Axions and topology in QCD - ECT* Indico (Indico)
Transcript of Axions and topology in QCD - ECT* Indico (Indico)
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Maria Paola Lombardo
INFN Firenze
Axions and topology in QCD
Interdisciplinary approach to QCD-like composite dark matter
ECT* Villazzano 1 October 2018
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Nf
Phases of strong interactions
Composite DM?
Nfc2we are here
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Nf
Phases of strong interactions
Composite DM?
Nfc2we are here
QCD axions
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Nf
Phases of strong interactions
Composite DM?
Nfc2we are here
QCD axions
Temperature
Tc
To learn about today’s axions
we need to go back to
the early Universe
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Different entangled topics
QCD phenomenology, hadron spectrum
History of the Universe - particle cosmology
Phases and Topology of QCD
Calculational tool: Lattice simulations
Axions
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Different entangled topics
QCD phenomenology, hadron spectrum
History of the Universe - particle cosmology
Phases and Topology of QCD
Calculational tool: Lattice simulations
Axions
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Plan
Axions Topology in QCD
Results:
Topological Susceptibility Bounds on the QCD axion’s mass Beyond Susceptibility - towards the axion’s potential
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= (< Q2 > � < Q >2)/V
✓ term, strong CP problem and topology
electric dipole moment
of the neutron
Axions ‘must’ be there (?)
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Axion potential
weakly coupled
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Temperatures:
Quark Gluon Plasma: Topology
150 MeV < T < 500 MeV
..and beyond
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After freezout constant
Wantz, Shellard 2010
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p�(T )/fa=
First numerical study:
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Cold Dark Matter candidates might have been created after the inflation
Several CDM candidates are highly speculative - but one, the axion, is
Theoretically well motivated in QCDAmenable to quantitative estimates once QCD topological properties are known:
Post-inflationary axionsAppear Freeze
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Origin of mass
Quarks Nuclei
Hadron cosmology:
QCD transition
time
Chiral symm. breaking Confinement:
Chiral perturbation theory + Potential models
= Hadron spectrum
Nucleosynthesys
Almost all hadrons can be described
taking into account chiral symmetry breaking
and confining potential
Hadrons
QCD topology and phenomenology
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Origin of mass
Quarks Nuclei
Hadron cosmology:
QCD transition
time
Chiral symm. breaking Confinement:
Chiral perturbation theory + Potential models
= Hadron spectrum
Nucleosynthesys
Almost all hadrons can be described
taking into account chiral symmetry breaking
and confining potential
Hadrons
With an importantexception
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Pseudoscalar light spectrum: eight pseudoGoldstones
Exception!
is too heavy
SU(3)LXSU(3)R ! SU(3)V
U(1)Ashould be broken as well producing a 9th Goldstone BUT:
⌘0
�PT predicts
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UA(1) problem:
would be broken by the (spontaneously generated) q̄q :
the candidate Goldstone is the ⌘0
too heavy!! (900 MeV)BUT: the divergence of the current contains a mass independent term
The UA(1) symmetry is explicitly broken
⌘0 and the
symmetryThe
IF
Topology,
6= 0
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It can be proven that = Q
The ⌘0 mass may now be computed from the decay of the correlation
which at leading order gives the Witten-Veneziano formula
and Q = n+ � n�
Gluonic definition
Fermionic definition
Successfulat T=0
FF̃
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It can be proven that = Q
The ⌘0 mass may now be computed from the decay of the correlation
which at leading order gives the Witten-Veneziano formula
and Q = n+ � n�
Gluonic definition
Fermionic definition
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It can be proven that = Q
The ⌘0 mass may now be computed from the decay of the correlation
which at leading order gives the Witten-Veneziano formula
and Q = n+ � n�
Gluonic definition
Fermionic definition
Successfulat T=0
Q(x) Q(y)
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ETMC 2017
solution
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Results
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Topology on a lattice
Cuts..
…It is difficult to identify different topological sectors
…and large temperatures require huge statistics..
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QCD topology, long standing focus of strong interaction:
-learning about: fundamental symmetries, mass, strongCP problem —> axions
-hampered by technical difficulties
Recent developments:-first results for dynamical fermions at high temperature:
Trunin et al. J.Phys.Conf.Ser. 668 (2016) no.1, 012123 Bonati et al. JHEP 1603 (2016) 155 Borsany et al. Nature 539 (2016) no.7627, 69 Petreczky et al. Phys.Lett. B762 (2016) 498
Phys.Rev. D95 (2017) no.5, 054502 Taniguchi et al.Burger et al.
