36
Andrey Shirokov (Moscow State Univ.) In collaboration with Alexander Mazur (Pacific National Univ.) Pieter Maris and James Vary (Iowa State Univ.) INT, Seattle, June 8, 2011

Resonant states in the shell model

  • Upload
    dyllis

  • View
    40

  • Download
    4

Embed Size (px)

DESCRIPTION

Resonant states in the shell model. Andrey Shirokov (Moscow State Univ.) In collaboration with Alexander Mazur (Pacific National Univ.) Pieter Maris and James Vary (Iowa State Univ.). INT, Seattle, June 8, 2011. - PowerPoint PPT Presentation

Citation preview

Page 1: Resonant states in the shell model

Andrey Shirokov (Moscow State Univ.)In collaboration withAlexander Mazur (Pacific National Univ.)Pieter Maris and James Vary (Iowa State Univ.)

INT, Seattle, June 8, 2011

Page 2: Resonant states in the shell model

*Conventional: bound state energies are associated with variational minimum in shell model, NCSM, etc., calculations*Is it also true for resonant states? Can we get resonance

width from such calculations?

Page 3: Resonant states in the shell model

*Resonant states: should we, probably, study excitation energies instead? Or the energies E = EA − EA − 1 for n−(A−1) scattering (or, generally, with A1 + A2 = A)? *Is it important for them to be stable with respect to ħΩ or Nmax

variation?

Page 4: Resonant states in the shell model

*Would be nice to have a simple answer from conventional calculations without doing, say, complicated NCSM−RGM calculations.*So, what are the general properties of eigenstates in continuum

consistent with resonance at the energy Er and width Γ?*Some observations, examples follow; this is still work in progress.

Page 5: Resonant states in the shell model

*So, what are the general properties of eigenstates in continuum consistent with resonance at the energy Er and width Γ?*Some observations, examples follow; this is still work in progress. *I discuss some general properties for oscillator basis calculations;

this is the only relavance to NCSM

Page 6: Resonant states in the shell model

*O.Rubtsova, V.Kukulin, V.Pomerantsev, JETP Lett. 90, 402 (2009); Phys. Rev. C 81, 064003 (2010):*I.M.Lifshitz (1947):

Page 7: Resonant states in the shell model

*O.Rubtsova, V.Kukulin, V.Pomerantsev, JETP Lett. 90, 402 (2009); Phys. Rev. C 81, 064003 (2010):*I.M.Lifshitz (1947):

So, the phase shift at the eigenenergies Ej can be easily calculated!

Page 8: Resonant states in the shell model

*O.Rubtsova, V.Kukulin, V.Pomerantsev, JETP Lett. 90, 402 (2009); Phys. Rev. C 81, 064003 (2010):*I.M.Lifshitz (1947):

Unfortunately, this does not work:The dimensionality of the matrix is small, the average spacing between the levels is not well-defined.One needs sometimes Dj value below the lowest Ej

0

Page 9: Resonant states in the shell model

Direct and inverse problem

Page 10: Resonant states in the shell model
Page 11: Resonant states in the shell model
Page 12: Resonant states in the shell model
Page 13: Resonant states in the shell model
Page 14: Resonant states in the shell model
Page 15: Resonant states in the shell model

*J-matrix inverse N-nucleus scattering analysis suggests values for resonant and non-resonant states that should be compared with that obtained in NCSM

Page 16: Resonant states in the shell model
Page 17: Resonant states in the shell model
Page 18: Resonant states in the shell model
Page 19: Resonant states in the shell model
Page 20: Resonant states in the shell model
Page 21: Resonant states in the shell model
Page 22: Resonant states in the shell model

*J-matrix:Let us try to extract resonance information

from Eλ behavior only

Page 23: Resonant states in the shell model

Eλ should increase with ħΩ

Within narrow resonance Eλ is nearly ħΩ-independent

The slope of Eλ(ħΩ) depends however on Nmax, l, Eλ value

Page 24: Resonant states in the shell model
Page 25: Resonant states in the shell model

*Breit-Wigner:

*Simple approximation: φ=0

Derivatives calculated through

Page 26: Resonant states in the shell model

*Breit-Wigner:

*Simple approximation: φ=0

Derivatives calculated through

Do not expect to get a reasonable result for Er or Γ if Γ/2Δ is small!

If |Γ/2Δ| is large, we get good results for Er, Γ and φ.

Page 27: Resonant states in the shell model
Page 28: Resonant states in the shell model
Page 29: Resonant states in the shell model
Page 30: Resonant states in the shell model
Page 31: Resonant states in the shell model

*What can we do if we obtain Eλ in a non-resonant region above the resonance?*We can extrapolate energies to larger

(finite) Nmax value when Eλ is in the resonant region.*Expected dependence is

Page 32: Resonant states in the shell model

This works. However this extrapolation seems to be unstable and inconvenient

Page 33: Resonant states in the shell model

More convenient is an exponential extrapolation.

Page 34: Resonant states in the shell model

*We get stable Er and Γ; Γ is too small as compared with experiment.

Page 35: Resonant states in the shell model

*I discussed general features of continuum states obtained in many-body calculations with oscillator basis.*The best way to compare the calculated results with

experiment is to use “experimental” phase shifts and get Eλ consistent with scattering data using simple inverse scattering technique.*Studying ħΩ dependence of Eλ obtained in NCSM, one

can get resonance energy and width. However, usually an extrapolation to a reasonable Nmax value is required.

Page 36: Resonant states in the shell model