Covariant and helicity formalisms - Indico · 2018. 11. 21. · Crossing symmetry in tensor...
Transcript of Covariant and helicity formalisms - Indico · 2018. 11. 21. · Crossing symmetry in tensor...
-
Covariant and helicity formalisms
Alessandro Pilloni
Joint Physics Analysis Center
Salamanca – September 25, 2017
A. Pilloni Covariant and helicity formalisms 1/14
-
Recipes to build an amplitude
The literature abounds with discussions on the optimal approachto construct the amplitudes for the hadronic reactions
I Helicity formalismJacob, Wick, Annals Phys. 7, 404 (1959)
I Covariant tensor formalismsChung, PRD48, 1225 (1993)Chung, Friedrich, PRD78, 074027 (2008)Filippini, Fontana, Rotondi, PRD51, 2247 (1995)Anisovich, Sarantsev, EPJA30, 427 (2006)
The common lore is that the former one is nonrelativistic,especially when expressed in terms of LS couplingsand the latter takes into account the proper relativistic corrections
A. Pilloni Covariant and helicity formalisms 2/14
-
How helicity formalism works
I Helicity formalism enforces the constraints about rotationalinvariance
I It allows us to fix the angular dependence of the amplitudeI What about energy dependence?
Example: Λb → ψΛ∗ → pK
ΛΛ
μ
μ
μ
μ
ψ
ppKKθ θ
φ
θ
*
+
−
+
−K − −ψ Λ
Λ
b
*ψ *
φ = 0
Λ
Λ
φ μψ*
Λ
b
lab frame
rest frame0
0
rest frame
∗
x
z
b
Λ
rest frame
LHCb, PRL115, 072001 (2015)
Each set of angles is defined in a different reference frameA. Pilloni Covariant and helicity formalisms 3/14
-
How helicity formalism works
I Helicity formalism enforces the constraints about rotationalinvariance
I It allows us to fix the angular dependence of the amplitudeI What about energy dependence?
Example: Λb → ψΛ∗ → pK
MΛ∗λΛ0b, λp ,∆λµ ≡
∑n
∑λΛ∗
∑λψ
HΛ0b→Λ
∗n ψ
λΛ∗ , λψD
12λΛ0b, λΛ∗−λψ(0, θΛ0b
, 0)∗
HΛ∗n→Kpλp , 0
DJΛ∗nλΛ∗ , λp
(φK , θΛ∗ , 0)∗
RΛ∗n (mKp)D1λψ ,∆λµ
(φµ, θψ, 0)∗,
LHCb, PRL115, 072001 (2015)
Each set of angles is defined in a different reference frameA. Pilloni Covariant and helicity formalisms 3/14
-
How tensor formalisms work
The method is based on the construction of explicitly covariantexpressions.
I To describe the decay a→ bc, we first consider thepolarization tensor of each particle, εiµ1...µji
(pi )
I We combine the polarizations of b and c into a “total spin”tensor Sµ1...µS (εb, εc)
I Using the decay momentum, we build a tensor Lµ1...µL(pbc) torepresent the orbital angular momentum of the bc system,orthogonal to the total momentum of pa
I We contract S and L with the polarization of a
Tensor ×RX (m) which contain resonances and form factors
A. Pilloni Covariant and helicity formalisms 4/14
-
What do we know?
I Energy dependence is not constrained by symmetry
I Still, there are some known properties one can enforce
RX (m) =B′LXΛ0b
(p, p0, d)
(p
MΛ0b
)LXΛ0b
BW(m|M0X , Γ0X )B ′LX (q, q0, d)(
q
M0X
)LXI Kinematical singularities: e.g. barrier factors (known)
I Left hand singularities (need model, e.g. Blatt-Weisskopf)
I Right hand singularities = resonant content (Breit Wigner,K-matrix...)