TmFT+work in progress
⌘0
Nucl.Phys. A967 (2017) 880
Burger et al. arXiv 180506001
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The Hot Twisted Mass project
Topology (and axion’s properties) from lattice QCD with a dynamical charm
Nucl.Phys. A967 (2017) 880-883
Chiral observables and topology in hot QCD with two families of quarks
arXiv:1805.06001
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Why Nf = 2 +1 +1 ?
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Nf = 2+1+1 Wilson fermions with a twisted mass term
‘twisted’ mass terms in flavor space:
are added to the standard Wilson Lagrangian
Consequences: -simplified renormalization properties -automatic O(a) improvement -control on unphysical zero modes
Frezzotti Rossi 2003
Successful phenomenology at T=0
iµ⌧3�5 for two degenerate light flavors
iµ�⌧1�5 + ⌧3µ� for two heavy flavors
ETMC collaboration 2003—
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Table 1. Number and parameters of used configurations
T = 0 (ETMC)nomenclature
� a [fm] [6] N
3
�
N
⌧
T [MeV] # confs.
A60.24 1.90 0.0936(38)243
323
567891011121314
422(17)351(14)301(12)263(11)234(10)211(9)192(8)176(7)162(7)151(6)
585137034197057752522710522941988
B55.32 1.95 0.0823(37) 323
5678910111213141516
479(22)400(18)342(15)300(13)266(12)240(11)218(10)200(9)184(8)171(8)160(7)150(7)
59534532723345329566711023081304456823
D45.32 2.10 0.0646(26)323
403
483
678101214161820
509(20)436(18)382(15)305(12)255(10)218(9)191(8)170(7)153(6)
403412416420380793626599582
7
Fixedvaryingscale
Four pionmasses
For each lattice spacing we explore a range of temperatures 150MeV — 500 MeV by varying Nt
We repeat this for three different lattice spacings following ETMC T=0 simulations.
Advantages: we rely on the setup of ETMC T=0 simulations. Scale is set once for all.
Disadvantages: mismatch of temperatures - need interpolation before taking the continuum limit
Nf = 2 +1+1 Setup
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Topological and chiral susceptibility
�top
=< Q2top
> /V = m2l
�5,disc
�top
=< Q2top
> /V = m2l
�disc
HotQCD, 2012
Kogut, Lagae, Sinclair 1999
From:
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Chiral susceptibility
Within errors, no discernable spacing dependence
D210B260A260
T [MeV]
χψ̄ψ/T2
500400300200100
102
101
100
10−1
10−2
10−3
10−4
B470A470
T [MeV]
χψ̄ψ/T2
500400300200100
102
101
100
10−1
10−2
10−3
D370B370A370
T [MeV]
χψ̄ψ/T2
500400300200100
102
101
100
10−1
10−2
10−3
10−4
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0
1
2
3
4
5
6
250 300 350 400 450
d(T)
T
Fermionic, all massesGluonic (nearly linear)
Borsanyi et al.Bonati et al.
Petreczky et al.DIGA, Nf = 2DIGA, Nf = 3
Comparisons with other results : �1/4top
= aT�d(T )Effective exponent d(T):
[MeV]
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�0.25(T ) = aT�d(T )
d(T ) = �T ddT ln�0.25(T ) Possibly consistent
with instant -dyon? Shuryak 2017
Faster decrease before DIGA sets in
Power-law decay?For instanton gas
d(T ) ⌘ const ' (7 + Nf
3 )
d effHTL
@MeVDT
DIGA HNf =2LDIGA HNf =3L
250 300 350 400 450
5
10
15
20
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Continuum limit (details)
20
35
50
300 350 400 450 500 550
�1/4
top
[MeV]
T [MeV]
A370B370D370
450400350300250200T [MeV]
a2 [fm2]
χ1/4
top[M
eV]
0.0120.010.0080.0060.0040.0020
100
200
50
20
the B ensemble is indeed representative of continuum
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Comparison with BNL results numerical data courtesy S. Sharma
Fermionic
Fermionic GluonicGluonicBNL BNL
199 < T < 210 MeV 333 < T < 350 MeV
�1/4[MeV] �1/4[MeV]
a2[fm2] a2[fm2]
dotted lines to guide the eye
