dipole moments

Electric Dipole moments as probes of physics beyond the Standard Model K. V. P. Latha Non-Accelerator Particle Physics Group Indian Institute of Astrophysics Plan of the Talk Parity (P) and Time-reversal (T) operations
Electric Dipole moments (EDMs) as consequences of P&T violations
Sources of EDMs in atoms
Experiments to measure EDMs – basic principle
Closed-shell atoms – dominant interactions
Calculation of EDMs – Requirement of atomic theory
Present Limits and Implications for Particle Physics
Conclusions Parity and Time-reversal transformations Parity operation X Y-X -Z-YZ Time reversal operationJ J + - + + +- -- P & T violation for a non-zero EDM Angular momentum + - + + +- - - -Physical system edmP T Quantity P T D - D + D σ + σ − σ D = D “ D = -D “ D = -D “Non-zero EDMs are direct evidence for Parity and Time-reversal violations Sources of EDMs in atoms Elementary Nucleon Nuclear Atomic particle de Da (open) Scalar-pseudo scalar e-q e-N e-Nuc Da (open) Tensor-pseudo tensor Da (closed) dq dN dNuc Da (closed) q-q dN, N-N dNuc Da Da is measured by atomic experiments Da / C , (C = CT , CS , or Q) is calculated using atomic theory, C is the coupling constant of the corresponding interaction, Compare theory and experiment and extract the value of ' C ' . Principle of measurement of EDM B
E B  E 2    B 2D   E B E 2  B 2D E  4DE  If D~10 -24 e-cm and =10 3 V/cm E~ 10 -3 HzB E  Closed-shell atoms with non-zero total angular momentum are sensitive to Nuclear Schiff moment Tensor-pseudo tensor e-N interactions Examples : 199 Hg , 171 Yb, 129 Xe - No contribution from the J of the electrons Closed-shell atoms Nuclear Schiff moment The total charge density of the nucleus is ρ(r) = ρ0(r) + δρ(r) P, T violating interactionRr OR ± r The total nuclear potential at a point R from the origin is, where nuclear electric dipole moment. Is the The nuclear potential that is first order in the T and P violating interaction is The above equation can be expressed as where R and r are the electron and nuclear coordinates respectively. After simplification, The interaction of the potential containing the Schiff moment with an electron in an atom is given by where Q depends on ’ρ0 ( r ) , δρ ( r ) and quantities related to them. Tensor-pseudo tensor e-N interaction The P and T violating T-PT electron-nucleon interaction is Where CT Is the T-PT coupling constant, GF is the Fermi constant = 2.22 10-14 a.u, σ µν, γ 5 are built from the Dirac matrices, © I © is the nuclear spin. The matrix elements of the He-N operator ~ Z2, hence heavy elements are preferred. => Relativistic many-body theory required. Many-body theory to calculate D a / C Required are Knowledge of the Hamiltonian of the system Accurate relativistic electronwavefunctions Ha = Dirac Hamiltonian for a many-electron atom = i ( C  i . p i + ‚ m c2 - Z e2 / r i ) + i<j e2 / rij Coulomb interaction= unperturbed Hamiltonian In the presence of a P, T violating interaction, H = Ha + C H PTV The Schroedinger equation for an exact atomic state is H| ™ψ > = Ε | ™ψ >Where | ™ψ > = | ™ψ(0) > + C | ™ψ (1) > Unperturbed wavefunctionFirst-order perturbed wavefunction | ™ψ (0) > ©s are obtained by solving the unperturbed Schroedinger equation, Ha | ™ψ (0) > = Ε (0) | ™ψ (0) > The perturbed Schroedinger equation hence becomes, ( Ha - E(0) ) | ™ψ (1) > = − H PTV | ™ψ (0) > The atomic EDM is given by = Expectation value of the Electric Dipole Operator. Hence Da < ψ (0) | D | ψ (1) > + < ψ (1) | D | ψ (0) >/ C = (< ψ (0) | ψ (0) >) | ψ (0) > is calculated by atomic many-body methods. Many -body perturbation theory Configuration Interaction Coupled-cluster theoryDa = < ψ | D | ψ > / < ψ | ψ > Present Limits And Implications For Particle Physics The limits for EDM of Hg induced by the Nuclear Schiff moment are Da / Q = -2.8 * 10-27 e-cm / (e fm3) (PRA 66, 012111 (2002)) And for | D (Hg) | < 2.1 * 10-28 e-cm Gives the upper limit for Q as -7.5 10-2 e-fm3 To derive the CP violating coupling constants at the quark level from this limit on Q, nuclear structure calculations are necessary. The Schiff moment of Hg is primarily sensitive to the S-PS interaction between the proton and the neutron. This interaction is parametrized in terms of ξ , which is related to Q by Q = -1.8 . 