Nuclear Structure Studies with the<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msup><mml:mrow /><mml:mrow><mml:mn>7</mml:mn></mml:mrow></mml:msup></mml:mrow><mml:mi>Li</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="italic">e</mml:mi><mml:mo>,</mml:mo><mml:mi /><mml:mrow><mml:msup><mml:mrow><mml:mi mathvariant="italic">e</mml:mi></mml:mrow><mml:mrow><mml:mo>′</mml:mo></mml:mrow></mml:msup></mml:mrow><mml:mi mathvariant="italic">p</mml:mi><mml:mo>)</mml:mo></mml:ma

Lapikás, L.; Wesseling, J.; Wiringa, R. B.

doi:10.1103/physrevlett.82.4404

Cited by 64 publications

(115 citation statements)

References 38 publications

Supporting

Mentioning

106

Contrasting

Order By: Relevance

“…In particular, variational Monte Carlo and Green's function Monte Carlo results using realistic free NN interactions and phenomenological but theoretically motivated NNN interactions have been published up to A = 8 [31]. Very impressive agreement with experiment has been obtained for 6 Li(e, e ′ ) 6 Li form factors [32] and for 7 Li(e, e ′ p) 6 He momentum distributions and spectroscopic factors [33]. The last result emphasises the essential quasi-particle nature of the shell model and the role played by (short-range) correlations [34,35].…”

Section: Structure Calculationsmentioning

confidence: 56%

Structure of unstable light nuclei

Millener

2001

Nuclear Physics A

View full text Add to dashboard Cite

The structure of light nuclei out to the drip lines and beyond up to Z ∼ 8 is interpreted in terms of the shell model. Special emphasis is given to the underlying supermultiplet symmetry of the p-shell nuclei which form cores for neutrons and protons added in sd-shell orbits. Detailed results are given on the wave functions, widths, and Coulomb energy shifts for a wide range of non-normal parity states in the p-shell.

show abstract

Section: Structure Calculationsmentioning

confidence: 56%

Structure of unstable light nuclei

Millener

2001

Nuclear Physics A

View full text Add to dashboard Cite

show abstract

“…2 '0' (24) since the propagator exp[-(H -Eo)~] commutes with the Hamiltonian. Thus (lJ(~))~iXed approaches EO in the limit r + 00, and the expectation value obeys the variational principle for all r. Direct GFMC calculations with the full interaction (in particular spindependent terms which involve the square of the momentum operator) have very large statistical errors.…”

Section: (@Tie-(h-eo)'/2 He-(h-e0)'/21vt) (V~le-(h-eo)'/2 E-~h-e0)"/2mentioning

confidence: 99%

Quantum Monte Carlo calculations for light nuclei

Wiringa

1998

Nuclear Physics A

View full text Add to dashboard Cite

Quantum Monte Carlo calculations of ground and low-lying xclted states for nuclei with A < 8 are made using a realistic Hamiltonian that fits NN scattering data. Results for more than 40 different (J=, T) states, plus isobaric analogs, are obtained and the known excitation spectra are reproduced reasonably well. Various density and momentum distributions and electromagnetic form factors and moments have also been computed. These are the first microscopic calculations that directly produce nuclear shell structure from realistic NN interactions.

show abstract

“…The routines used to compute the integral relations were written as modified versions of existing spectroscopic-overlap routines [60][61][62][63]. The integral-relation routines were used previously to compute bound-state ANCs [33], and only very minor modification (replacing regular Whittaker functions with regular scattering functions) was necessary for width calculations.…”

Section: B Overlap and Integral-relation Calculationsmentioning

confidence: 99%

Ab initiocalculations of nuclear widths via an integral relation

Nollett

2012

Phys. Rev. C

View full text Add to dashboard Cite

I describe the computation of energy widths of nuclear states using an integral over the interaction region of ab initio variational Monte Carlo wave functions, and I present calculated widths for many states. I begin by presenting relations that connect certain short-range integrals to widths. I then present predicted widths for 5 ≤ A ≤ 9 nuclei, and I compare them against measured widths. They match the data more closely and with less ambiguity than estimates based on spectroscopic factors. I consider the consequences of my results for identification of observed states in 8 B, 9 He, and 9 Li. I also examine failures of the method and conclude that they generally involve broad states and variational wave functions that are not strongly peaked in the interaction region. After examining bound-state overlap functions computed from a similar integral relation, I conclude that overlap calculations can diagnose cases in which computed widths should not be trusted.

show abstract

Nuclear Structure Studies with the7Li(e,e′p)

Cited by 64 publications

References 38 publications

Structure of unstable light nuclei

Structure of unstable light nuclei

Quantum Monte Carlo calculations for light nuclei

Ab initiocalculations of nuclear widths via an integral relation

Contact Info

Product

Resources

About