P. F. Harrison (U. of Warwick) PERSPECTIVE ON · PDF filePREDICTED IN TRIMAX. MIX.! ! ! ! THE...
Transcript of P. F. Harrison (U. of Warwick) PERSPECTIVE ON · PDF filePREDICTED IN TRIMAX. MIX.! ! ! ! THE...
Miami-2008, 17 Dec 2008 Presented by: W. G. Scott, PPD/RAL. 1
1) “Plaquette Invariants and the Flavour-Symmetric…” P.F. Harrison, D. R. J. Roythorne,
and W. G. Scott, Phys. Lett. B 657 (2007) 210. arXive:0709.1439 [hep-ph]
2)“Real Invariant Matrices and Flavour-Symmetric…” P.F. Harrison, W. G. Scott
and T. J. Weiler, Phys. Lett. B 641 (2006) 372. hep-ph/0607336
3)“Simplified Unitarity Triangles for the Lepton Sector…” J. D. Bjorken, P.F. Harrison,
and W. G. Scott, Phys. Rev D 74 (2006) 073012. hep-ph0511201
4)“Covariant Extremisation of Flavour-Symmetric Jartlskog Invariants…” P.F. Harrison,
and W. G. Scott Phys. Lett. B 628 (2005) 93. hep-ph/0508012
5) “The Simplest Neutririo Mass Matrix” P. F. Harrison and W. G. Scott
Phys Lett. B B594 (2004) 324. hep-ph/0403278. ……..
A FLAVOUR-SYMMETRIC P. F. Harrison (U. of Warwick)
W. G. Scott (STFC, PPD/RAL)
Miami-2008 17 Dec 2008
( )
=
1/21/31/6
1/21/31/6
01/32/3
τ
µ
e
U
ν ν ν
2lν
321
“Tri-Bimaximal Lepton Mixing and the Neutrino Oscillation Data” P.F. Harrison,
D. H. Perkins, W. G. Scott, Phys. Lett. B. 530 (2002) 167. hep-ph/0202074 (see also: HPS hep-ph/9904297 )
OUTLINE OF TODAYS TALK:
NOW OFFICIALLY
A “FAMOUS” PAPER ( > 250 CITES).
“A TREMENDOUS ACHIEVEMENT!”
T. D. LEE AT CERN - 30 AUG 2007
(CERN indico video min. 42!!)
PERSPECTIVE ON NEUTRINO MIXING
(emphasis on Flavour-Symmetry )
OF COURSE IT IS ACTUALLY THE EXPERIMENTS WHICH ARE TREMENDOUS!
“Review”
of
past few
years
2004-2007
of HS…
Miami-2008, 17 Dec 2008 Presented by: W. G. Scott, PPD/RAL. 2
T. D. LEE LECTURE AT CERN 30 AUG 2007
CERN video: http://indico.cern.ch/conferenceDisplay.py?confId=19674 (min. 42)
Miami-2008, 17 Dec 2008 Presented by: W. G. Scott, PPD/RAL. 3
2/13/16/1
2/13/16/1
03/13/2
321
τµ
νννe
3/13/13/1
3/13/13/1
3/13/13/1
321
τµ
νννe
WE DID “ACHIEVE” SOMETHING HOWEVER:WE PREDICTED TWO SM+ PARAMETERS!!:
Tri-Bi-Maximal (HPS 1999/2002)
Tri-Maximal Mixing (HS/HPS 1994/1995)
HS/BHS (2002-2006)
* 3/1*
* 3/1*
* 3/1*
321
τµ
νννe
via Tri-Phi-Maximal & Tri-Chi-Maximal
(HS 2002)
“ -Trimaximal Mixing”
“S3 Group Mixing”
“Magic-Square Mixing”
“Tri-χφ-Maximal”
3/122 == µUUe
CHOOZ EXPT.SAYS < 0.03 (not HS/HPS!!)
There was never a prediction from HPS/HS of exact Ue3≡0!
2ν
Please not just “tri-maximal”!!
IMMEDIATELY
GENERALISES
Miami-2008, 17 Dec 2008 Presented by: W. G. Scott, PPD/RAL. 4
Solar Datadist. spect. B and . systs corr. ignoring -Salt NoSalt of
average naivemy is 03.035.0/point SNO
8+
±=NCCC
ph/9601346-hep 111 (1996) 374 PLB also see ;ph/0202074-hep 167 (2002) 530 PLB HPS
Miami-2008, 17 Dec 2008 Presented by: W. G. Scott, PPD/RAL. 5
ph/9601346-hep 111. (1996) 374 PLB HPS3 Fig.
MIX.TRIMAX.IN DICTEDPRE ! ! ! !
