Wednesday, 22 February 2012 New-Type Fermions on the Lattice
Chiral Enough?
A D Kennedy
University of Edinburgh
Chiral Enough? A D Kennedy University of Edinburgh Wednesday, 22 - - PowerPoint PPT Presentation
Chiral Enough? A D Kennedy University of Edinburgh Wednesday, 22 February 2012 New-Type Fermions on the Lattice Outline We shall review algorithms for on-shell chiral lattice (approximate overlap) fermions In QCD chiral symmetry is
Wednesday, 22 February 2012 New-Type Fermions on the Lattice
University of Edinburgh
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Wednesday, 22 February 2012 A D Kennedy
We shall review algorithms for on-shell chiral lattice (approximate overlap) fermions In QCD chiral symmetry is explicitly broken by quark masses So there is no reason to require “too much” chirality, we just need
res q
m m
We shall show results from a preliminary dynamical study to compare the cost of using different approximations to achieve this
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Conventions
We work in Euclidean space
γ matrices are Hermitean
We write We assume all Dirac operators are γ5 Hermitean
γ γ =
† 5 5
D D
µ µ
γ = ⋅ D D
4
Such a transformation should be of the form (Lüscher)
is an independent field from has the same Spin(4) transformation properties as does not have the same chiral transformation properties as in Euclidean space (even in the continuum)
ζ is a free parameter
Wednesday, 22 February 2012 A D Kennedy
It is possible to have chiral symmetry on the lattice without doublers if we only insist that the symmetry holds on shell
y
†
y y
( )
α ζ γ αγ ζ
ψ ψ ψ ψ
− − −
→ →
5 5
1 2 1 1 2
;
i aD i aD
e e
y
†
y
†
y
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For it to be a symmetry the Dirac operator must be invariant
( )
ζ ζ
α γ αγ
− − −
→ =
5 5 1 2 1 1 2 aD aD
i i
D e De D
For an infinitesimal transformation this implies that
( )
ζ γ γ ζ − − + − =
5 5
1 2 1 1 2 aD D D aD
γ γ γ + =
5 5 5
2 D D aD D
Which is the Ginsparg-Wilson relation
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( ) ( ) ( )
γ γ γ − = = − − −
5 5 5 †
sgn ˆ
W w W W
D M D M D M D M Both of these conditions are satisfied if we define (Neuberger)
We can find a solution of the Ginsparg-Wilson relation as follows
[ ]
γ γ γ γ γ γ = + = ⇒ =
† † 1 5 5 5 5 5 5 2 1
; ˆ ˆ ˆ aD aD aD Let the lattice Dirac operator to be of the form This satisfies the GW relation iff γ
=
2 5
1 ˆ It must also have the correct continuum limit
Where we have defined where
( )
W W
D Z O a
→ ∂ / +
2
W
Z M aZ
=
( )
( ) ( )
γ γ γ → ∂ / ⇒ = ∂ / − + = − +
2 2 5 5 5
2 1 1 ˆ
W
D D Z aZ O a O a M
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H Neuberger hep-lat/9806025 A Boriçi hep-lat/9909057, hep-lat/9912040, hep-lat/0402035 A Boriçi, A D Kennedy, B Pendleton, U Wenger hep-lat/0110070 R Edwards & U Heller hep-lat/0005002
趙挺偉 (T-W Chiu) hep-lat/0209153,
hep-lat/0211032, hep-lat/0303008 R C Brower, H Neff, K Orginos hep-lat/0409118 Hernandez, Jansen, Lüscher hep-lat/9808010
菊川芳夫 & 野口達也 (Y Kikukawa &
T Noguchi) hep-lat/9902022
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Is DN local?
It is not ultralocal (Hernandez, Jansen, Lüscher)
It is local iff DW has a gap DW has a gap if the gauge fields are smooth enough Reflection positivity?
