Built on

M. Kaplinghat, M. Valli, and H.-B. Yu, “ Too Big To Fail in Light of Gaia
Original
1904
Earlier work this paper cites.
O. Sameie, H.-B. Yu, L. V. Sales, M. Vogelsberger, and J. Zavala, “ Self-Interacting Dark Matter Subhalos in the Milky Way’s Tides
Original
1904
Earlier work this paper cites.
J. Zavala, M. R. Lovell, M. Vogelsberger, and J. D. Burger, “ The diverse dark matter density at sub-kiloparsec scales in Milky Way satellites:implications for the nature of dark matter
Original
1904
Earlier work this paper cites.
F. Kahlhoefer, M. Kaplinghat, T. R. Slatyer, and C.-L. Wu, “ Diversity in density profiles of self-interacting dark matter satellite halos
Original
1904
Earlier work this paper cites.
C. Cappiello and J. F. Beacom, “ Strong New Limits on Light Dark Matter from Neutrino Experiments
Original
1906
Earlier work this paper cites.
X. Chu, C. Garcia-Cely, and H. Murayama, “ A Practical and Consistent Parametrization of Dark Matter Self-Interactions
Original
1908
Earlier work this paper cites.
H. A. Bethe, “ Theory of the Effective Range in Nuclear Scattering
1949
Earlier work this paper cites.
S. Nussinov, “ TECHNOCOSMOLOGY: COULD A TECHNIBARYON EXCESS PROVIDE A ’NATURAL’ MISSING MASS CANDIDATE?
1985
Earlier work this paper cites.
R. S. Chivukula and T. P. Walker, “ TECHNICOLOR COSMOLOGY
1990
Earlier work this paper cites.
Butterworth-Heinemann, Oxford, 1991
L. D. Landau and E. M. Lifshits, Quantum Mechanics · 1991
Earlier work this paper cites.
A. Kusenko and M. E. Shaposhnikov, “ Supersymmetric Q balls as dark matter
1998
Earlier work this paper cites.
A. Kusenko, V. Kuzmin, M. E. Shaposhnikov, and P. G. Tinyakov, “ Experimental signatures of supersymmetric dark matter Q balls
1998
Earlier work this paper cites.
D. N. Spergel and P. J. Steinhardt, “ Observational evidence for selfinteracting cold dark matter
2000
Earlier work this paper cites.
A. Kusenko and P. J. Steinhardt, “ Q ball candidates for selfinteracting dark matter
2001
Earlier work this paper cites.
E. W. Mielke and F. E. Schunck, “ Nontopological scalar soliton as dark matter halo
2002
Earlier work this paper cites.
C. F. Perdrisat, V. Punjabi, and M. Vanderhaeghen, “ Nucleon Electromagnetic Form Factors
2007
Earlier work this paper cites.
S. W. Randall, M. Markevitch, D. Clowe, A. H. Gonzalez, and M. Bradac, “ Constraints on the Self-Interaction Cross-Section of Dark Matter from Numerical Simulations of the Merging Galaxy Cluster 1E 0657-56
Original
2008
Earlier work this paper cites.
R. Kuzio de Naray, S. S. McGaugh, and W. J. G. de Blok, “ Mass Models for Low Surface Brightness Galaxies with High Resolution Optical Velocity Fields
Original
2008
Earlier work this paper cites.
J. L. Feng, M. Kaplinghat, and H.-B. Yu, “ Halo Shape and Relic Density Exclusions of Sommerfeld-Enhanced Dark Matter Explanations of Cosmic Ray Excesses
Original
2010
Earlier work this paper cites.
D. E. Kaplan, G. Z. Krnjaic, K. R. Rehermann, and C. M. Wells, “ Atomic Dark Matter
Original
2010
Earlier work this paper cites.
B. Feldstein, A. L. Fitzpatrick, and E. Katz, “ Form Factor Dark Matter
Original
2010
Earlier work this paper cites.
S.-H. Oh, W. J. G. de Blok, E. Brinks, F. Walter, and R. C. Kennicutt, Jr, “ Dark and luminous matter in THINGS dwarf galaxies
Original
2011
Earlier work this paper cites.
M. Gillioz, A. von Manteuffel, P. Schwaller, and D. Wyler, “ The Little Skyrmion: New Dark Matter for Little Higgs Models
Original
2011
Earlier work this paper cites.

Similar

M. Vogelsberger, J. Zavala, and A. Loeb, “ Subhaloes in Self-Interacting Galactic Dark Matter Haloes
Original
2012
Cited alongside, same era.
K. Kumar, A. Menon, and T. M. P. Tait, “ Magnetic Fluffy Dark Matter
Original
2012
Cited alongside, same era.
M. Rocha, A. H. G. Peter, J. S. Bullock, M. Kaplinghat, S. Garrison-Kimmel, J. Onorbe, and L. A. Moustakas, “ Cosmological Simulations with Self-Interacting Dark Matter I: Constant Density Cores and Substructure
Original
2013
Cited alongside, same era.
A. H. G. Peter, M. Rocha, J. S. Bullock, and M. Kaplinghat, “ Cosmological Simulations with Self-Interacting Dark Matter II: Halo Shapes vs. Observations
Original
2013
Cited alongside, same era.
S. Tulin, H.-B. Yu, and K. M. Zurek, “ Beyond Collisionless Dark Matter: Particle Physics Dynamics for Dark Matter Halo Structure

Then

K. K. Boddy, M. Kaplinghat, A. Kwa, and A. H. G. Peter, “ Hidden Sector Hydrogen as Dark Matter: Small-scale Structure Formation Predictions and the Importance of Hyperfine Interactions
Original
2016
Later among the works it cites.
R. Kitano and M. Kurachi, “ Electroweak-Skyrmion as Topological Dark Matter
Original
2016
Later among the works it cites.
A. Robertson, R. Massey, and V. Eke, “ What does the Bullet Cluster tell us about self-interacting dark matter?
Original
2017
Later among the works it cites.
J. S. Bullock and M. Boylan-Kolchin, “ Small-Scale Challenges to the Λ \Lambda CDM Paradigm
Original
2017
Later among the works it cites.
A. Mitridate, M. Redi, J. Smirnov, and A. Strumia, “ Dark Matter as a weakly coupled Dark Baryon

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2019

Finite-size dark matter and its effect on small-scale structure

Chu, Xiaoyong, Garcia-Cely, Camilo, Murayama, Hitoshi

Understand

If dark matter has a finite size that is larger than its Compton wavelength, the corresponding self-interaction cross section decreases with the velocity.

We investigate the implications of this Puffy Dark Matter for addressing the small-scale problems of the $\Lambda$CDM model.
In particular, we show that the way the non-relativistic cross section varies with the velocity is largely independent of the dark matter internal structure when the range of the mediating force is very short.
We present an explicit example in the context of a QCD-like theory of dark matter and show that low-threshold direct detection experiments have the potential to probe Puffy Dark Matter.