Abstract
The internal solar structure predicted by the standard solar model disagrees with the helioseismic observations even by utilizing the most updated physical inputs, such as the opacity and element abundances. By increasing the Rosseland mean, the decade-old open problem of the missing opacity can be resolved. Herein, we propose that the continuum electrons in the radiative processes lose phases and coherence as matter waves, giving rise to a phenomenon of transient spatial localization. It not only enhances the continuum opacity but also increases the line widths of the bound-bound transitions. We demonstrate our theoretical formulation by investigating the opacity of solar mixtures in the interior. The Rosseland mean demonstrates an increase of 10%–26% in the range of 0.3R⊙–0.75R⊙. The results are compared with the recent experimental data and the existing theoretical models. Our findings provide novel clues to the open problem of the missing opacity in the solar interior and new insight on the radiative opacity in the hot dense-plasma regime.
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References
F. J. Rogers, and C. A. Iglesias, Science 263, 50 (1994).
S. Basu, and H. M. Antia, Phys. Rep. 457, 217 (2008), arXiv: 0711.4590.
A. M. Serenelli, S. Basu, J. W. Ferguson, and M. Asplund, Astrophys. J. 705, L123 (2009), arXiv: 0909.2668.
J. Christensen-Dalsgaard, Living Rev. Sol. Phys. 18, 2 (2021), arXiv: 2007.06488.
M. Asplund, N. Grevesse, A. J. Sauval, and P. Scott, Annu. Rev. Astron. Astrophys. 47, 481 (2009), arXiv: 0909.0948.
M. Asplund, A. M. Amarsi, and N. Grevesse, arXiv: 2105.01661.
J. N. Bahcall, A. M. Serenelli, and M. Pinsonneault, Astrophys. J. 614, 464 (2004), arXiv: astro-ph/0403604.
H. Saio, Mon. Not. R. Astron. Soc. 258, 491 (1992).
J. N. Bahcall, S. Basu, M. Pinsonneault, and A. M. Serenelli, Astrophys. J. 618, 1049 (2005), arXiv: astro-ph/0407060.
J. Christensen-Dalsgaard, M. P. Di Mauro, G. Houdek, and F. Pijpers, Astron. Astrophys. 494, 205 (2009).
J. E. Bailey, T. Nagayama, G. P. Loisel, G. A. Rochau, C. Blancard, J. Colgan, P. Cosse, G. Faussurier, C. J. Fontes, F. Gilleron, I. Golovkin, S. B. Hansen, C. A. Iglesias, D. P. Kilcrease, J. J. MacFarlane, R. C. Mancini, S. N. Nahar, C. Orban, J. C. Pain, A. K. Pradhan, M. Sherrill, and B. G. Wilson, Nature 517, 56 (2015).
T. Nagayama, J. E. Bailey, G. P. Loisel, G. S. Dunham, G. A. Rochau, C. Blancard, J. Colgan, P. Cosse, G. Faussurier, C. J. Fontes, F. Gilleron, S. B. Hansen, C. A. Iglesias, I. E. Golovkin, D. P. Kilcrease, J. J. MacFarlane, R. C. Mancini, R. M. More, C. Orban, J. C. Pain, M. E. Sherrill, and B. G. Wilson, Phys. Rev. Lett. 122, 235001 (2019).
G. A. Rochau, J. E. Bailey, R. E. Falcon, G. P. Loisel, T. Nagayama, R. C. Mancini, I. Hall, D. E. Winget, M. H. Montgomery, and D. A. Liedahl, Phys. Plasmas 21, 056308 (2014).
C. A. Iglesias, and F. J. Rogers, Astrophys. J. 371, 408 (1991).
M. J. Seaton, Y. Yan, D. Mihalas, and A. K. Pradhan, Mon. Not. R. Astron. Soc. 266, 805 (1994).
S. B. Hansen, J. Bauche, C. Bauche-Arnoult, and M. F. Gu, High Energy Density Phys. 3, 109 (2007).
Q. Porcherot, J. C. Pain, F. Gilleron, and T. Blenski, High Energy Density Phys. 7, 234 (2011), arXiv: 1105.2494.
C. Blancard, P. Cosse, and G. Faussurier, Astrophys. J. 745, 10 (2012).
J. Colgan, D. P. Kilcrease, N. H. Magee Jr., G. S. J. Armstrong, J. Abdallah Jr., M. E. Sherrill, C. J. Fontes, H. L. Zhang, and P. Hakel, High Energy Density Phys. 9, 369 (2013).