It seems reasonable that good approximations to DN will be local if DN is local and vice versa
Otherwise DWF with n5 → ∞ may not be local
( ) ( ) ( )
µ µ µ γ = + + −
1 , 1 1 sgn 5 2 D H H N
1 0 μ
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Four dimensional space of algorithms
Representation (CF , PF , CT= DWF) Constraint (5D, 4D)
ε ≈ =
,
( ) sgn( ) ( ) ( )
n n m m
P H H H Q H Approximation
( )
γ = −
5 W
H D M Kernel
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Shamir kernel
( ) ( )
5 5 5 5
; 2
W T T T W
a D M H D a D a D M
γ − = = + −
Möbius kernel
( ) ( ) ( ) ( )
5 5 5 5 5 5 5 5
; 2
W M M M W
a b c D M H D a D a b c D M
γ + − = = + − −
( )
γ = −
5 W W
H D M Boriçi (Wilson/Whatever) kernel
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− = ⋅ ⋅ − − −
1 1 1 1 1 1 1 A A B CA D CA B
= ⋅ ⋅
1 1 1 1
= ⋅ − − −
1 1 1 1 A B CA D CA B
It may be block diagonalised by an LDU factorisation (Gaussian elimination)
( )
−
= −
1
det det A B AD ACA B C D In particular
A B C D
Consider the block matrix
Equivalently a matrix over a skew field = division ring The bottom right block is the Schur complement
12 Wednesday, 22 February 2012 A D Kennedy 1 2 2 1
ψ φ φ φ φ
− −
=
n n
D χ
1 2 5 2 1
φ φ φ φ ψ
− −
=
n n
D
1 2 2 1
φ φ φ φ ψ
− −
=
n n
DU
So, what can we do with the Neuberger
Consider the five-dimensional system of linear equations
χ =
1 −
L
1 −
L L
The bottom four-dimensional component is
, N n n
D D
ψ ψ χ = =
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Alternatively, introduce a five-dimensional pseudofermion field
1 1 2 n
−
Then the pseudofermion functional integral is
† 1 5
† 5 , 1
det det det det
n D j j j
d d e D LDU D D
−
−Φ Φ =
Φ Φ ∝ = = =∏
So we also introduce n-1 Pauli-Villars fields
† ,
1 1 1 † , 1 1
det
j j j j
n n D j j j j j j
d d e D
ξ ξ
ξ ξ
− − − − = =
∝
and we are left with just det Dn,n = det DN
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Pandey, Kenney, & Laub; Higham; Neuberger (KLN) For even n (analogous formulæ for odd n)
( )
( )
ε
− − + − − +
− = = +
1 1 1 1, 1 1
1 tanh tanh 1
n x x n n n x x
x n x
( )
( )
π π − + = + + =
=
2 2 2 2 2 2
1 tan 1 1 2 tan 1
n n
k x n k k x n k
xn
( ) ( )
π π − + − =
=
2 2 2 2 1 1 2 2
cos sin 1
2 1
n
x k k k n n
x n
ωj
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( ) ( ) ( ) ( ) ( ) ( )
( )
λ
=
− ′ = − ′ −
2 2 / 2 2 1 2 1 2
sn ; 1 sn / ; sn 2 / ; 1 sn ; sn ; 1 sn 2 / ;
n m
z k z M iK m n k z k M z k iK m n k
sn(z/M,λ) sn(z,k)
ωj
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The fermion sgn problem
Approximation over 10-2 < | x| < 1 Rational functions of degree (7,8)
ε(x) – sgn(x) log10 x
0.01 0.005
1.5
0.5
Золотарев tanh(8 tanh-1x)
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Dependence on degree
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Error over approximation interval as function of degree and interval
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Derivative of Золотарев approximation at origin (maximum MD force)
, .