A. Pilloni Covariant and helicity formalisms 5/14
-
Kinematical singularities
I Kinematical singularities appear because of the spin of theexternal particle involved
I We can write the most general covariant parametrization ofthe amplitude astensor of external polarizations ⊗ scalar amplitudes
I Scalar amplitudes must be kinematical singularities free
I They can be matched to the helicity amplitudes
I We can get the minimal energy dependent factor
I Any other additional energy factor would be model-dependent
A. Pilloni Covariant and helicity formalisms 6/14
-
Crossing symmetry in tensor formalisms
I The process B → D̄ππ is composed of scalar particles onlyLHCb, PRD92, 032002 (2015)
I One defines the helicity angle in the isobar rest frame, thenthe amplitude is Lorentz Invariant
I Let’s consider the ρ intermediate state, B → D̄ρ(→ ππ)
A =m2B + s −m2D
2m2Bcos θ × qp = E
(B)ρ
mBcos θ × qp
I The factors p and q are the L = 1 expected barrier factors.The additional factor is analytical in s, not a kinematicalsingularity. Why is it there?
A. Pilloni Covariant and helicity formalisms 7/14
-
Crossing symmetry in tensor formalisms
B
D̄ π2
π1
L = 1ρ
L = 1
The tensor amplitude is given by
p(B)D · p
(ρ)π , where p
(B)D is the
breakup momentum in the B
frame, and p(ρ)π the decay
momentum in the isobar frame
A =m2B0 + s −m
2h3
2m2B0
pq cos θ
B
D π2
π1
L = 1ρ
L = 1
However, one can consider thescattering process just in theisobar rest frame.
A = pq cos θ
By crossing symmetry theamplitudes must be the same.
The usual implementation fails crossing symmetry
A. Pilloni Covariant and helicity formalisms 8/14
-
Example: B → ψπK
To consider the effect of spin, let’s consider B → ψπKWe focus on the parity violating amplitude for the K ∗ isobars,scattering kinematics
B(0+)
ψ(1−)
K(0−)
π(0−)
K∗(0+, 1−...)
ψ
π
B
Kp2
p1p3
p4
θs
p =λ
1/212
2√s, q =
λ1/234
2√s, zs =
s(t − u) + (m21 −m22)(m23 −m24)λ
1/212 λ
1/234
A. Pilloni Covariant and helicity formalisms 9/14
-
Helicity amplitude
Aλ =1
4π
∞∑j=|λ|
(2j + 1)Ajλ(s) djλ0(zs)
d jλ0(zs) = d̂jλ0(zs)ξλ0(zs), ξλ0(zs) =
(√1− z2s
)λd̂ jλ0(zs) is a polynomial of order j − |λ|
A. Pilloni Covariant and helicity formalisms 10/14
-
Helicity amplitude
Aλ =1
4π
∞∑j=|λ|
(2j + 1)Ajλ(s) djλ0(zs)
d jλ0(zs) = d̂jλ0(zs)ξλ0(zs), ξλ0(zs) =
(√1− z2s
)λd̂ jλ0(zs) is a polynomial of order j − |λ|The kinematical singularities of Ajλ(s) can be isolated by writing
Aj0 =m1p√s
(pq)j Âj0 for j ≥ 1,
Aj± = q (pq)j−1 Âj± for j ≥ 1,
A00 =p√s
m1Â00 for j = 0,
A. Pilloni Covariant and helicity formalisms 10/14
-
Identify covariants
Two helicity couplings → two independent covariant structuresImportant: we are not imposing any intermediate isobar
Aλ(s, t) = εµ(λ, p1)
[(p3 − p4)µ −
m23 −m24s
(p3 + p4)µ
]C (s, t)
+ εµ(λ, p1)(p3 + p4)µB(s, t)
A. Pilloni Covariant and helicity formalisms 11/14
-
Identify covariants
Two helicity couplings → two independent covariant structuresImportant: we are not imposing any intermediate isobar
C (s, t) =1
4π√
2
∑j>0
(2j + 1)(pq)j−1Âj+(s) d̂j10(zs)
B(s, t) =1
4πÂ00 +
1
4π
4m21λ12
∑j>0
(2j + 1)(pq)j
×
[Âj0(s)d̂
j00(zs) +
s + m21 −m22√2m21
Âj+(s) zs d̂j10(zs)
].