J. Zeng, and J. Yuan, Phys. Rev. E 74, 025401 (2006).
C. A. Iglesias, High Energy Density Phys. 15, 4 (2015).
D. J. Hoarty, J. Morton, M. Jeffery, L. K. Pattison, A. Wardlow, S. P. D. Mangles, S. J. Rose, C. Iglesias, K. Opachich, R. F. Heeter, and T. S. Perry, High Energy Density Phys. 32, 70 (2019).
J. C. Pain, and F. Gilleron, High Energy Density Phys. 15, 30 (2015), arXiv: 1503.08939.
M. Krief, A. Feigel, and D. Gazit, Astrophys. J. 824, 98 (2016), arXiv: 1603.01153.
C. J. Fontes, C. L. Fryer, A. L. Hungerford, P. Hakel, J. Colgan, D. P. Kilcrease, and M. E. Sherrill, High Energy Density Phys. 16, 53 (2015).
R. M. More, S. B. Hansen, and T. Nagayama, High Energy Density Phys. 24, 44 (2017).
J. C. Pain, High Energy Density Phys. 26, 23 (2018), arXiv: 1711.11295.
M. Krief, Y. Kurzweil, A. Feigel, and D. Gazit, Astrophys. J. 856, 135 (2018).
J. Colgan, D. P. Kilcrease, N. H. Magee, M. E. Sherrill, J. Abdallah Jr., P. Hakel, C. J. Fontes, J. A. Guzik, and K. A. Mussack, Astrophys. J. 817, 116 (2016), arXiv: 1601.01005.
C. A. Iglesias, and S. B. Hansen, Astrophys. J. 835, 284 (2017).
P. Liu, C. Gao, Y. Hou, J. Zeng, and J. Yuan, Commun. Phys. 1, 95 (2018).
S. X. Hu, B. Militzer, V. N. Goncharov, and S. Skupsky, Phys. Rev. Lett. 104, 235003 (2010).
S. H. Glenzer, and R. Redmer, Rev. Mod. Phys. 81, 1625 (2009).
R. F. Smith, D. E. Fratanduono, D. G. Braun, T. S. Duffy, J. K. Wicks, P. M. Celliers, S. J. Ali, A. Fernandez-Pañella, R. G. Kraus, D. C. Swift, G. W. Collins, and J. H. Eggert, Nat. Astron. 2, 452 (2018).
C. Gao, J. Zeng, Y. Li, F. Jin, and J. Yuan, High Energy Density Phys. 9, 583 (2013).
R. K. Janev, S. Zhang, and J. Wang, Matter Radiat. Extrem. 1, 237 (2016).
B. F. Rozsnyai, Phys. Rev. A 5, 1137 (1972).
M. F. Gu, Can. J. Phys. 86, 675 (2008).
S. K. Son, R. Thiele, Z. Jurek, B. Ziaja, and R. Santra, Phys. Rev. X 4, 031004 (2014), arXiv: 1404.5484.
Y. Li, J. Wu, Y. Hou, and J. Yuan, J. Phys. B-At. Mol. Opt. Phys. 42, 235701 (2009).
J. Zeng, Y. Li, C. Gao, and J. Yuan, Astron. Astrophys. 634, A117 (2020).
J. Zeng, Y. Li, Y. Hou, C. Gao, and J. Yuan, Astron. Astrophys. 644, A92 (2020).
M. W. C. Dharma-wardana, and R. Taylor, J. Phys. C-Solid State Phys. 14, 629 (1981).
S. Ichimaru, H. Iyetomi, and S. Tanaka, Phys. Rep. 149, 91 (1987).
M. J. Seaton, J. Phys. B-At. Mol. Phys. 20, 6431 (1987).
Z. Zhao, J. Yuan, and Y. Sun, Chin. Phys. Lett. 16, 885 (1999).
J. Zeng, Y. Li, and J. Yuan, J. Quant. Spectr. Radiat. Transfer 272, 107777 (2021).
J. Zeng, Y. Li, and J. Yuan, Mon. Not. R. Astron. Soc. 504, 4785 (2021).
J. N. Bahcall, and R. K. Ulrich, Rev. Mod. Phys. 60, 297 (1988).
D. B. Guenther, P. Demarque, Y. C. Kim, and M. H. Pinsonneault, Astrophys. J. 387, 372 (1992).
J. Zeng, and J. Yuan, Phys. Rev. E 76, 026401 (2007).
M. S. Dimitrijević, and N. Konjević, Astron. Astrophys. 172, 345 (1987).
N. R. Badnell, M. A. Bautista, K. Butler, F. Delahaye, C. Mendoza, P. Palmeri, C. J. Zeippen, and M. J. Seaton, Mon. Not. R. Astron. Soc. 360, 458 (2005), arXiv: astro-ph/0410744.
