Magnetic structure of<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mmultiscripts><mml:mrow><mml:mi mathvariant="normal">O</mml:mi></mml:mrow><mml:mprescripts /><mml:mrow /><mml:mrow><mml:mn>17</mml:mn></mml:mrow><mml:mrow /><mml:mrow /></mml:mmultiscripts></mml:mrow></mml:math>at high momentum

Kalantar‐Nayestanaki, N.; Baghaei, H.; Bertozzi, W.; Dixit, S.; Finn, J. M.; Hyde-Wright, C. E.; Kowalski, S.; Lourie, R.; Sargent, C. P.; Ulmer, P. E.; Weinstein, Lawrence; Hynes, M. V.; Berman, B. L.; Kelly, J. J.

doi:10.1103/physrevlett.60.1707

Cited by 29 publications

(15 citation statements)

References 23 publications

Supporting

Mentioning

Contrasting

Order By: Relevance

“…The spectroscopic factors of M5 from NL-SH and TM2 are 0.92 and 0.94, respectively. These values are similar to the value 0.96±0.11 deduced from elastic electron scattering form factors in the high-q region [40]. As for 41 Ca, the rms radius of the 1f 7/2 orbital obtained from sub-Coulomb transfer reactions are 4.00 ± 0.06 fm [44] and 3.89 ± 0.12 fm [45].…”

Section: Numerical Resultssupporting

confidence: 86%

“…[43] is 3.35 ± 0.03 fm [41], which is very close to the value 3.36 fm of Ref. [40]. The spectroscopic factors of M5 from NL-SH and TM2 are 0.92 and 0.94, respectively.…”

Section: Numerical Resultssupporting

confidence: 85%

“…[46]. The agreement of the [40,43] and [46,47], respectively. rms radii and spectroscopic factors in the RMF theory with the experimental data and other theoretical ones implies the validity of the RMF theory in reproducing the magnetic form factor.…”

Section: Numerical Resultsmentioning

confidence: 82%

“…These results agree with the values of Refs. [40][41][42]. The valence rms radius of 17 O deduced from the best fit of the overall spectroscopic factors α , L s to the magnetic electron scattering data taken from Ref.…”

Section: Numerical Resultsmentioning

confidence: 99%

See 3 more Smart Citations

Elastic magnetic form factors of exotic nuclei

2007

View full text Add to dashboard Cite

How to identify the orbital of the valence nucleon(s) of exotic nuclei is an important problem. The elastic magnetic electron scattering is an excellent probe to determine the valence structure of odd-A nuclei. The relativistic mean-field theory has been successfully applied to systematic studies of the elastic charge electron scattering from even-even exotic nuclei. The extension of this method to investigate the elastic magnetic electron scattering from odd-A exotic nuclei is a natural generalization. The experimental form factors of 17 O and 41 Ca are reproduced very well with the help of the spectroscopic factors which are introduced into the relativistic treatment of the magnetic electron scattering for the first time. The emphases are put on the magnetic form factors of 15,17,19 C, 23 O, 17 F, and 49,59 Ca calculated in the relativistic impulse approximation. Great differences have been found in the form factors of the same nucleus with different configurations. Therefore, the elastic magnetic electron scattering can be used to determine the orbital of the last nucleon of odd-A exotic nuclei. Our results can provide references for the electron scattering from exotic nuclei in the near future.

show abstract

Section: Numerical Resultssupporting

confidence: 86%

“…[43] is 3.35 ± 0.03 fm [41], which is very close to the value 3.36 fm of Ref. [40]. The spectroscopic factors of M5 from NL-SH and TM2 are 0.92 and 0.94, respectively.…”

Section: Numerical Resultssupporting

confidence: 85%

Section: Numerical Resultsmentioning

confidence: 82%

Section: Numerical Resultsmentioning

confidence: 99%

See 2 more Smart Citations

Elastic magnetic form factors of exotic nuclei

2007

View full text Add to dashboard Cite

show abstract

“…In Table II we list our choice of the data along with their sources [34,35,36,37,38,39,40,41,42]. It must be noted that in addition to the data on the binding energy, charge radii and single particle energies, the values of the Skyrme parameters are further constrained by including in the fit the experimental data for the radii of valence neutron orbits, breathing mode energies together with a realistic EOS for the pure neutron matter upto the densities (∼ 0.8 fm r v (ν1d 5/2 ) = 3.36 fm and r v (ν1f 7/2 ) = 3.99 fm, [37,38] respectively. The theoretical error taken for the rms radii for the valence neutron orbits is 0.06 fm.…”

Section: B Data Used In the Fitting Proceduresmentioning

confidence: 99%

Exploring the extended density-dependent Skyrme effective forces for normal and isospin-rich nuclei to neutron stars

2006

View full text Add to dashboard Cite

We parameterize the recently proposed generalized Skyrme effective force (GSEF) containing extended density dependence. The parameters of the GSEF are determined by the fit to several properties of the normal and isospin-rich nuclei. We also include in our fit a realistic equation of state for the pure neutron matter up to high densities so that the resulting Skyrme parameters can be suitably used to model the neutron star with the "canonical" mass (∼ 1.4M ⊙ ). For the appropriate comparison we generate a parameter set for the standard Skyrme effective force (SSEF) using exactly the same set of the data as employed to determine the parameters of the GSEF. We find that the GSEF yields larger values for the neutron skin thickness which are closer to the recent predictions based on the isospin diffusion data. The Skyrme parameters so obtained are employed to compute the strength function for the isoscalar giant monopole, dipole and quadrupole resonances. It is found that in the case of GSEF, due to the the larger value of the nucleon effective mass the values of centroid energies for the isoscalar giant resonances are in better agreement with the corresponding experimental data in comparison to those obtained using the SSEF. We also present results for some of the key properties associated with the neutron star of "canonical" mass and for the one with the maximum mass. 21.65+f,24.30.Cz,21.60jz,26.60.+c

show abstract

Electron Scattering Off Stable and Unstable Nuclei

Suda

2022

Handbook of Nuclear Physics

View full text Add to dashboard Cite

Magnetic structure ofO17at high momentum

Cited by 29 publications

References 23 publications

Elastic magnetic form factors of exotic nuclei

Elastic magnetic form factors of exotic nuclei

Exploring the extended density-dependent Skyrme effective forces for normal and isospin-rich nuclei to neutron stars

Electron Scattering Off Stable and Unstable Nuclei

Contact Info

Product

Resources

About