THE “5/9-1/3-5/9” BATHTUB
Miami-2008, 17 Dec 2008 Presented by: W. G. Scott, PPD/RAL. 6
=
21
31
61
21
31
61
031
32
|U| 2
Symmetries of TriBimaximal Mixing:
1) “CP symmetry”
Zero CP violation J=0
(hopefully approximate!)
2) “µτ-reflection symmetry”
“Two rows equal” (=Max CPV!)
|Uµi|=|Uτi| for all i=1-3.
3) “democracy symmetry”
one trimaximal eigenvector
|Uαi|=|1/3 for all α for some i.
Miami-2008, 17 Dec 2008 Presented by: W. G. Scott, PPD/RAL. 7
HPS “Derivation” of TriBimaximal Mixing:
2
10
2
1
010
2
1-0
2
1
*
*
*
3
ω
3
1
3
33
1
3
ω3
1
3
1
3
1
τ
µ
e
ν ν ν * * * 321
ϖ
ϖ
νUUU l
m=
=
abb
bab
bba
*
*
*
MM
* * *
ll
=
x0y
0z0
y0x
*
*
*
MM
* * *
νν
=
τωµe
τµe
τµe
l
mωmm
ωmωmm
mmm
*
*
*
M
−
−−
2
i
3
1
6
12
i
3
1
6
1
03
1
3
2
τ
µ
e
ν ν ν 321
⇒
3 x 3 circulant
(by definition
of the * basis)
2 x 2 circulant
(determines
the physics)
=
m mm
UMMU
τµe
llll
diag2=mm
diag
3212 mmm
UMMU =ννννmm
mMM M →
In the “circulant basis”: *
ω/3m/3ωm/3mb
/3ωmω/3m/3mb
/3m/3m/3ma
2τ
2µ
2e
2τ
2µ
2e
2τ
2µ
2e
++=
++=
++=
A popular choice:
Harrison, Perkins, Scott, Phys. Lett. B. 530 (2002) 167. hep-ph/0202074
† †
Miami-2008, 17 Dec 2008 Presented by: W. G. Scott, PPD/RAL. 8
YES – YOU’VE SEEN THESE NUMBERS BEFORE SOMEWHERE!
2
1
3
1
6
111
2
1
3
1
6
111
03
1
3
200
000
102
21
−+−
−+
−
Mmm
JM = 0
SUBSET
OF
CLEBSCH-
GORDAN
COEFFS.
e.g.
1 1 21 =⊗= jj
COULD
PERHAPS BE
A USEFUL
REMARK ?!!
See: J. D. Bjorken, P. F. Harrison and W.G. Scott. hep-ph/0511201
Miami-2008, 17 Dec 2008 Presented by: W. G. Scott, PPD/RAL. 9
++
−−+
+−
++
−−
−−
+−
−−+
6
cissc
2
siscc
3
1
2
cissc
6
siscc6
cissc
2
siscc
3
1
2
cissc
6
siscc
cs3
2isc
3
2
3
1ss
3
2icc
3
2
φχφχφχφχφχφχφχφχ
φχφχφχφχφχφχφχφχ
φχφχφχφχ
“ν2-Trimaximal Mixing”
+−−
+−+−
−
6
si
2
c
3
1
2
si
6
c6
si
2
c
3
1
2
si
6
c
s3
2i
3
1c
3
2
χχχχ
χχχχ
χχ
++−
+−−−
−
6
s
2
c
3
1
2
s
6
c6
s
2
c
3
1
2
s
6
c
s3
2
3
1c
3
2
φφφφ
φφφφ
φφ
“Tri-χ-Maximal Mixing” “Tri-Φ-Maximal Mixing”
cosφc
sinφs
cosχc
sinχs
φ
φ
χ
χ
=
=
=
=
Exact µτ - Refl. Symm., J≠0 J=0, Break µτ-Symmetry
Χ→0Φ→0
“Tri-φχ-maximal mixing”, “S3 group mixing”
“Magic-square mixing”, “BHS-mixing”… .
“Symmetries and Generalisations of Tri-Bimaxiaml Mixing” P.F. Harrison, and W. G. Scott Phys. Lett. B 535 (2002) 163. hep-ph/0203029
“Permutation Symmetry, Tri-Bimaximal Mixing and the S3 Group ...” P.F. Harrison, and W. G. Scott Phys. Lett. B 557 (2003) 76. hep-ph/0302025
Miami-2008, 17 Dec 2008 Presented by: W. G. Scott, PPD/RAL. 10
Symmetric Group S3
(natural representation):
=
001
100
010
P(123)
=
010
001
100
P(321)
=
100
010
001
I
=
100
001
010
P(12)
=
010
100
001
P(23)
=
001
010
100
P(31)
zP(12)yP(31)xP(23) P(321)bbP(123)aI
MM νν
+++++=
+=∗
odd"" even""
+
=∗
∗
∗
zxy
xyz
yzx
ν
ν
ν
abb
bab
bba
ν
ν
ν
ν ν ν ν ν ν
τ
µ
e
τ
µ
e
τµeτµe
Nature Plays Sudoku !!
