Abstract
The effect of interaction between hyperons on the moment of inertia of proto neutron star (PNS) PSR J0740+6620 is examined with relativistic mean field theory considering the octet of baryons. The nucleon coupling constant GM1 is used and the temperature of the PNS is chosen as \(T=20\) MeV. Under the constraint of the mass \(M=2.08 M_{\odot }\), considering the interaction between hyperons, the radius of the PNS PSR J0740+6620 is reduced by 0.08% from \(R=14.518\) km to \(R=14.507\) km and the moment of inertia of the PNS PSR J0740+6620 is reduced by about 0.49% from \(I=2.460 \times 10^{45}\) g cm\(^{2}\) to \(I=2.448 \times 10^{45}\) g cm\(^{2}\), respectively. The moment of inertia of the PNS has a peak with the change of central energy density \(\varepsilon _{c}\), mass M or radius R. Considering the interaction between hyperons, the value of the moment of inertia I of the PNS corresponding to this peak will decrease.
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Acknowledgements
The authors are thankful to the anonymous referee for some valuable suggestions. This work was supported by the Natural Science Foundation of China (Grant No. 11447003).
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Zhao, XF. Effect of the interaction between hyperons on the moment of inertia of proto neutron star PSR J0740+6620. Pramana - J Phys 97, 209 (2023). https://doi.org/10.1007/s12043-023-02694-y
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DOI: https://doi.org/10.1007/s12043-023-02694-y