Continuum limit (details)
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Results for physical pion mass Rescaled according to
100 200 300 400 500 600
5
10
20
50
100
c top1ê4¥Hm pph
ysêm pL
@MeVD
@MeVDT
D210ÌAB260ÛıD370â
370 continuum135 MeV@Borsanyi et al.D
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ctop
1ê4@MeVD
@MeVDT
470 MeVÌ370 MeV·260 MeVÛ210 MeVı
500200 300
10
100
50
20
30
15
150
70
Using the B ensemble as representative of continuum
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1 5 10 50 100 5001.0
0.8
0.6
0.4
0.2
0.0WaêW D
M
Axion mass @meVD
WaêW D
M
Axion mass @meVD
370 MeVÁ
210 MeV‡260 MeVâ
d=8 HDIGALÏd=4ÌÚ A ¥104
Ù A ê 104
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1 5 10 50 100 5001.0
0.8
0.6
0.4
0.2
0.0
WaêW D
M
Axion mass @meVD
WaêW D
M
Axion mass @meVD
370 MeVÁ
210 MeV‡260 MeVâ
d=8 HDIGALÏd=4ÌÚ A ¥104
Ù A ê 104
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..towards the axion’s potential
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Distribution of the topological charge P(Q) cluster around integers as cooling proceeds
P(Q) P(Q)
Q Q
T=153 MeV T=253 MeV
(results for a = 0.06 fm)
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Gradient flow
Stop flowing when
Continuum limit of is independent on thechosen reference value
Monitor as a function of t
Evolve the link variables in a fictitious flow time:
< O(t) >Observables renormalized at µ = 1/p8t
< O(t) >
Luscher, Luscher Weisz¨ ¨
Caveat: note comments by Kanaya et al.
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t2 < E > |t=t
x
,x=0�6 = (0.3, 0.66, 0.1, 0.15, 0.2, 0.25, 0.45)
Flowing towards the plateau
�0.25[MeV ]
T
We focuson
t(0.3) = t0and
t(0.66)= t1
Reference value
a = 0.082 fm
t0 t1
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a = 0.082 fm a = 0.065 fm
On finer lattices, plateau is almost reached: �0.25[M
eV]
Reference value Reference value
Gradient method coincides with cooling
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e�F (✓) = hei✓Qi
P⌫
=
Z⇡
�⇡
d✓
2⇡e�i✓⌫e�F (✓)
Cn
= (�1)n+1 1
V
d2n
d✓2nF (✓)
���✓=0
⌘< Q2n >conn
F (✓) = V1X
n=1
(�1)n+1 ✓2n
(2n)!C
n
P⌫
=e�
⌫2
2�2
p2⇡�2
1 +
1
4!
⌧
�2He4 (⌫/�)
�
�2 = V C1 and ⌧ = C2/C1
Taylor expansion, and cumulants of the topological charge distributionP (Q)
Q
Q = ⌫
P(Q) is Gaussian for V ! 1
F (✓) is ‘hidden’ in P(Q)’s cumulants
F (✓)
Cumulants ofP(Q)
Taylor coefficients of
Computing
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Instanton potential - cumulants’ ratio b2
Consistent with Bonati et al.
-2
-1
0
1
2
3
4
5
6
150 200 250 300 350 400 450 500 550
(<Q
4 > -3
<Q2 >2 )/<
Q2 >)
= -1
2 b2
T
a=0.082 fm,t0a=0.082 fm,t1a=0.065 fm,t0a=0.065 fm,t1
DIGAChPT
Gaussian
DIGA limit for T > 350 MeV
b2 = -1/12
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0
1
2
3
4
5
6
250 300 350 400 450
d(T)
T
Fermionic, all massesGluonic (nearly linear)
DIGA, Nf = 2DIGA, Nf = 3
Effective exponent : Same DIGA onset seen in b2 ≈ 350 MeV
-2
-1
0
1
2
3
4
5
6
150 200 250 300 350 400 450 500 550
(<Q
4 > -3
<Q2 >2 )/<
Q2 >)
= -1
2 b2
T
a=0.082 fm,t0a=0.082 fm,t1a=0.065 fm,t0a=0.065 fm,t1
DIGAChPT
Gaussian
[MeV] [MeV]
�1/4top
= aT�d(T ) Results for F (✓) coherent with d(T)
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Topology in hot QCD is a rich field which is only recently becoming truly quantitative:
there is room for improvement!
Topology constraints the QCD axion mass
Parting remarks
Questions: requirements from phenomenology?
axion potential?
1 5 10 50 100 5001.0
0.8
0.6
0.4
0.2
0.0
WaêW D
M
Axion mass @meVD
WaêW D
M
Axion mass @meVD
370 MeVÁ
210 MeV‡260 MeVâ
d=8 HDIGALÏd=4ÌÚ A ¥104
Ù A ê 104