Experiment tells us that
the neutrino mass matrix²in the (charged-lepton)
flavour basis can be written
as a 3 x 3 Magic Square !!All row/column sums equal !!
The most general such (hermitian) matrix may be constructed as an “S3 Group Matrix”
in the natural representation of the S3 group ring
2x)yy)/(x(z32φ
zx)yzxyzy(Imb)/(x62χ 222
−+−=−−−++=
tan
tan
Any “S3 Group Matrix”
clearly has (at least) one
trimaximal eigenvector:
1
1
1
3
1
ννMM
“circulant” “retro-circulant”
“ -Trimaximal Mixing”
=“Magic-Square”/”S3 Group Mixing”
=“Democracy Symmetry”
†
†
2ν
“Permutation Symmetry, Tri-Bimaximal Mixing and the S3 Group ...” P.F. Harrison, and W. G. Scott Phys. Lett. B 557 (2003) 76. hep-ph/0302025
Miami-2008, 17 Dec 2008 Presented by: W. G. Scott, PPD/RAL. 11
Simplified Unitarity Traingles in the Lepton Sector
The Matrix* of UT angles:
“ν2.ν3”=“the ν1-triangle”
−−
−
−−
e3
e3
e3
321
U2
1C
2
1
3
1 C
6
1
U2
1C
2
1
3
1 C
6
1
U 3
1 C
6
2
τ
µ
e
ν ν ν
=
τ3τ2τ1
µ3µ2µ1
e3e2e1
321
φφφ
φφφ
φφφ
τ
µ
e
Φ
ν ν ν
“BHS” Mixing
Each angle Φαi appears inone row-based triangle and one column-based triangle
e
µ
τ
Uτ3
1σ
Uµ3Ue3
*Footnote [42] hep-ph/0511201
Note the natural “complementary”
labelling of angles and triangles
J. D. Bjorken, P.F. Harrison, and W. G. Scott, Phys. Rev D 74 (2006) 073012. hep-ph0511201
CPCPCPCPe3e3e3e3
23232323e3e3e3e3 JJJJ
22223333
UUUU θθθθ----
4444
ππππ
2222
UUUU ≈≈
ImImImImReReReRe
= “ν2-Trimaximal”
Miami-2008, 17 Dec 2008 Presented by: W. G. Scott, PPD/RAL. 12
“Simplified Unitarity Triangles for the Lepton Sector…”
J. D. Bjorken, P.F. Harrison, and W. G. Scott, Phys. Rev D 74 (2006) 073012. hep-ph/0511201
×
××
×
++−+
+−−−
1ν 1l*
1ν 1l
lν
*1ν 1l1ν 1l
321
UU
Π
UU
τ
µ
e
ν ν ν
*1ν 1l1ν 1l
*1ν 1l1ν 1llν UUUU: Π −++++−−−=
J i K: Π lνlν +−=
π π π
π|
π|
π|
Π- ArgΠ- ArgΠ- Arg
Π- ArgΠ- ArgΠ- Arg
Π- ArgΠ- ArgΠ- Arg
τ
µ
e
φφφ
φφφ
φφφ
τ
µ
e
Φ
ν ν ν ν ν ν
τ3τ2τ1
µ3µ2µ1
e3e2e1
τ3τ2τ1
µ3µ2µ1
e3e2e1
321321
=
=
=
UUUUUUUUUUUU
UUUUUUUUUUUU
UUUUUUUUUUUU
τ
µ
e
Π
ν ν ν
*µ1
*e2µ2e1
*µ3
*e1µ1e3
*µ2
*e3µ3e2
*τ2
*e1τ1e2
*τ1
*e3τ3e1
*τ3
*e2τ2e3
*τ1
*µ2τ2µ1
*τ3
*µ1τ1µ3
*τ2
*µ3τ3µ2
321
We define the Matrix of UT Angles:*
From the Plaquette Products:
Form the Matrix of Plaquette Products:
*Footnote [42] hep-ph/0511201
3) (mod
Miami-2008, 17 Dec 2008 Presented by: W. G. Scott, PPD/RAL. 13
ooo
o
o
o
4oo
ooo
ooo
tbtstd
cbcscd
ubussud
180 180 180
180|
180|
180|
)0(λ68112
239067
157221
t
c
u
φγφφ
χβφαφχγφ
φβφχβφ
t
c
u
Φ
bs d b s d
≈
=
+==−=
=≈=
=
UNITARITY TRIANGLES IN THE QUARK SECTOR
THE MATRIX OF UNITARITY TRIANGLES IN THE QUARK SECTPR
EQUIVALENT INFO. TO CKM MATRIX !!
