Fetching the paper…
Reading the bibliography…
Dark matter may be composed of light bosons, ${m_b \sim 10^{-22}\, \mathrm{eV}}$, with a de Broglie wavelength $\lambda \sim 1 \,\mathrm{kpc}$ in typical galactic potentials.
Landau, L. 1936, Phys. Z. Sowjetunion, 10, 154
1936
Earlier work this paper cites.
Chandrasekhar, S. 1942, Principles of Stellar Dynamics (Chicago: University of Chicago Press)
1942
Earlier work this paper cites.
—. 1943, ApJ, 97, 255
1943
Earlier work this paper cites.
Rosenbluth, M. N., MacDonald, W. M., & Judd, D. L. 1957, PhRv, 107, 1
1957
Earlier work this paper cites.
Hénon, M. 1960, AnAp, 23, 467
1960
Earlier work this paper cites.
Ruffini, R., & Bonazzola, S. 1969, PhRv, 187, 1767
1969
Earlier work this paper cites.
Cohen, L. 1975, in Dynamics of Stellar Systems, ed. A. Hayli, IAU Symposium 69 (Dordrecht: Reidel), 33
1975
Earlier work this paper cites.
Tremaine, S. D., Ostriker, J. P., & Spitzer, L., J. 1975, ApJ, 196, 407
1975
Earlier work this paper cites.
Begelman, M. C., Blandford, R. D., & Rees, M. J. 1980, Nature, 287, 307
1980
Earlier work this paper cites.
Tremaine, S., & Weinberg, M. D. 1984, MNRAS, 209, 729
1984
Earlier work this paper cites.
Binney, J., & Lacey, C. 1988, MNRAS, 230, 597
1988
Earlier work this paper cites.
Risken, H. 1989, The Fokker-Planck Equation. Methods of Solution and Applications (Berlin: Springer)
1989
Earlier work this paper cites.
Rauch, K. P., & Tremaine, S. 1996, New A, 1, 149
1996
Cited alongside, same era.
Navarro, J. F., Frenk, C. S., & White, S. D. M. 1997, ApJ, 490, 493
1997
Cited alongside, same era.
Hu, W., Barkana, R., & Gruzinov, A. 2000, Phys. Rev. Lett., 85, 1158
2000
Cited alongside, same era.
Binney, J., & Tremaine, S. 2008, Galactic Dynamics, 2nd ed. (Princeton University Press)
2008
Cited alongside, same era.
Heyvaerts, J. 2010, MNRAS, 407, 355
2010
Cited alongside, same era.
Klypin, A. A., Trujillo-Gomez, S., & Primack, J. 2011, ApJ, 740, 102
2011
Cited alongside, same era.
Chavanis, P.-H. 2012, Physica A, 391, 3680
Weinberg, D. H., Bullock, J. S., Governato, F., Kuzio de Naray, R., & Peter, A. H. G. 2015, PNAS, 112, 12249
2015
Later among the works it cites.
Armengaud, E., Palanque-Delabrouille, N., Yèche, C., Marsh, D. J. E., & Baur, J. 2017, MNRAS, 471, 4606
2017
Later among the works it cites.
Hui, L., Ostriker, J. P., Tremaine, S., & Witten, E. 2017, Phys. Rev. D, 95, 043541
2017
Later among the works it cites.
Iršič, V., Viel, M., Haehnelt, M. G., Bolton, J. S., & Becker, G. D. 2017, Phys. Rev. Lett., 119, 031302
2017
Later among the works it cites.
Kobayashi, T., Murgia, R., De Simone, A., Iršič, V., & Viel, M. 2017, Phys. Rev. D, 96, 123514
2017
Later among the works it cites.
Fouvry, J.-B., & Bar-Or, B. 2018, MNRAS, 481, 4566
2018
alphaXiv searches the wider corpus for related work and actual follow-ups.
alphaXiv is searching for related work…
2012
Cited alongside, same era.
Lora, V., Magaña, J., Bernal, A., Sá nchez-Salcedo, F. J., & Grebel, E. K. 2012, Journal of Cosmology and Astro-Particle Physics, 2012, 011
2012
Cited alongside, same era.
Chavanis, P. H. 2013, A&A, 556, A93
2013
Cited alongside, same era.
Kormendy, J., & Ho, L. C. 2013, ARA&A, 51, 511
2013
Cited alongside, same era.
Viel, M., Becker, G. D., Bolton, J. S., & Haehnelt, M. G. 2013, Phys. Rev. D, 88, 043502
2013
Cited alongside, same era.
Kocsis, B., & Tremaine, S. 2015, MNRAS, 448, 3265
2015
Cited alongside, same era.
Closest in time.
Leong, K.-H., Schive, H.-Y., Zhang, U.-H., & Chiueh, T. 2018, ArXiv e-prints, arXiv:1810.05930
2018
Closest in time.
Levkov, D. G., Panin, A. G., & Tkachev, I. I. 2018, Phys. Rev. Lett., 121, 151301
2018
Closest in time.
Lin, S.-C., Schive, H.-Y., Wong, S.-K., & Chiueh, T. 2018, Phys. Rev. D, 97, 103523
2018
Closest in time.
Mocz, P., Lancaster, L., Fialkov, A., Becerra, F., & Chavanis, P.-H. 2018, Phys. Rev. D, 97, 083519
2018
Closest in time.
Veltmaat, J., Niemeyer, J. C., & Schwabe, B. 2018, Phys. Rev. D, 98, 043509
2018
Closest in time.
Nori, M., Murgia, R., Iršič, V., Baldi, M., & Viel, M. 2019, MNRAS, 482, 3227
2019
Closest in time.