Covariant and helicity formalisms - Indico · 2018. 11. 21. · Crossing symmetry in tensor...

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Covariant and helicity formalisms Alessandro Pilloni Joint Physics Analysis Center Salamanca – September 25, 2017 A. Pilloni Covariant and helicity formalisms 1/14

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

    ∞∑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

    ∞∑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

    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 =

    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