χ
α
β+χγ -χ
s
d
b
α
βγ
u t
c
“d.b”=“the s-triangle” “t.u”=“the c-triangle”
( in SM - see e.g. F. Muheim “Flavour in the Era of LHC” HEP Forum 21 June 2007)o1≈χ
!!!20 CDF/D0 o≈
Systematic “complemenatry” notation here
is a big improvement on existing notations!!
Miami-2008, 17 Dec 2008 Presented by: W. G. Scott, PPD/RAL. 14
(3)(3)(3)(3)
22222T(2)∆∆
(2)
)1(1D 1)1(B )11(A 1) (1C
xy)(wz)zyx(wz)yx(w1)/2P.P (Tr1) (1G
xy)3(wzNL
T DetP Det)11( F
×=×=×=×=
+−+++++++=−=×=
−===×=
P.F. Harrison, D. R. J. Roythorn, and W. G. Scott, Phys. Lett. B 657 (2007) 210. arXive:0709.1439 [hep-ph]
1) Flavour Symmetry: A fundamental theory of flavour should
be Flavour-Symmetric (ie. it should make no reference to explicit flavour indices).
The Principles which guide us:
Use Flavour-Symmetric Jarlskog Invariant variables!!The Architypal example:The Jarlskog CP-Invariant:
∆∆lν
N2L
N][L, DetiΠIm J −==
2) Jarlskog Invariance: A fundamental theory should be weak-basis independent
(i.e. it should make no reference to any preferred weak-basis).
We define 6 New Flavour-Symmetric Jarlskog-Invariant mixing variables :
Independent, of plaquette choice l,νhence “Plaquette Invariant”
νl S3S3 )11( ×⇐×
The Jarlskogian J is “odd-odd” under separate l and νflavour permutations:
νl S3S3 ×
ν33 CC l ×spanning theInvariant polynomial ring
(functions only of mixing angles)
“Plaquette Invariants and the Flavour-Symmetric …”
with odd/even symmetry under:
36F272C18G1081 J 22 −+−=An `elemental” set - not all independent, e,g,
ννν
lll
MMM N
MMM L
→=→= †
†
Miami-2008, 17 Dec 2008 Presented by: W. G. Scott, PPD/RAL. 15
( )
′
′
′
b
s
d
1
1
1
tcu ( )
′′′
b
s
d
1
1
1
tcu
Jarlskog Invariance:
U(3)
(Also known as Weak-Basis Invaraince)
In any “weak” (“gauge”) basis the weak interaction
is diagonal and universal (i.e proportional to the identity matrix)
We often seem to choose to blame
the mixing on the “down” quarks!
weak basis
But we could equally choose to
blame it on the “up”-type quarks!
weak basis
Elsewhere in the Lagrangian: (i.e in the yukawa sector)
Mu is diagonal
(Md is non-diagonal)
Md is diagonal
(Mu is non-diagonal)
Mass²
Matrices
CC
weak
int.
All observables are Jarlskog Invariant:
e.g. masses, mixing angles: etc. J δ m m m
V m m m
13 3 µe
2 ub t du
θ
Note that the Jarlskogian J is (moreover) also Flavour-Symmetric !!
Miami-2008, 17 Dec 2008 Presented by: W. G. Scott, PPD/RAL. 16
3333
3
2222
2
1
Tr :
Tr :
Tr :
τµ
τµ
τµ
mmmLL
mmmLL
mmmLL
e
e
e
++==
++==
++==
FLAVOUR-SYMMETRIC
Charged-Leptons: Mass Matrix:
JARLSKOG INVARIANT MASS PARAMETERS
321
τµ mmm
LLL
e
≅
3
3
3
2
3
1
3
3
2
3
2
2
2
1
2
2
3211
Tr :
Tr :
Tr :
mmmNN
mmmNN
mmmNN
++==++==++==
321
321
mmm
NNN
≅
Neutrinos: Mass Matrix:
lll MMM : L →=†
ννν MMM : N →= †
Miami-2008, 17 Dec 2008 Presented by: W. G. Scott, PPD/RAL. 17
6/)23( Det
)/2( Pr
Tr
321
3
1
2
2
1
1
LLLLmmmL
LLmmmmmmL
LmmmL
e
ee
e
+−==
−=++=
=++=
τµ
ττµµ
τµ
THE CHARACTERISTIC EQUATION
e.g. For the Charged-Lepton Masses:
0 ) (Det ) Pr( ) (Tr 23 =−+− LLL λλλwhere:
The Disciminant:
222
6
13
3
1
2
3
2
2
2
1
3212
4
1
3
2
2
) ()()(
6/3/432/7
62/32/
ee mmmmmm
LLLLLL
LLLLLLL
−−−=−−−−
+−=∆
ττµµ
All are Flavour-Symmetric and Jarlskog Invariant!!