C. A. Iglesias, and F. J. Rogers, Astrophys. J. 464, 943 (1996).
P. Giannozzi, O. Andreussi, T. Brumme, O. Bunau, M. Buongiorno Nardelli, M. Calandra, R. Car, C. Cavazzoni, D. Ceresoli, M. Cococcioni, N. Colonna, I. Carnimeo, A. Dal Corso, S. de Gironcoli, P. Delugas, R. A. DiStasio Jr, A. Ferretti, A. Floris, G. Fratesi, G. Fugallo, R. Gebauer, U. Gerstmann, F. Giustino, T. Gorni, J. Jia, M. Kawamura, H. Y. Ko, A. Kokalj, E. Küçükbenli, M. Lazzeri, M. Marsili, N. Marzari, F. Mauri, N. L. Nguyen, H. V. Nguyen, A. Otero-de-la-Roza, L. Paulatto, S. Poncé, D. Rocca, R. Sabatini, B. Santra, M. Schlipf, A. P. Seitsonen, A. Smogunov, I. Timrov, T. Thonhauser, P. Umari, N. Vast, X. Wu, and S. Baroni, J. Phys.-Condens. Matter 29, 465901 (2017), arXiv: 1709.10010.
Y. Hou, and J. Yuan, Phys. Rev. E 79, 016402 (2009).
J. P. Perdew, K. Burke, and M. Ernzerhof, Phys. Rev. Lett. 77, 3865 (1996).
J. J. Boland, S. E. Crane, and J. D. Baldeschwieler, J. Chem. Phys. 77, 142 (1982).
C. del Burgo, and C. Allende Prieto, Mon. Not. R. Astron. Soc. 479, 1953 (2018), arXiv: 2106.10752.
J. T. Bueno, and N. Shchukina, Astrophys. J. 694, 1364 (2009), arXiv: 0812.3494.
T. M. Brown, and J. Christensen-Dalsgaard, Astrophys. J. 500, L195 (1998), arXiv: astro-ph/9803131.
F. L. Villante, and B. Ricci, Astrophys. J. 714, 944 (2010), arXiv: 0912.4696.
J. Christensen-Dalsgaard, W. Däppen, S. V. Ajukov, E. R. Anderson, H. M. Antia, S. Basu, V. A. Baturin, G. Berthomieu, B. Chaboyer, S. M. Chitre, A. N. Cox, P. Demarque, J. Donatowicz, W. A. Dziembowski, M. Gabriel, D. O. Gough, D. B. Guenther, J. A. Guzik, J. W. Harvey, F. Hill, G. Houdek, C. A. Iglesias, A. G. Kosovichev, J. W. Leibacher, P. Morel, C. R. Proffitt, J. Provost, J. Reiter, E. J. Rhodes Jr., F. J. Rogers, I. W. Roxburgh, M. J. Thompson, and R. K. Ulrich, Science 272, 1286 (1996).
The Borexino Collaboration, Nature 587, 577 (2020), arXiv: 2006.15115.
Q. Ma, J. Dai, D. Kang, M. S. Murillo, Y. Hou, Z. Zhao, and J. Yuan, Phys. Rev. Lett. 122, 015001 (2019).
G. S. Bisnovatyi-Kogan, and M. V. Glushikhina, Plasma Phys. Rep. 44, 1114 (2018), arXiv: 1902.01156.
K. Fukushima, and Y. Hidaka, Phys. Rev. Lett. 120, 162301 (2018), arXiv: 1711.01472.
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This work was supported by the Science Challenge Project (Grant No. TZ2018005), the National Key R&D Program of China (Grant Nos. 2019YFA0307700, and 2017YFA0403202), and the National Natural Science Foundation of China (Grant Nos. 12174343, and 11774322).
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Zeng, J., Gao, C., Liu, P. et al. Electron localization enhanced photon absorption for the missing opacity in solar interior. Sci. China Phys. Mech. Astron. 65, 233011 (2022). https://doi.org/10.1007/s11433-021-1812-1
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DOI: https://doi.org/10.1007/s11433-021-1812-1