2023
DOI: 10.1088/1674-1137/acdc8b
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New insights into the limit of the magnetic monopole flux and the heating source in white dwarfs*

Abstract: Based on the magnetic monopoles(MMs) catalytic nuclear decay (RC effect), we propose five new models to discuss the limit of the MMs' flux and the cooling energy resources of the white dwarfs (WDs) by some observations from 13 RGB stars. We find that the number of MMs captured can reach the maximum value of $9.1223\times10^{24}$ when $m=10^{17}, n_B=5.99\times10^{31}, \phi=7.59\times10^{-26}$. The good agreement of our luminosities calculated for WDs with the observations shows that our model is rational due t… Show more

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Cited by 2 publications
(4 citation statements)
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“…Recently, we discussed the energy source problem for WDs. First, we discussed the numbers of MMs captured in space at the surface of stars, which is given by (Peng et al 1985;Peng & Liu 2023;Liu et al 2023aLiu et al , 2023bLiu & Liu 2023c, 2023d g m = 3hc/2e and m B , which are the magnetic charge of MMs and the baryon number mass, respectively. The MM mass is about m m ∼ 10 16 m p (Polyakov 1974), where m p is the mass of a proton.…”
Section: Our Recent Work On the Numbers Of Mms Captured And The Lumin...mentioning
confidence: 99%
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“…Recently, we discussed the energy source problem for WDs. First, we discussed the numbers of MMs captured in space at the surface of stars, which is given by (Peng et al 1985;Peng & Liu 2023;Liu et al 2023aLiu et al , 2023bLiu & Liu 2023c, 2023d g m = 3hc/2e and m B , which are the magnetic charge of MMs and the baryon number mass, respectively. The MM mass is about m m ∼ 10 16 m p (Polyakov 1974), where m p is the mass of a proton.…”
Section: Our Recent Work On the Numbers Of Mms Captured And The Lumin...mentioning
confidence: 99%
“…where R g = 2.96 × 10 5 M * is the Schwarzschild radius, and M 12 = M * /10 12 , M * = M/M e and R * = R/R e (Peng et al 1985;Peng & Liu 2023;Liu et al 2023aLiu et al , 2023bLiu & Liu 2023c, 2023d. As a general rule, the values of reaction cross-section are distributed between 10 −26 and 10 −24 cm 2 .…”
Section: Our Recent Work On the Numbers Of Mms Captured And The Lumin...mentioning
confidence: 99%
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