Miami-2008, 17 Dec 2008 Presented by: W. G. Scott, PPD/RAL. 18
+++
+++
+++
==
LLL
L
L
3
1
3
1
3
1
z3
1y
3
1
3
1
x3
1w
3
1
3
1
)U(P2
xy)3(wzNL
T DetP Det)11( F
∆∆
(2) −===×=
)xy(wz)zyx(wz)yx(w1)/2P.P (Tr1) (1G 22222T(2) +−+++++++=−=×=
Flavour-Symmetric Mixing Observables…P.F. Harrison, D. R. J. Roythorn, and W. G. Scott, Phys. Lett. B 657 (2007) 210. arXive:0709.1439 [hep-ph]
Six New FS Variables (“Plaquette Invariants”)
A, B, C, D, F, G, analogous to Jarlskog J,
order (n) with odd/even symmetry under - scalar or pseudoscalar.
z)]wz(wy)[xy(x2
9wxy)wxzwyz9(xyz1) (1C (3) +++++++=×=
y)]xy(xz)[wz(w2
3y)]wz(xz)xy(wx)xz(z
y)yz(zy)wy(wx)3[wx(w)zyx2(w)11(A 3333(3)
+−+++−++−+
−+−+−++−−=×=
x)]yyxwzz(w2
1wyz-xyz-wxzwxy
yz-zywxx[w331)1( B
2222
2222(3)
−+−+++
−+=×=
y)]xxywzz(w2
1wxz-xyz-wyzwxy
xz-zxwyy[w33)1(1 D
2222
2222(3)
−+−+++
−+−=×=
/4FF/43GBDAC 2G2GFDCBA 32322222 +=++=+++Not all independent
)xS3(S3 νl
B, D are
not l ↔ν
symmetric
νl xS3S32 x 2 of
Miami-2008, 17 Dec 2008 Presented by: W. G. Scott, PPD/RAL. 19
−−−−++++
++−−
++−−
=
zx3
1yw
3
1zyxw
3
1
z3
1y
3
1zy
3
1
x3
1w
3
1xw
3
1
P
Plaquette Invariance (= Invariance)νl C3 x C3
xy-wzF/3 =
xy-wz
yzy-xy-yw- zyzwy yw
z)yxy(w-y)z)(w(yF/322
=−+++=
+++++=
“PLAQUETTE INVARIANT”!!!
Miami-2008, 17 Dec 2008 Presented by: W. G. Scott, PPD/RAL. 20
−++++−−−+−
−−−+++−+−−
+−−++
≈
9G
C
3G
A
G62
F
6
G
3
1
9G
2C
G6
F
3
1
9G
C
3G
A
G62
F
6
G
3
1
9G
C
3G
A
G62
F
6
G
3
1
9G
2C
G6
F
3
1
9G
C
3G
A
G62
F
6
G
3
1
9G
2C
6
G2
3
1
9G
4C
3
1
9G
2C
6
G2
3
1
P
Solving more generally for the P-matrix
Flavour-Symmetric Weak-Basis-Invariant Constraints on Mixing:
Democracy Symmetry
ie. one column=(1/3,1/3.1/3), iff: 0C 0F ==
“ µ–τ ” - Reflection Symmetry,
ie. two rows (or columns) equal, iff: 0A 0F ==
Tri-Bi-Maximal Mixing, iff: 0JACF ====
1/6G =in the limit F, A, C → 0 and 0 < G < 1/6, gives:
Miami-2008, 17 Dec 2008 Presented by: W. G. Scott, PPD/RAL. 21
Ansatz F G C A Symm. 18J B D
Tri-Bi-Max. 0 1/6 0 0 Dem., µτ, CP 0 0 1/12√3Tri-Max. Mix. 0 0 0 0 Dem., µτ 1/6 0 0Tri-χφ-Max. 0 - 0 - Dem.(ocracy) - 0 -2 Rows Eq. 0 - - 0 e.g. µ-τ - 0 -2 Cols. Eq. 0 - - 0 e.g. 1-2 - - 0Alt.-Feruglio 0 - (6G-1)/8 0 µτ, CP 0 0 -Tri-χ-Max. 0 - 0 0 Dem., µτ - 0 -Tri-φ-Max. 0 1/6 0 - Dem., CP 0 0 -Orig. Bi-Max. 0 1/8 -1/32 0 CP, µ-τ,1-2 0 0 0No Mixing 1 1 1 1 CP 0 0 0
Jarlskog J measures CP-violation (J=0 protects against violation of CP).
F measures the acoplanarity of the P-vectors in the flavour space
(F=0 => Det <P(∞)> = 0, i.e. protects distant source against flavour analysis)
G = 3<<Pll(∞)>>-1 measures the flavour-averaged asymptotic survival prob….
