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<h2 id="references">References</h2>

<ol>
<li id="fn:1">Jacob Bekenstein & M. Milgrom (1984). "Does the missing mass problem signal the breakdown of Newtonian gravity?". Astrophys. J. 286: 7–14. Bibcode:1984ApJ...286....7B. doi:10.1086/162570. <a href="/wiki/Bibcode_(identifier)" target="_blank">/wiki/Bibcode_(identifier)</a> <a href="#fnref:1" class="footnote-back-ref">↩</a></li>
<li id="fn:2">Milgrom, M (1986). "Solutions for the modified Newtonian dynamics field equation". Astrophys. J. 302: 617–625. Bibcode:1986ApJ...302..617M. doi:10.1086/164021. <a href="https://doi.org/10.1086%2F164021" target="_blank">https://doi.org/10.1086%2F164021</a> <a href="#fnref:2" class="footnote-back-ref">↩</a></li>
<li id="fn:3">Felten, J. E. (1984). "Milgrom's revision of Newton's laws - Dynamical and cosmological consequences". The Astrophysical Journal. 286: 3. doi:10.1086/162569. ISSN 0004-637X. <a href="https://doi.org/10.1086%2F162569" target="_blank">https://doi.org/10.1086%2F162569</a> <a href="#fnref:3" class="footnote-back-ref">↩</a></li>
<li id="fn:4">Sanders, Robert H.; McGaugh, Stacy S. (2002). "Modified Newtonian dynamics as an alternative to dark matter". Annual Review of Astronomy and Astrophysics. 40 (1): 263–317. arXiv:astro-ph/0204521. Bibcode:2002ARA&A..40..263S. doi:10.1146/annurev.astro.40.060401.093923. <a href="/wiki/ArXiv_(identifier)" target="_blank">/wiki/ArXiv_(identifier)</a> <a href="#fnref:4" class="footnote-back-ref">↩</a></li>
<li id="fn:5">Chae, Kyu-Hyun (2023-08-01). "Breakdown of the Newton–Einstein Standard Gravity at Low Acceleration in Internal Dynamics of Wide Binary Stars". The Astrophysical Journal. 952 (2): 128. arXiv:2305.04613. doi:10.3847/1538-4357/ace101. ISSN 0004-637X. <a href="https://doi.org/10.3847%2F1538-4357%2Face101" target="_blank">https://doi.org/10.3847%2F1538-4357%2Face101</a> <a href="#fnref:5" class="footnote-back-ref">↩</a></li>
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