Relativistic many-body calculation of energies, oscillator strengths, transition rates, lifetimes, polarizabilities, and quadrupole moment of a Fr-like Thiv ion

@article{Safronova2013RelativisticMC,
  title={Relativistic many-body calculation of energies, oscillator strengths, transition rates, lifetimes, polarizabilities, and quadrupole moment of a Fr-like Thiv ion},
  author={Marianna S. Safronova and U. I. Safronova},
  journal={Physical Review A},
  year={2013},
  volume={87}
}
Atomic properties of the 24 low-lying ns, np, nd, nf, and ng states in Th IV ion are calculated using the high-precision relativistic all-order method where all single, double, and partial triple excitations of the Dirac-Fock wave functions are included to all orders of perturbation theory. Recommended values are provided for a large number of electric-dipole matrix elements, oscillator strengths, transition rates, and lifetimes. Scalar polarizabilities of the ground and six excited states… 

Tables from this paper

Laser-induced electronic bridge for characterization of the 229mTh ⃗ 229gTh nuclear transition with a tunable optical laser

An alternative method to determine the excitation energy of the 229mTh isomer via the laser-induced electronic bridge is investigated theoretically. In the presence of an optical or ultra-violet

Populating 229mTh via two-photon electronic bridge mechanism

The isomer $$^{229{\text{m}}}$$ Th is the most promising candidate for clocks based on the nuclear transition because it has the lowest excitation energy of only $$8.10\pm 0.17$$ eV. Various

Heavy metals in intermediate He-rich hot subdwarfs: the chemical composition of HZ 44 and HD 127493

Context. Hot subluminous stars can be spectroscopically classified as subdwarf B (sdB) and O (sdO) stars. While the latter are predominantly hydrogen deficient, the former are mostly helium

References

SHOWING 1-10 OF 26 REFERENCES

Phys

  • Rev. A 83, 062501
  • 2011

in International Tables of Selected Constants

  • Vol. 20
  • 1992

Phys

  • Rev. A 83, 052508
  • 2011

B 37

  • 4193
  • 2004

Phys

  • Rev. A 76, 042504
  • 2007

Phys

  • Rev. A 85, 022504
  • 2012

Phys

  • Rev. A 74, 042511
  • 2006

Phys

  • Rev. Lett. 102, 233004
  • 2009

Phys

  • Rev. Lett. 102, 210801
  • 2009

11 Nature 443

  • 316
  • 2006