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The Weak Production of Hypernuclei D.D. van Niekerk (M.Sc. project) B.I.S. van der Ventel G.C. Hillhouse Department of Physics Stellenbosch University South Africa
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Stellenbosch, South Africa
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Outline Motivation Our Model Formalism The Hadronic Vertex Kinematics The Transition Matrix Leptonic Tensor Hadronic Tensor Constructing W µ (Example) Conclusion
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Motivation Recent large scale interest in astrophysics and the role of neutrinos in stellar processes (i.e. supernovae) Neutrino osscillations (changing of flavour) BooNE / MiniBooNE (Fermilab)MiniBooNE J-PARC Super-Kamiokande (50 GeV) Super-Kamiokande Nucleon decay postulated by supersymmetry Hyperon and hypernuclei production form important part of neutrino- induced reaction cross sections
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Our Model Based on relativistic Dirac equation never been studied (nuclear process) first attempt in a fully relativistic framework Quasifree process (interaction takes place between neutrino and single bound nucleon) Bound state wave functions are calculated using relativistic mean field formalism Aim: Obtain quantitive results that will give indication of nuclear model uncertainties Provide theoretical basis for interpretation of experimental results
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Types of Reactions: Charged Current (CC) (S = strangeness) ΔS = 0 ΔS = 1 Neutral Current ΔS = 0 ΔS = 1 not observed
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Formalism Neutral Current (NC)Charged Current (CC)
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Modelling the Hadronic Vertex Quasifree Region Use form factors bound hyperon bound nucleon Vertex Approximation
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K is kinematic factor determined from normalisation of flux etc. First order diagram: L μν contains projectile information W μν contains nuclear information
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Kinematics CC In CC reactions we can detect the outgoing muon.
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Kinematics NC In NC reactions we cannot detect the outgoing neutrino.
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Transition Matrix Element Leptonic Current Parity not conserved Left-handed neutrinos Propagator Vector Boson (W + or Z 0 ) Coupling strengths follow from GSW Theory (η l and η h )
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Leptonic Tensor Lepton spinor normalised as helicity representation Neutrino: m = 0 and h = -1 Feynman trace techniques and identities of the gamma matrices can be used to simplify the expression for L μν
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Hadronic Tensor The hadronic tensor is expanded in a basis consisting of the independent four-momenta, the metric tensor and the Levi-Civita tensor
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This expansion is model independent The W i expansion coefficients are the structure functions Extract W i : done once
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The contraction of hadronic and leptonic tensors is done considering symmetric and anti-symmetric contractions separately General equation Model is needed for guidance
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Construction of h µ Born Term Model (s,t and u channels) Propagators: spin ½ spin 0 Vertices: Strong coupling (baryon-baryon-meson) in s,t,u channels Coupling constant Weak coupling (meson-meson) in t channel Phenomenological meson form factors Mecklenberg W., Acta Physica Austriaca 48, 293 (1976) Weak coupling (baryon-baryon) in s,u channel Form factors Weak Current Operator
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s t u Elementary process:
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s-channel neutron-proton vertex Form Factors
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CVC relates weak vector form factors to isovector form factors of EM current EM isovector current Axial form factor determined phenomenologically
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Total (for s-channel)
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u-channel Vertex: Weak current i.t.o. SU(3) octet currents
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where and λ i = 3X3 generators of SU(3) γ μ = 4X4 Dirac matrices
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EM current For O j any octet current operator For EM current Comparison yields
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For weak current Belongs to same octet as EM current Axial form factor From s-channel
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u-channel weak baryon-baryon vertex: propagator: strong baryon-baryon-meson vertex:
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Total (for u-channel)
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Summary
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Conclusion We are constructing a relativistic model for the description of weak hypernuclei production of relevance to experiments at Fermilab (BooNE) and J-PARC Hadronic tensor parametrised in model independent way to facilitate different hadronic models through structure functions Code written in Fortran 95 and Mathematica. In process of obtaining results: We are investigating the relation between the structure functions W i and the kaon scattering angle as well as dependence of Wi on the momentum transfer Calculate the cross section email: ddvniekerk@sun.ac.za
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