Skip to main content
Log in

Influence of super-strong magnetic fields on beta decay of nuclide \({}^{59}\mbox{Co}\) in magnetar surface

  • Original Article
  • Published:
Astrophysics and Space Science Aims and scope Submit manuscript

Abstract

Based on the relativistic theory in super-strong magnetic fields (SMFs), we investigate the influence of SMFs on beta decay and the change rates of electron fraction (CREF) of nuclei \({}^{59}\mbox{Co}\) in magnetars. Firstly, we find the magnetic fields have a slight influence on the beta decay rates for a given temperature when \(\rho_{7}<1\). However, the beta decay rates decrease greatly by more than five orders of magnitude when \(\rho_{7}>1\). Secondly, our results show that this effect of SMFs can increase beta reaction rates by two orders magnitude when \(10 \leq B_{12} \leq 10^{4}~\mbox{G}\). For instance, the beta decay rate for \({}^{56}\mbox{Co}\) increases from \(4.797\times10^{-3}\) to \(3.284\times10^{-1}\) at \(\rho_{7}=4.32\). Finally, we find that the CREF increases about by two orders of magnitude in SMFs and the enhancement factor will be high as 95.95 for \(\rho_{7}=4.32\).

This is a preview of subscription content, log in via an institution to check access.

Access this article

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Fig. 1
Fig. 2
Fig. 3
Fig. 4

Similar content being viewed by others

References

Download references

Acknowledgements

This work was supported in part by the National Natural Science Foundation of China under grants 11565020, and the Natural Science Foundation of Hainan province under grant 114012.

Author information

Authors and Affiliations

Authors

Corresponding author

Correspondence to Jing-Jing Liu.

Rights and permissions

Reprints and permissions

About this article

Check for updates. Verify currency and authenticity via CrossMark

Cite this article

Liu, JJ., Liu, DM. Influence of super-strong magnetic fields on beta decay of nuclide \({}^{59}\mbox{Co}\) in magnetar surface. Astrophys Space Sci 361, 246 (2016). https://doi.org/10.1007/s10509-016-2830-0

Download citation

  • Received:

  • Accepted:

  • Published:

  • DOI: https://doi.org/10.1007/s10509-016-2830-0

Keywords

Navigation