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1 Ground and excited states for exotic three-body atomic systems Lorenzo Ugo ANCARANI Laboratoire de Physique Moléculaire et des Collisions Université Paul Verlaine – Metz Metz, France FB19 - Bonn, 1 September 2009 Collaborators: Gustavo GASANEO and Karina RODRIGUEZ Universidad Nacional del Sur, Bahia Blanca, Argentine Dario MITNIK Universidad de Buenos Aires, Buenos Aires, Argentine
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2 OUTLINE Generalities Angularly correlated basis Results for three-body exotic systems - ground state - excited states Simple function – predictive tool for stability Concluding remarks
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3 m 3,z 3 : heaviest and positively charged m 2,z 2 : light and negatively charged m 1,z 1 : lightest and negatively charged m 1,z 1 m 2,z 2 r 13 r 23 m 3,z 3 m 3,z 3 r 12 THREE-BODY PROBLEM OF ATOMIC SYSTEMS BOUND STATES REDUCED MASSES: Schrödinger Equation No analytical solution !
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4 z 3 =1 z 3 =2
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5 NO ANALYTICAL SOLUTION CONSTRUCTION OF A TRIAL WAVAFUNCTION ANALYTICAL - SIMPLE (few parameters) - GOOD FUNCTIONAL FORM - ENERGY : not so good (ground state) NUMERICAL - VERY LARGE number of parameters - Functional form ? - ENERGY: very good (ground state) INTERMEDIATE (compromise) - Limited number of parameters - Functional form ? - ENERGY: good (also excited states?) - Practical for applications (e.g. collisions)
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6 (e,3e) e-e- kiki k0k0 e-e- k1k1 e-e- k2k2 e-e- A Initial channel Final Channel DOUBLE IONISATION : (e,3e) e - + He He ++ + e - + e - + e - HeHe e - (E i,k i ) e - (E 0, k 0 ) e - (E 2, k 2 ) e - (E 1, k 1 ) He ++ 4-body problem (6 interactions) Detection in coincidence: FDCS
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7 Momentum transfer : Interaction 3-body BOUND problem Ground state of He 3-body CONTINUUM problem First Born Approximation (FBA) r1r1r1r1 e-e-e-e- r2r2r2r2 e-e-e-e- He 2+ (Z=2) r 12
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8 Asymptotic behaviour - one particle far away from the other two - all particles far away from each other Close to the two-body singularities (r 13 =0, r 23 =0, r 12 =0) (Kato cusp conditions) Important for calculations of - double photoionization (Suric et al, PRA, 2003) - expectation values of singular operators (annihilation,Bianconi, Phys lett B,2000) Triple point (all r ij =0) FUNCTIONAL FORM OF WF
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9 (Garibotti and Miraglia, PRA (1980); Brauner, Briggs and Klar, JPB (1989)) C3 MODEL FOR DOUBLE CONTINUUM Sommerfeld parameters: - Correct global asymptotic behaviour - OK with Kato cusp conditions ANGULARLY CORRELATED BASIS
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10 Non-relativistic Schrödinger Equation No analytical solution ! S states - Hylleraas Equation : 3 interparticle coordinates
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11 DOUBLE BOUND FUNCTIONS ANALOG TO THE C3 DOUBLE CONTINUUM (Ancarani and Gasaneo, PRA, 2007) For two light particles 1,2 (z 1 0) r 13 r 23 m 3,z 3 m 3,z 3 r 12 m 1,z 1 m 2,z 2
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12 ANGULAR CORRELATED CONFIGURATION INTERACTION (ACCI) (Gasaneo and Ancarani, PRA, 2008) By construction: - Angularly correlated (r 12 ) - Parameter-free: three quantum numbers (n 1, n 2, n 3 ) - OK with Kato cusp conditions Basis functions:
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13 CALCULATIONS of - energies of ground and excited states - mean values of with p>0 or <0 ALL RESULTS are in Hartree atomic units (ENERGY:1 a.u.=27.2 eV) SELECTION: compared to « numerically exact » values when available (obtained with hundreds/thousands of variational parameters)