Miami-2008, 17 Dec 2008 Presented by: W. G. Scott, PPD/RAL. 22
=22211
22112
22111
2122122
21121
211
2121112
211
311
(3)
CC CC CC
CC CC CC
CC CC C
C
TrTrTr
TrTrTr
TrTrTr
C) NL
C
NL
T xy)3(wzP F
∆∆
(3)
∆∆3 Det (
DetDetDet ==−==
]N,i[LC nmmn −=Generalised Jarlskog Commutators:
The Matrix of Cubic Commutator Traces
The Jarlskog Commutator: N]i[L,C −=
3C C 3TrDet =controls CP violation:
=
222120
121110
020100
A A A
A A A
A A A
2
1T
TrTrTr
TrTrTr
TrTrTr
The Matrix of Anti-Commutator Traces(traces of mass-matrix products):
N,LA nmmn =And Anti-Commutators:
For example, F:
Directly in Terms of Mass Matrices: †
ννν
lll
MMMN
MMML
→=→=
†
In terms
of Mass
Matrices
only
Miami-2008, 17 Dec 2008 Presented by: W. G. Scott, PPD/RAL. 23
=
===
=
=
=
22122
21111
21
2m
1m
0m
NL TrNL TrL
NL TrNL TrL
NN3
T
2n 1n 0n
=22222222
222222
2222
]N,[L Tr]N,N][L,[L TrN],[L Tr
]N,][LN[L, Tr]N,N][L[L, TrN],N][L[L, Tr
]N[L, Tr]NN][L,[L, TrN][L, Tr
2
1 Q
==2
τ12
τ12
τ1
2µ1
2µ1
2µ1
2e3
2e2
2e1
2
3ν2ν 1ν
|U||U||U|
|U||U||U|
|U||U||U|
τ
µ
e
)U(P
nν
ml
nmmn m P. .mNL TrT ==
“Real Invariant Matrices and Flavour-Symmetric…”P.F. Harrison, W. G. Scott and T. J. Weiler, Phys. Lett. B 641 (2006) 372. hep-ph/0607336
==
τ3τ2τ1
µ3µ2µ1
e3e2e1
lν
3ν2ν 1ν
KKK
KKK
KKK
τ
µ
e
)(KK
νν1n
l1m
llTlmn ∆ ∆ diag )Σ (diag K )Σ (diag ∆ diag ∆ Q −−=
The “P-matrix”: ) lνP(WPlν →= “T-matrix”
“Q-matrix”
The “K-matrix”
Moment Transform:
Moment Transform:
*1ν 1l
*1ν 1l1ν 1l1ν 1llν
lνlν
UUUUΠ
ΠRe K
−++−++−−=
−=2)PPPP(PK 1ν 1l1ν 1l1ν 1l1ν 1llνlν +−−+++−− +−=
”permanent”
3) (mod
(invertible)
(invertible)
Miami-2008, 17 Dec 2008 Presented by: W. G. Scott, PPD/RAL. 24
FFTT .T.N.LT - .P..P 6F Tr -Tr =∈∈=
N .T..LT .PP 12G GGTT Tr Tr ==+
CCTT .Q.N.LT - .KP 612G32C Tr Tr =−=−−
AATT .Q.N.LT .K..P 2F-2A Tr Tr =∈∈=
CATT .Q.N.LT .K.P 32B Tr Tr =∈=
ACTT .Q.N.LT .K.P 32D Tr Tr =∈=
0.P.P .P.P TT ∈==∈ Tr Tr
011
101
110
−
−
−
=∈
Expressed as Traces
Two l ↔ν asymmetric cubic variables B,D:
No l ↔ν asymmetric quadratic variables:
Two quadratic variables G,Fentirely in terms of
Mass Matrices
Two l ↔ν symmetric cubic variables C,A:
etc. )L,L,(LLL 321GG =
Miami-2008, 17 Dec 2008 Presented by: W. G. Scott, PPD/RAL. 25
−
−
−
=
03L
30L
LL0
L
1 L
1
2
12
∆F
Expressed as Traces (cont.)