10-7 ξ e. fm3 This gives the constraint on ξ. From ξ, the upper limit on the quark-chromo EDMs is Limit for the T-PT electron-nucleus coupling constant, C T = 1 * 10-8 We need nuclear structure and particle theory to deduce CT for electron-nucleon and electron-quark interactions. DYb = 4.75 CT σ N * 10-12 e a0 ( Angom Dilip et. al. Jphys ± B, 34, 3089(2001) ) Electron EDM can also be deduced from closed shell atoms by considering the hyperfine interaction as a perturbation. The EDM of an electron, as predicted by the Standard model of Particle physics in comparison with other models : Model de e-cm Standard Model < 10 -38 SUSY Multi-Higgs Left-right asymmetric10 -26 ± 10 -28Implications for Particle Physics | D Tl | < 9.4 * 10-25 e-cm and comparing theory and experiment gives de (tl) < 1.6 * 10-27 e-cm ( PRL, 88 (071805) (2002) ) is consistent with the predictions of the non-standard models. The current best limit for the EDM of an electron is obtained from the experiment on Tl atom, Conclusions Presence of EDMs is a direct evidence of T ± violation. The knowledge of the T ± PT coupling constants and the Schiff moment, Q gives deep insights into the interactions responsible for them. P & T violation for a non-zero EDM Non-zero EDMs are direct evidence for Parity and Time-reversal violations Electrons are assumed to move independently of each other in an average field due to the nucleus and the other electrons. Residual interaction is treated as the perturbation The exact two-body interaction is approximated by an average one-body body interaction. The many-electron anti-symmetric wavefunction in IPM is a Slater determinant φ = The single particle orbitals are determined by using Variational principle which leads to Hartree Fock equations. Ves = i<j e 2 / r ij - i U i ( r i ) , U i ( r i ) = Hartree-Fock potential ; Ves is treated as perturbation.Independent particle model ± starting point 1 / N! Configuration interaction method The many-body wave function is expanded as a linear combination of determinantal wavefunctions, where the coefficients of various deter- minants are found using Variational principle. These determinants include HF reference state Singly excited determinant Doubly excited determinant identified by the total angular momentum J and it©s projection MJ. Therefore, the CI wavefunction is given by Many-body perturbation theory Different orders of perturbation are introduced in a systematic way MBPT takes care of all the excitations upto a given order of perturbation Residual Coulomb interaction is treated as a perturbation The wavefunction in MBPT in terms of the perturbation parameter is | ψ MBPT > = | φ > + λ | φ (1) > + λ2 | φ (2) > + ......... | φ > | φar > = CS | φ S > | φabrs > = CD | φ D > Coupled-cluster theory Decomposing the wavefunction of the wavefunction of a many-particle system in terms of amplitudes for exciting clusters of a finite number of particles. Let | ψ > be the exact wave function and | φ > be the reference state. In CCT, | ψ > = eT | φ > The problem of finding these coefficients reduces to the diagonalisation of the total Hamiltonian in the space of configurations. Hence the CI equation can be cast in the form H C = E C and solved for the energies and the coefficients. Where T = excitation operator | φ > = Reference state| ψ CI > = C 0 | φ > + Σ S CS | φ S > + ........