Neutron Skin Thickness of 48Ca, 132Sn, and 208Pb with KIDS Density Functional
@article{Hyun2022NeutronST, title={Neutron Skin Thickness of 48Ca, 132Sn, and 208Pb with KIDS Density Functional}, author={Chang Ho Hyun}, journal={New Physics: Sae Mulli}, year={2022} }
Neutron skin thickness (Rnp) of the atomic nuclei 48Ca, 132Sn and 208Pb are considered in the KIDS (Korea:IBS-Daegu-Sungkyunkwan) density functional formalism. Model parameters most relevant to Rnp are constrained from standard nuclear data and neutron star properties determined from modern observations. Mean values of Rnp are obtained as 0.161, 0.220 and 0.160 fm for 48Ca, 132Sn and 208Pb, respectively, and the corresponding standard deviations are 0.011, 0.020 and 0.021 fm. Correlations…
References
SHOWING 1-5 OF 5 REFERENCES
ASTRO
- Physics, Computer Science
- 2021
The findings reveal that, despite no prior training and noisy sensory measurements, ASTRO drones are able to learn the propagation environment in the scale of seconds and localize a target with a mean accuracy of 8 m.
Phys
- Rev. C 85 401302(R)
- 2012
Phys
- Rev. C 99, 064319
- 2019
Phys
- Rev. C 102, 044316
- 2020
Phys
- Rev. C 104, 044613
- 2021