Everything looks fine but the λ12 in the denominatorThe brackets must vanish at λ12 = 0⇒ s = s± = (m1 ±m2)2,Âj+ and Â
j0 cannot be independent
A. Pilloni Covariant and helicity formalisms 11/14
-
General form and comparisons
Âj+ = 〈j − 1, 0; 1, 1|j , 1〉gj(s) + fj(s)
Âj0 = 〈j − 1, 0; 1, 0|j , 0〉s + m21 −m22
2m21g ′j (s) + f
′j (s)
gj(s±) = g′j (s±), and fj(s), f
′j (s) ∼ O(s − s±)
All these four functions are free of kinematic singularity.
A. Pilloni Covariant and helicity formalisms 12/14
-
General form and comparisons
Âj+ = 〈j − 1, 0; 1, 1|j , 1〉gj(s) + fj(s)
Âj0 = 〈j − 1, 0; 1, 0|j , 0〉s + m21 −m22
2m21g ′j (s) + f
′j (s)
gj(s±) = g′j (s±), and fj(s), f
′j (s) ∼ O(s − s±)
All these four functions are free of kinematic singularity.
Comparison with ordinary LS
gj(s) = g′j (s)
s + m21 −m222m1√s
=
(2j − 12j + 1
)1/2Ĝ jj−1(s),
fj(s) =m1√sf ′j (s) = p
2
(2j + 3
2j + 1
)1/2Ĝ jj+1(s).
If the Ĝ jL are the usual Breit-Wigner, the g′, f ′ have singularities
A. Pilloni Covariant and helicity formalisms 12/14
-
General form and comparisons
Âj+ = 〈j − 1, 0; 1, 1|j , 1〉gj(s) + fj(s)
Âj0 = 〈j − 1, 0; 1, 0|j , 0〉s + m21 −m22
2m21g ′j (s) + f
′j (s)
gj(s±) = g′j (s±), and fj(s), f
′j (s) ∼ O(s − s±)
All these four functions are free of kinematic singularity.
Comparison with tensor formalisms (j = 1)
Aλ = εµ(λ, p1)
(−gµν + P
µPν
s
)Xν(q)gS(s)
+ ερ(λ, p1)Xρµ(p)
(−gµν + P
µPν
s
)Xν(q)gD(s)
A. Pilloni Covariant and helicity formalisms 12/14
-
General form and comparisons
Âj+ = 〈j − 1, 0; 1, 1|j , 1〉gj(s) + fj(s)
Âj0 = 〈j − 1, 0; 1, 0|j , 0〉s + m21 −m22
2m21g ′j (s) + f
′j (s)
gj(s±) = g′j (s±), and fj(s), f
′j (s) ∼ O(s − s±)
All these four functions are free of kinematic singularity.
Comparison with tensor formalisms (j = 1)
g1 = g′1 =
4π
3gS , f1 =
2πλ123s
gD , f′
1 = −4πλ12
3s
s + m21 −m22m21
gD .
If the gS , gD are the usual Breit-Wigner, the g′, f ′ are fine
but for singularities at s = 0
A. Pilloni Covariant and helicity formalisms 12/14
-
Few words on form factors and Blatt-Weisskopf
I Left hand singularities are due to dynamics →model-dependent!
I They originate from the cross-channel exchanges in scatteringprocesses
I These singularities are far from the physical region, but modifythe high-energy behaviour (e.g. suppress the barrier factors)
I In nonrelativistic potential theory, they can be univocallycalculated depending on the potential shape, e.g.Blatt-Weisskopf for square well+centrifugal potential
I Best practice: explore different form factor models,check the stability of the resonant parameters
A. Pilloni Covariant and helicity formalisms 13/14
-
Conclusions
I There is no God-given recipe to build the right amplitude, butone can ensure the right singularities to be respected
I The LS couplings are perfectly relativistic, although the naiveimplementation fails to respect the analyticity requirements
I The tensor formalisms have some of the right features, butexplicitly violates crossing symmetry
Misha Mikhasenko, Tomasz Skwarnicki, Adam Szczepaniak
A. Pilloni Covariant and helicity formalisms 14/14