.005 0.01 0.015 0.02 0.025 0.03 0.035 0.04 0.045 0.05 1 2 3 4 5 6 7 8 9 10

M2

  • t0 scale of g2 in chiral limit

6/g0

2 = 3.25

m=0.003−0.006,0.008 fitted Chiral PT fits excellent 2 fits

t0 scale of selected g2 series in m=0 chiral limit

slide-25
SLIDE 25

0.05 0.1 0.15 0.2 0.25 0.3 0.35 0.4 1 2 3 4 5 6 ( g2(sL) - g2(L) ) / log( s2 ) g2(L) Nf = 2 sextet continuum c=7/20 SSC 1 loop 2 loop

LatHC Nf = 2 sextet

new, preliminary

the running coupling and the β function finite volume

monotonic increase of g2 with scale is consistent with:

  • mass deformed spectroscopy at low fermion mass
  • chiral condensate
  • GMOR
  • mass anomalous dimension
  • connection with g2(t,m) in bulk with chiSB

lattice step functions: 12➞18, 16➞24, 20➞30, 24➞36 last two step functions are critical in the analysis: SSC vs. WSC are consistent at large flow times which requires the large volumes

slide-26
SLIDE 26

0.05 0.1 0.15 0.2 0.25 0.3 0.35 0.4 1 2 3 4 5 6 ( g2(sL) - g2(L) ) / log( s2 ) g2(L) Nf = 2 sextet continuum c=7/20 SSC 1 loop 2 loop

LatHC Nf = 2 sextet

new, preliminary

the running coupling and the β function finite volume

Nf = 2 sextet

0.1 0.2 0.3 0.4 0.5

u = 1/g

2

  • 0.05

0.05

  • ~(u)

6 = 0 6 = 0.5 linear extrap quad extrap

  • ne loop

two loops

DeGrand, Shamir, Svetitsky

monotonic increase of g2 with scale is consistent with:

  • mass deformed spectroscopy at low fermion mass
  • chiral condensate
  • GMOR
  • mass anomalous dimension
  • connection with g2(t,m) in bulk with chiSB

lattice step functions: 12➞18, 16➞24, 20➞30, 24➞36 last two step functions are critical in the analysis: SSC vs. WSC are consistent at large flow times which requires the large volumes

slide-27
SLIDE 27

0.05 0.1 0.15 0.2 0.25 0.3 0.35 0.4 1 2 3 4 5 6 ( g2(sL) - g2(L) ) / log( s2 ) g2(L) Nf = 2 sextet continuum c=7/20 SSC 1 loop 2 loop

LatHC Nf = 2 sextet

new, preliminary

the running coupling and the β function finite volume

Nf = 2 sextet

0.1 0.2 0.3 0.4 0.5

u = 1/g

2

  • 0.05

0.05

  • ~(u)

6 = 0 6 = 0.5 linear extrap quad extrap

  • ne loop

two loops

DeGrand, Shamir, Svetitsky

monotonic increase of g2 with scale is consistent with:

  • mass deformed spectroscopy at low fermion mass
  • chiral condensate
  • GMOR
  • mass anomalous dimension
  • connection with g2(t,m) in bulk with chiSB

lattice step functions: 12➞18, 16➞24, 20➞30, 24➞36 last two step functions are critical in the analysis: SSC vs. WSC are consistent at large flow times which requires the large volumes

  • 0.2
  • 0.1

0.1 0.2 0.3 0.4 0.5 1 2 3 4 5 6 7 8 9

β(g2) g2

2-loop perturb. 4-loop MS continuum 104 124 144 164

Boulder-Tel Aviv Nf = 2 sextet without step functions 20➞30, 24➞36 Wilson flow only

slide-28
SLIDE 28

0.05 0.1 0.15 0.2 0.25 0.3 0.35 0.4 1 2 3 4 5 6 ( g2(sL) - g2(L) ) / log( s2 ) g2(L) Nf = 2 sextet continuum c=7/20 SSC 1 loop 2 loop

LatHC Nf = 2 sextet

new, preliminary

the running coupling and the β function finite volume

Nf = 2 sextet

0.1 0.2 0.3 0.4 0.5

u = 1/g

2

  • 0.05

0.05

  • ~(u)

6 = 0 6 = 0.5 linear extrap quad extrap

  • ne loop

two loops

DeGrand, Shamir, Svetitsky

monotonic increase of g2 with scale is consistent with:

  • mass deformed spectroscopy at low fermion mass
  • chiral condensate
  • GMOR
  • mass anomalous dimension
  • connection with g2(t,m) in bulk with chiSB

lattice step functions: 12➞18, 16➞24, 20➞30, 24➞36 last two step functions are critical in the analysis: SSC vs. WSC are consistent at large flow times which requires the large volumes

  • 0.2
  • 0.1

0.1 0.2 0.3 0.4 0.5 1 2 3 4 5 6 7 8 9

β(g2) g2

2-loop perturb. 4-loop MS continuum 104 124 144 164

Boulder-Tel Aviv Nf = 2 sextet without step functions 20➞30, 24➞36 Wilson flow only

This is disagreement is between two analyses nothing to do with staggered formulation

besides: promoting a beta function zero to conformal IRFP would require to remove the cutoff with the ω scaling exponent

slide-29
SLIDE 29

Kogut-Sinclair work consistent with χSB EW phase transition Relevance in early cosmology (order of the phase transition?) LatHC is doing a new analysis using different methods

17

Early universe

  • Nf=2 Qu=2/3 Qd = -1/3 fundamental rep

udd neutral dark matter candidate

  • dark matter candidate sextet Nf=2

electroweak active in the application

  • 1/2 unit of electric charge (anomalies)
  • rather subtle sextet baryon

construction (symmetric in color)

  • charged relics not expected?

Three SU(3) sextet fermions can give rise to a color singlet. The tensor product 6⌦6⌦6 can be decomposed into irreducible representations of SU(3) as, 6⌦6⌦6 = 12⇥810103⇥27282⇥35 where irreps are denoted by their dimensions and 10 is the complex conjugate of 10. Fermions in the 6-representation carry 2 indices, ψab, and transform as ψaa0 ! Uab Ua0b0 ψbb0 and the singlet can be constructed explicitly as εabc εa0b0c0 ψaa0 ψbb0 ψcc0.

slide-30
SLIDE 30

Summary: simplest composite scalar is probably very light (near conformality)

  • successful knock on LHC door ATLAS analysis and CMS plan
  • very efficient staggered BG/Q code 30-40 percent CG efficiency sextet Janos
  • light scalar (dilaton-like?) emerging close to conformal window
  • spectroscopy emerging resonance spectrum ~ 2-3 TeV
  • chiral condensate, large γ(λ) new method is very promising
  • scale-dependent coupling difficult, Gradient Flow is huge improvement
  • Electroweak phase transition and baryon intriguing