New insights into the limit of the magnetic monopole flux and the heating source in white dwarfs

[1]
L. Mestel, MNRAS. 112, 583 (1952)
[2]
R. M. Avakian, CoMBAO. 44, 115 (1972)
[3]
L. Bildsten and D. M. Hall, Astrophys. J. 549, 219 (2001)
[4]
C. J. Deloye and L. Bildsten, Astrophys. J. 580, 1077 (2002)
[5]
E. García-Berro, L. G. Althaus, A. H. Córsico et al., Asstrophys. J. 677, 473 (2008)
[6]
R. V. Lobato, M. Malheiro, and J. G. Coelho, Mgm. Conf. 4313, 4318 (2018)
[7]
S. H. Cheng, J. D. Cummings, and B. Ménard, Asstrophys. J. 886, 100 (2019)
[8]
M. E. Caplan, C. J. Horowitz, and A. Cumming, Astrophys. J. 902(2), 44C (2020)
[9]
C. Callan et al., Nucl. Phys. 212, 391 (1983)
[10]
V. A. Rubakov, JETP Lett. 33, 644 (1981)
[11]
M. Detrixhe, D. Besson, P. W. Gorham et al., Phys. Lett. D 83, 023513 (2011)
[12]
M. Frank, A. Antoshkin, C. Dukes et al., ICRC 36, 888 (2019)
[13]
T. Fujii and A. C. Pierre, ICRC 34, 319 (2015)
[14]
B. Kain, Phys. Rev. D 100, 063003 (2019)
[15]
A. Rajantie, Phil. Trans. R. Soc. A. 370, 5705 (2012)
[16]
N. E. Mavromatos and V. A. Mitsou, IJMPA 35, 2030012 (2020)
[17]
J. J. Liu, MNRAS. 433, 1108 (2013)
[18]
J. J. Liu, MNRAS. 438, 930 (2014)
[19]
J. J. Liu and W. M. Gu, Astrophys. J. Suppl. 224, 29 (2016)
[20]
J. J. Liu, D. M. Liu et al., Chin. Phys. C 41(12), 125102 (2017)
[21]
J. J. Liu and D. M. Liu, EPJC. 78, 84 (2018a)
[22]
J. J. Liu and D. M. Liu, RAA. 18(1), 8 (2018)
[23]
J. J. Liu and D. M. Liu, Astrophys. Space Sci. 363(5), 115 (2018)
[24]
J. J. Liu and D. M. Liu, New Astron. 69, 69 (2019a)
[25]
J. J. Liu, D. M. Liu, and L. H. Hao, ChPhC 43, 064107 (2019b)
[26]
J. J. Liu and D. M. Liu, Astron. Nachr. 341, 291 (2020)
[27]
Q. H., Peng, J. J. Liu, and C. K. Chou, MPLA 35, 2050030 (2020)
[28]
Q. H. Peng, J. J. Liu, and Z. Q. Ma, New Astron. 57, 59 (2017)
[29]
W. Bernreuther and N. S. Craigie, Phys. Rev. Lett. 55, 2555 (1985)
[30]
Q. H. Peng, Z. Y. Lie, and D. Y. Wang, Sci. Sin. Phys. Mech. As. 28, 970 (1985)
[31]
E. Kolb and M. S. Turner., Astrophys. J. 286, 702 (1984)
[32]
K. Freese, Asstrophys. J. 286, 216 (1984)
[33]
Z. Q. Ma and J. F. Tang, Phys. Lett. B 153, 59 (1983)
[34]
T. Kallinger, W. W. Weiss, C. Barban et al., A&A 509, A77 (2010)
[35]
D. Stello, and H. Bruntt, H. Preston et al., Astrophys. J. 674, L53 (2008)
[36]
D. Huber, T. R. Bedding, D. Stello et al., Astrophys. J. 743, 143 (2011)
[37]
S. Sharma, D. Stello, and J. Bland-Hawthorn et al., Astrophys. J. 822, 15 (2016)
[38]
T. M. Brown, D. W. Latham, M. E. Everett et al., Astron. J. 142, 112 (2011)
[39]
E. Parker, Asstrophys. J. 160, 383 (1970)
[40]
K. Freese and E. Krasteva, Phys. Rev. D 59, 063007 (1999)
[41]
S. K. Grunblatt, J. C. Zinn, A. M. Price-Whelan et al., Astrophys. J. 916, 88 (2021)
[42]
V. Silva Aguirre, G. R. Davies, and S. Basu, MNRAS 452, 2127 (2015)
[43]
T. D. Morton, Isochrones: Stellar Model Grid Package, v2.0, (Astrophysics Source Code Library, ascl: 1503.010, 2015)
[44]
D. Huber, J. Zinn, M. Bojsen-Hansen et al., Astrophys. J. 844, 102 (2017)
[45]
L. da Silva, L. Girardi, L. Pasquini et al., A&A 458, 609 (2006)
[46]
T. S. Rodrigues, D. Bossini, and A. Miglio, Mon. Not. R. Astron. Soc. 467, 1433 (2017)
[47]
E. P. Bellinger, Mon. Not. R. Astron. Soc. 492, L50 (2020)
[48]
K. Belkacem, M. J. Goupil, M. A. Dupret et al., A&A 530, A142 (2011)
[49]
H. Kjeldsen and T. R. Bedding, A&A 293, 87 (1995)
[50]
D. Huber, D. Stello, T. R. Bedding et al., Comm. Asteroseismology 160, 74 (2009)
[51]
K. Freese, M. S.Turner, and D. N. Schramm, Phys. Rev. Lett. 51, 1625 (1983)
[52]
M. Schwarzschild, Structure and Evolution of the Star., (Princeton: Princeton university Press, 1958)
[53]
R. Bjork, Stephan, and B. Chaboyer, Astrophys. J. 641, 1102 (2006)
[54]
D. A. Dicus, D. N. Page, and V. L. Teplitz, Phys. Rev. D 26, 1306 (1982)
[55]
L. G. Althaus, A. H. Córsico, J. Isern et al., Astron. Astrophys. Rev. 18, 471 (2010)
[56]
N. Itoh, H. Hayashi, A. Nishikawa et al., Astrophys. J. Suppl. 102, 411 (1996)
[57]
M. Izawa, Prog. Theor. 75, 556 (1986)