The Mass-Polynomial Matrices Requd:entirely in terms of
Mass Matrices
etc. )L,L,(LLL 321GG =
1
432
321
21
G
LLL
LLL
LL3
L
−
=
221
2231
414 LL2L3L4L6L L −++=
3 L0 =
Anti-symmetric Matrix
Symmetric Matrix
K
K
== L
L
A
C
-1G∆ L DetL =
Miami-2008, 17 Dec 2008 Presented by: W. G. Scott, PPD/RAL. 26
×
×
×
×
×
×
−+++
−−+−
+−−−
−+++
−−+−
+−−−
*1ν 1l1ν 1l
1ν 1l*
1ν 1l
*1ν 1l1ν 1l
*1ν 1l1ν 1l
1ν 1l*
1ν 1l
*1ν 1l1ν 1l
UU
UU
UU
UU
UU
UU
*1ν 1l1ν 1l
*1ν 1l1ν 1l
*1ν 1l1ν 1lI UUUUUU:Ω −++++−−−+−−−=
1/9 G1/3 C2/9 ΩΩoddeven
+−== ∑∑
*1ν 1l1ν 1l
*1ν 1l1ν 1llν UUUU: Π −++++−−−=
J i K: Π lνlν +−=
×
××
×
++−+
+−−−
1ν 1l*
1ν 1l
lν
*1ν 1l1ν 1l
UU
Π
UU
J 9i 1)/2- (G Πlν
lν +=∑ G)/2- (1 Klν
lν =∑
Flavour-Summed Loop Amplitudes
Usual Plaquette Product:4-Plaquette
Hexaplaquette Product:6-Plaquette
even odd
purely real
Miami-2008, 17 Dec 2008 Presented by: W. G. Scott, PPD/RAL. 27
More Flavour-Symmetric Constarints:
0AF)(CG27F8C 23 =−−
0DF)(BG27F8B 23 =−−
1/3|U| 2i =α
2i
2i |U||U| βα =
Completely Symmetric CKM P-matrix:
DB =2
i2
i |V||V| αα =
0|U| 2i =α
F/54FC/2754F27A K Det|K|
36F272C18G1081 J3
22
−−+==
−+−=
0J 0|K| 2 ==
0V 0V 0V 0V
JFCAJ)F,C,V(A,
JFCA
2222
=∂=∂=∂=∂+++=
Extremise a “Potential”, e.g.:
0JFCA ====
Tri-Bi-Maximal
Mixing !!!
oαi
2
90φ
0J 0|K|
≈⇒
→=!!!
Miami-2008, 17 Dec 2008 Presented by: W. G. Scott, PPD/RAL. 28
z yxAction =
EXTREMISATION: A TRIVIAL EXAMPLE
In the SM:
NOT BAD!!
><=><=><=
φφϕ
τ
µ
z
y
x
m
m
meGeV 180
2
v ≈=><φ
Add to SM Action, the determinant :
0 y
0
0
==∂==∂==∂
xA
zxA
zyA
z
y
x
0
0
0
≠==
z
y
x
τµ mmmL e Det =(taken here to be dimensionless) i. e.
zyx , ,Yukawa couplings
e.g.
P.F. Harrison and W. G. Scott Phys. Lett. B 333 (1994) 471. hep-ph/9406351
i.e. 2 zero mass
1 non-zero!
This notion appeared in:
Miami-2008, 17 Dec 2008 Presented by: W. G. Scott, PPD/RAL. 29
“Covariant Extremisation of Flavour-Symmetric….”
P.F. Harrison, and W. G. Scott Phys. Lett. B 628 (2005) 93. hep-ph/0508012
0 ]Ci[L, /3 C Tr
0]Ci[N, /3 C Tr T23
N
T23L
=+=∂
=−=∂
0 C]i[L, /2C Tr
0C]i[N, /2C Tr T2
N
T2L
=−=−∂
=+=−∂
/3C 3 TrExtremising:
Extremising: - /2C 2Tr
We extremise wrt Mass Matrices theselves:
N]i[L,C −=
ννν
lll
MM MN
MM ML
→=→=
†
†
The Jarlskog Commutator:
31
31
31
31
31
31
31
31
31
21
210
21
210
001
Extremising:
/2Cr/3C 23 Tr TrV(C) +=
0/3)CC /2)CC C)C 3223 =−+− TrTrTr (((Characteristic Equationn:
0C =Tr
3 x 3 Max
2 x 2 Max
)V(C“The Simplest Neutrino Mass Matrix”P. F. Harrison and W. G. Scott PLB 594 (2004) 324. hep-ph/0403278
C) Det=(
(=ΣPrincipal Minors C)
et
perms.
Miami-2008, 17 Dec 2008 Presented by: W. G. Scott, PPD/RAL. 30
( )X/ : X ∂∂=∂TX A AX Tr =∂
) N][L, i : C ( −=
0] ],[,[
],[F
/2F Tr A
c.f.
νµµ
νµ
2
=∇∇∇⇓
∇∇==
Mills-Yang / Maxell
Extremise wrt the Mass matrices themselves!
Exploit Matrix Calculus Theorem
0 ]Ci[L, /3 C Tr
0 ]Ci[N, /3 C Tr T23
N
T23L
=+=∂
=−=∂
Apply to Extremise Tr C³
Weak-Basis
Covariant !!
