This list is by no means complete. If you would like to have your work listed here, please send an e-mail to LelliF@cardiff.ac.uk. The list indicatively follows the date of appearance on the arXiv.
"The mass discrepancy acceleration relation in a LCDM context"
Di Cintio A. & Lelli F. 2016, MNRAS, 456, 127 (ADS)
"A statistical investigation of the mass discrepancy-acceleration relation"
Desmond H. 2017, MNRAS, 464, 4160 (ADS)
"Universal MOND relation between the baryonic and 'dynamical' central surface densities of disk galaxies"
Milgrom M. 2016, PRL, 117, 141101 (ADS)
"MOND impact on and of the recently updated mass-discrepancy-acceleration relation"
Milgrom M. 2016, arXiv:1609.06642 (ADS)
"Four principles for quantum gravity"
Smolin, L. 2016, arXiv:1610.01968 (ADS)
"LCDM is consistent with SPARC acceleration law"
Keller B.W. & Wadsley J.W. 2017, ApJL, 835, 17 (ADS)
"Acceleration in Modified Gravity (MOG) and the Mass-Discrepancy Baryonic Relation"
Moffat J.W. 2016, arXiv:1610.06909 (ADS)
"The LCDM simulations of Keller & Wadsley do not account for the MOND mass-discrepancy-acceleration relation"
Milgrom, M. 2016, arXiv:1610.07538 (ADS)
"Radial Acceleration Relation from screening of fifth forces"
Burrage C., Copeland E.J. & Millington P. 2016, PRD, 95, 064050 (ADS)
"Mass-Discrepancy Acceleration Relation: A Natural Outcome of Galaxy Formation in Cold Dark Matter Halos"
Ludlow, A.D. et al. 2017, PRL, 118, 1103 (ADS)
"Radial Acceleration Relation and Dissipative Dark Matter"
Chashchina, O. et al. 2016, PRD, 95, 023009 (ADS)
"The origin of the mass discrepancy-acceleration relation in LCDM"
Navarro, J.F. et al. 2017, MNRAS, 471, 1841 (ADS)
"Dark Matter Strikes Back"
Salucci, P. 2016, arXiv:1612.08857 (ADS)
"Rotation Curves of High-Resolution LSB and SPARC Galaxies in Wave (Fuzzy) and Multistate (Ultra-light Boson) Scalar Field Dark Matter"
Bernal, T. 2018, MNRAS, 475, 1447 (ADS)
"The mass discrepancy-acceleration relation: a universal maximum dark matter acceleration and implications for the ultra-light scalar field dark matter model"
Urena-Lopez L. A., Robles V. H., Matos T. 2017, PRD, 96, 3005 (ADS)
"Mass Discrepancy-Acceleration Relation in Einstein Rings"
Tian, Y. & Jo, C.-M. 2017, MNRAS, 472, 765 (ADS)
"The radial acceleration relation in disk galaxies in the MassiveBlack-II simulation"
Tenneti, A. et al. 2018, MNRAS, 474, 3125 (ADS)
"Universal properties of centripetal accelerations in spiral galaxies"
O'Brien, J.G., Chiarelli, T.L., Mannheim, P.D. 2017, arXiv:1704.03921 (ADS)
"The scatter, residual correlations and curvature of the SPARC baryonic Tully-Fisher relation"
Desmond, H. 2017, MNRAS, 472, 35 (ADS)
"Searching for a cosmological preferred direction with 147 rotationally supported galaxies"
Zhou, Y. et al. 2017, ApJ, 847, 86 (ADS)
"Modified Dark Matter in Galaxies and Galaxy Clusters"
Edmonds, D. et al. 2018, arXiv:1801:00160 (ADS)
"Theoretical implications of the galactic radial acceleration relation of McGaugh, Lelli, and Schombert"
Nesbet, R. K. 2018, arXiv:1802:10211 (ADS)
"A Method for Discriminating Between Dark Matter Models and MOND Modified Inertia via Galactic Rotation Curves"
Petersen, J. & Frandsen, M.T. 2017, arXiv:1710:03096 (ADS)
"On the radial acceleration relation of ΛCDM satellite galaxies"
Garaldi E. et al. 2018, arXiv:1712:04448 (ADS)
"Testing the Cubic Galileon Gravity model by the Milky Way rotation curve and SPARC data"
Chan M. H. & Hui H. K. 2018, arXiv:1803.01455 (ADS)
"The radial acceleration relation is a natural consequence of the baryonic Tully-Fisher relation"
Wheeler C. et al. 2018, arXiv:1803.01455 (ADS)
"Rotation curves of galaxies and the stellar mass-to-light ratio"
Haghi H. et al. 2018, MNRAS (ADS)
"Searching for a dipole anisotropy on acceleration scale with 147 rotationally supported galaxies"
Chang Z. et al. 2018, arXiv:1803:08344 (ADS)
"The Redshift-Dependence of Radial Acceleration: Modified Gravity versus Particle Dark Matter"
Hossenfelder S. & Mistele T. 2018, arXiv:1803:08344 (ADS)
"The angular momentum-mass relation: a fundamental law from dwarf irregulars to massive spirals"
Post L. et al. 2018, arXiv:1804.04663 (ADS)
"On the radial acceleration relation for galaxies in a wide range of redshifts"
Navia C.E. 2018, arXiv:1804.05914 (ADS)
"Self-similar behavior in galaxy dynamics and distributions of dark matter"
van Putten M. 2018, arXiv:1804.06212 (ADS)
"Galactic Rotation Curves vs. Ultra-Light Dark Matter: Implications of the Soliton -- Host Halo Relation"
Bar N. et al 2018, arXiv:1805.00122 (ADS)
"Investigating Dark Matter and MOND Models with Galactic Rotation Curve Data"
Frandsen M.T. and Petersen J. 2018, arXiv:1804.04663 (ADS)
"Galaxy rotation curves in modified gravity models"
de Almeida A.O.F et al. 2018, arXiv:1804.05914 (ADS)
"Absence of a fundamental acceleration scale in galaxies"
Rodrigues D.C. et al. 2018, Nature Astronomy, 2, 668 (ADS)
"Revisiting galaxy rotation curves using a non-parametric regression method"
Fernández-Hernández L. M. et al. 2018, arXiv:1804.04663 (ADS)
"Dark matter-baryon scaling relations from Einasto halo fits to SPARC galaxy rotation curves "
Ghari A., Famaey B., Laporte C., Haghi H. 2019, arXiv:1811.06554 (ADS)
"Constraints on Chameleon f(R)-Gravity from Galaxy Rotation Curves of the SPARC Sample"
Aneesh P. Naik, Ewald Puchwein, Anne-Christine Davis, Debora Sijacki, Harry Desmond, arXiv:1905.13330 (ADS)