. . ;
Z N KLN
N N
e e e
0 87
0 49 0 025
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HMC energy change (323 × 64 lattice)
Nigel Cundy, A.D. Kennedy, Andreas Schäfer, Nucl.Phys. B845, 30—47 (2011) [arXiv:1010.5629]
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N dependence of Residual mass (323 × 64 lattice)
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Ratio of “bulk” to “low mode” contributions to residual mass (323 × 64 lattice)
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Representation: Continued Fraction I
1 2 3
1 1 1 1 1 1 A A A A
Consider a five-dimensional matrix of the form
1 1 1 1 1 1 1 2 1 2 1 3 2
1 1 1 1 1 1 1 1 S S S S S S S S S S
− − − − − −
= ⋅ ⋅
Compute its LDU decomposition
1
1 ;
n n n
S A S A S −
= + =
where
3 3 3 3 2 2 2 1 1
1 1 1 1 1 1 S A A A S A A S A A
= − = − = − − − −
then the Schur complement of the matrix is the continued fraction
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Representation: Continued Fraction II
We may use this representation to linearise our rational approximations to the sgn function
1 1 2 1 1 1 1 2 2 , (
)
n n n n n n
c c H H H H H c c c c c c ε β β β β
− −
= + + + +
1 2 1 2 1 2 1 1 2 2 1 2 2 1 2 1 1 1 c c c n n n c c c n n n c c c c c c c H n H n H H H c β β β β β − − − − − −
as the Schur complement of the five- dimensional matrix
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2 2 2 1 1 1 2 2
1 1 1 1 1 1 1 1
x p p x x p q p x q
R − −
Consider a five-dimensional matrix of the form (Neuberger & Narayanan)
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Compute its LDU decomposition
So its Schur complement is
1 2 2 1 2 2 2 2
p x x q p x R x q + − + −
2 2 2 2 2 2 2 1 1 1 1 2 1 2 2 11 1 1 1 1
p x p q x q x x q x q p x p q x q x x q x q − − − − − + + −
1 2 2 1 1 2 1 1 2 2 2 2 2 2 2 2 2 2 2 2 2 1( ( ) ) x p p x q xq p x x q x p p x q R xq p x x q − − + − − +
1 2 1 1 1 2 2 1 1 2 2 2 2 2 2 21 0 0 0 1 0 0 0 0 1 0 0 0 1 0 0 0 0 1
p p x x p x q x q x q x q p x q x q x q x q − − + − + + − +
1 1 1 1 1 1 1 1 1 2 2 1 2 1 x p p x q x R x p p q = − −
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This allows us to represent the partial fraction expansion of our rational function as the Schur complement of a five-dimensional linear system
ε
− =
= −
1, 2 2 1
( )
n j n n j j
p H H H q
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1 2 1 3 2 1 4 3 2 1
1 1 1 1 1 1 1 A C A A C A A A C C A A A A C
+ + + − +
− − − −
1 2 1 3 2 1 4 3 2 1
1 1 1 A C A A C A A A C C A A A A C
+ + + − +
− − − −
2 3 4
1 1 1 1 A A A
− − −
=
1 2 3 4
1 1 1 A C A A A C
+ −
− − − −
Consider a five-dimensional matrix of the form
Compute its LDU decomposition
CT 1 2 1 n n
S C A A A AC
− − +
= −
So its Schur complement is
L does not depend on C
( )
( )
( ) ( )
CT 5 2 5 1 1
1 1 1 1 1 T S T T
µ µ γ µ γ
−
− = + − + + − +
If where , and , then C P P
µ
± ±
= −
1 n
T T T
=
1 s s
A T
−
=
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Representation: Cayley Transform II
The Neuberger operator is
( ) ( ) ( )
CT N CT
, 1 S D H S
µ µ ≈
In Minkowski space a Cayley transform maps between Hermitean and unitary matrices
For an odd function we have
( ) ( ) ( ) ( )
1 x x T x T x
ε ε − = − ⇔ − =
( ) ( )
1 T
ε = ⇔ =
( )
j j j
x T x x
ω ω − = +
T(x) is the Euclidean Cayley transform of
( ) ( ) ( ) ( ) ( )
1 1 ( ) ; 1 1 T x x x T x T x x
ε ε ε − − = = + +
, (
) sgn( )
n m x
x
ε ≈
32
D P P P D P P D P P P D
µ µ
+ + − − + + − + + + − +
− − − − − −
The Neuberger operator with the Shamir kernel and the KLN approximation is related to the Schur complement of the Domain Wall operator
1 1 1 1 1 1 D D D D P P D D D D
µ µ
+ + + + − + + + + +
− − − = + − − −
Wednesday, 22 February 2012 A D Kennedy
Representation: Cayley Transform III
with and
( )
+ =
− +
5 5
1
W
a D a D M
( )
γ
± =
±
1 5 2 1
P
P+
μP+
P-
μP-
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(1) (1) (1) (2) (2) (2) (3) (3) (3) ( 4) ( 4) ( 4)
D D P D P D P D D P D P D D P D P D P D
µ µ
+ − + − − − − + − + − − + − + + + − − +
− −
The Neuberger operator with a Möbius kernel and any approximation is related to the Schur complement of D5 (μ)
(1) (1) (1) (1) (2) (2) (2) (2) (3) (3) (3) (3) ( 4) ( 4) ( 4) ( 4)