Apply to Extremise Tr C²
0 C]i[L, /2C Tr
0 C]i[N, /2C Tr T2
N
T2L
=+=∂
=−=∂
Where A is any constant matrix and X is a variable matrix.
Miami-2008, 17 Dec 2008 Presented by: W. G. Scott, PPD/RAL. 31
−+
+−
−+
==
cidxidy
idxbidz
idyidza
ν
ν
ν
MMN
ν ν ν
τ
µ
e
νν
τµe
The “Epsilon” Phase Convention*
The usual (charged-lepton) flavour basis
has not been completely defined.
There remains the freedom to re-phase the fields
such that he imaginary part of the neutrino mass
matrix is proportional to the epsilon matrix
Incredible but true!!
Now the 7 parameters a, b, c, d, x, y, z encode directly
the 3 neutrino masses and the usual 4 mixing parameters.
*See Footnote 1 of: “The Simplest Neutrino Mass Matrix”
P. F. Harrison & W. G. Scott Phys Lett. B B594 (2004) 324. hep-ph/0403278
†
=
00001111----1111
111100001111----
1111----11110000
εεεε
εεεε NNNN ImImImIm i.e.i.e.i.e.i.e. ×=d
“the epsilom matrix”:
Miami-2008, 17 Dec 2008 Presented by: W. G. Scott, PPD/RAL. 32
/2)C( Tr r /3)(C Tr V(C) 23 −+= N]i[L,C −=
Try a simple linear combination of the two:
)m)(mm(m
)md(mrdZ
Z
ZXY z
)m)(mm(m
)md(mrdY
Y
YZX y
)m)(mm(m
)md(mrdX
X
XYZ x
τµeτ
µe2
µeτµ
eτ2
eτµe
τµ2
−−
−−=±=
−−−
−=±=
−−
−−=±=
=
0.550.330.11
0.250.330.41
0.190.330.48
P
0.035h
GeV0.163 r/d 2
=→=
With the “Magic-Square constraint” imposed
there are analytical solutions:
Take r to be a constant with dimensions of (mass)²
In general, for sufficiently extreme hierarcy h → 0,
we are close to the pole at X →0, i.e. x→∞ and we have |x| >> y, z,
whereby the “Simplest” assumption must hold.
In this sense this V(C) above points to the “Simplest Neutrino Mass Matrix”
despite that in practice (in actuality!) the hierarchy h is too large!!
In practice:
X
Miami-2008, 17 Dec 2008 Presented by: W. G. Scott, PPD/RAL. 33
”The Simplest Neutrino Mass Matrix”
P. F. Harrison and W. G. Scott Phys Lett. B594 (2004) 324. hep-ph/0403278.
0.030.13
m3m2
χ sin 2/3sinθ
2atm
2sol
13
±≈∆∆=
=
+−−
−+−=
2
ci
6
s-
3
1
2
si
6
c2
ci
6
s-
3
1
2
si
6
c
s3
2
3
1c3
2
τ
µ
e
U
ν ν ν
χχχχ
χχχχ
χχ
321
[ ] 0Mν =,DDDD
“Democracy Symmetry”
=
111
111
111
DDDD
“Mu-Tau Reflection Symmetry” (“mutautivity”)
ννT M) M( =*
EEEEEEEE
=
010
100
001
EEEE
Finally, implementing the “Simplest” Condition:
In the charged-lepton flavour basis, ie. where lM Is diagonal, we impose:
the “democracyoperator”
Ie. commutes withνM
the “µτ-exchangeoperator”
Note definition includesa complex conjugation
ddddεεεεxxxxaIaIaIaIMMMMνννν ++= EEEE
Miami-2008, 17 Dec 2008 Presented by: W. G. Scott, PPD/RAL. 34
CONCLUSIONS
Again T. D. Lee’s lecture (a 2nd clip- from earlier in his talk)
Inspirational for anyone working on fermion mixing and flavour etc. :
“….these two 3 x 3 matrices (CKM and MNS) are the cornerstones
of particle physics… ….but do we understand them???”
1) “Tri-BiMaximal Mixing” has useful partners “Tri-χ-Maximal Mixing”,
and “Tri-φ-Maximal Mixing” and more generally “Tri- χφ-Maximal Mixing”
(now “ν2-Trimaximal Mixing”) which are also consistent with the data.
2) We have introduced 6 New Flavour-Symmetric Mixing Observables,
A,B,C,D,F,G which like the Jarlskogian J can be used to constrain
the mixings in an entirely flavour-symmetric way.
3) A programme of Extremisiing Flavour Symmetric Jarlskog Invariants,
Is under way with the aim of constraining both Mixings and Masses.
Thus far the best that can be said is that our results point towards
“The Simplest…” PLB 594 (2004) 324 (hep-ph/0403278) and Θ13 ~ 0.13.