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14 RESULTS (infinite m 3 ): GROUND STATE Configurations included: 1s1s+(1s2s+2s1s)+2s2s Angular correlation: n 3 up to 5 M = number of linear coefficients
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15 RESULTS (infinite m 3 ): EXCITED STATES (Gasaneo and Ancarani, PRA, 2008) All states obtained - form an orthogonal set - satisfy two-body Kato cusp conditions Good energy convergence Can be systematically be improved by increasing M Even get the doubly excited state: 2s 2 1 S ( E (M=20) =-0.7659 )
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16 RESULTS (finite m 3 ): GROUND AND EXCITED STATES Configurations included: 1s1s+(1s2s+2s1s)+(1s3s+3s1s)+2s2s and n 3 =1,2,3,4,5 M=30
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17 RESULTS (finite m 3 ): GROUND AND EXCITED STATES Configurations included: 1s1s+(1s2s+2s1s)+(1s3s+3s1s) and n 3 =1,2 M=10
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18 ACCI WITH EXTRA CORRELATION Same methodology (only linear parameters, analytical, …) Set of orthogonal functions, satisfying Kato cusp conditions Even better energy convergence (method suggested by Rodriguez et al., JPB 2005+2007) (Drake, 2005)
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19 ACCI WITH EXTRA CORRELATION (Rodriguez, Ancarani, Gasaneo and Mitnik, IJQC, 2009) (Frolov, PRA, 1998) GROUND STATE: only 1s1s included (n 1 =n 2 =1) and n 3 =1,2
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20 ACCI WITH EXTRA CORRELATION (Rodriguez, Ancarani, Gasaneo and Mitnik, IJQC, 2009) (Frolov, PRA, 2000) (Drake, 2005) GROUND STATE: only 1s1s included (n 1 =n 2 =1) and n 3 =1,2
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21 ACCI WITH EXTRA CORRELATION (Rodriguez, Ancarani, Gasaneo and Mitnik, IJQC, 2009) (Frolov, Phys.Lett. A, 2006) (Drake, 2005) GROUND STATE: only 1s1s included (n 1 =n 2 =1) and n 3 =1,2
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22 ACCI WITH EXTRA CORRELATION (Rodriguez, Ancarani, Gasaneo and Mitnik, IJQC, 2009) GROUND STATE: only 1s1s included (n 1 =n 2 =1) and n 3 =1,2 D. Exotic systems : n=1: positronium Ps- n ∞ : negative Hydrogen ion H-
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23 (Frolov and Yeremin, JPB, 1989) Ps- H- (Rodriguez et al, Hyperfine Interactions, 2009)
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24 SIMPLE FUNCTION WITHOUT PARAMETERS Pedagogical Without nodes With both radial (r 1,r 2 ) and angular (r 12 ) correlation Satisfies all two-body cusp conditions Sufficiently simple: analytical calculations of c opt (Z) and mean energy E(Z) Without parameters (only Z); Rather good energies, and predicts a ground state for H - !! No ground state for H - !! r1r1r1r1 r2r2r2r2 Z r 12 e- e- e- (Ancarani, Rodriguez and Gasaneo,JPB, 2007)
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25 r1r1r1r1 r2r2r2r2 r 12 GENERALISATION TO THREE-BODY SYSTEMS 3 masses m i and 3 charges z i : Reduced masses: Same properties (in particular: analytical!) Same form for any system m1,z1 m1,z1 SIMPLE FUNCTION WITHOUT PARAMETERS m2,z2 m2,z2 m3,z3 m3,z3 (Ancarani and Gasaneo,JPB, 2008)
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26 z 3 =1 z 3 =2 (Ancarani and Gasaneo,JPB, 2008)
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27 PREDICTIVE CHARACTER STABILITY OF EXOTIC SYSTEMS 3 masses m i and 3 charges z i : with m 1 the lightest Stability condition: Example: m 1 =m 2 et z 1 =z 2 z 2 /z 3 = -1 Critical charge for a given r : Nucleus of virtual infinite mass: (Ancarani and Gasaneo,JPB, 2008)
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28 … L>0 states … atomic systems with N > 3 bodies … molecular systems Summary Future
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29 Thanks for listening
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32 Optimisation d ’ une fonction d ’ essai Energie moyenne: Variance: Autres valeurs moyennes: Th é or è me du Viriel: Valeurs moyennes: Energie locale: Fluctuations moyenn é es
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