D D D D D D D D P P D D D D D D D D
µ µ
+ − + − − + + − − + − + + − − + − +
− = + −
Representation: Cayley Transform IV
with and
( ) ( ) 5 ( ) ( ) 5
( ) 1 ( ) 1
s s s W s s s W
D b D M D c D M
α α
+ −
= − + = − −
( )
γ
± =
±
1 5 2 1
P
( ) ( ) ( ) ( ) 5 5 5 5 5 5 5 5
;
s s s s s
b c b c b c b c
ω + + = − = −
P+
μP+
P-
μP-
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(1) (1) (1) (1) (2) (2) (2) (2) 5 (3) (3) (3) (3) ( 4) ( 4) ( 4) ( 4)
( ) D D D D D D D D D P P D D D D D D D D
µ µ µ
+ − − + − + + − − + − + + − − + + −
− = + −
1 1 1 1 1 1 1 1 1
P P
−
−
≡ +
Cyclically shift the columns of the right-handed part where
5 5
D D
→
Representation: Cayley Transform V
P+ P-
μP+ μP-
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( ) ( ) ( ) s s s
Q D P D P
± + ± −
≡ +
Representation: Cayley Transform VI
1 ( ) ( ) s s s M s s M
H T Q Q H
ω ω
− + −
− ≡ − = +
With some simple rescaling
1 1 1 2 1 3 1 4
1 1 1 5 1
( )
T C T T T C
D
µ
− + − − − −
− − − − −
=
The domain wall operator reduces to the form introduced before
( ) ( ) ( ) ( )
1 2 3 4
Q Q Q Q
− − − − −
=
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Representation: Cayley Transform VII
It therefore appears to have exact off-shell chiral symmetry But this would violate the Nielsen-Ninomiya theorem! However, DDW is a very non-local operator
We can only use DDW for valence (“external”) propagators, and thus use off-shell (continuum) chiral symmetry to manipulate matrix elements
We solve the equation
{ }
5
,
DW
D
γ =
Hence Note that satisfies
1 1 DW N
D D a
− −
= −
{ } { }
{ }
1 1 1 1 5 5 5 5 5
, , 2 , 2
DW N N N N
D D a D D D a
γ γ γ γ γ
− − − −
= − = − =
5 5
( ) (1) D D
µ φ χ =
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Ginsparg-Wilson defect
5 5 5 5
2
L
D D aD D
γ γ γ γ + − = ∆
Using the approximate Neuberger operator
( )
1 5 2 1
aD H
γ ε = + ∆L measures chiral symmetry breaking
( )
2 1 2 1 L
a H
ε ∆ = −
The quantity is essentially the usual domain wall residual mass (Brower et al.)
† res †
tr tr
L
G G m G G
∆ =
mres is just one moment of ∆L G is the quark propagator
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For state-of-the-art dynamical QCD computations with on-shell chiral fermions Boriçi (Wilson or Whatever) kernel seems
nicest, except for historical compatibility
Möbius kernel can be used to shift the spectrum to make better use of tanh approximation
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4D pseudofermions seem simpler than 5D ones 5D Domain Wall requires pseudofermions = Pauli- Villars fields (pseudo-pseudofermions) to avoid being killed by noise
This seems unnecessary work
Hasenbusch acceleration
5 dimensional multishift? Possible advantage of 4 dimensional nested Krylov solvers
Quantitative comparison still required (only old results
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Zolotarev approximation with moderate ε seems to give much smaller (x 10-4) residual mass than tanh for a small (≈20%) extra cost DWF using Möbius kernel may also be competitive
But its benefits seem to follow from shifting the spectrum to make better use of the tanh approximation So why not just use shifted tanh approximation? And if so, why not use “truncated” Zolotarev approximation?
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There appear to be opportunities to tune five dimensional representations Zolotarev DWF (Chiu)
Old data indicated it was much slower than alternatives Should be compared with DWF at same small residual mass Condition number improved significantly by naïve “tuning” of
the parameter αs (caveat: unpublished result)
Can its condition number be further improved?
Quantitative comparison of CF, PF, and CT (DWF) for realistic systems would be nice
But expensive…
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Slow tunnelling between topological sectors
Algorithmic or physical problem (at μ=0)?
Include extra determinant terms in the action to suppress defects without suppressing topological modes? Does global topology change matter?
Finite volume effect? Cluster decomposition Local topology change suffices? (Whatever this means)
Lots of interesting things still to study!