Recognition: unknown
Infrared Spectral Gap in a Gluonic Dark Sector as the Origin of the Galactic Acceleration Scale
Pith reviewed 2026-05-10 15:41 UTC · model grok-4.3
The pith
A spectral gap in a gluonic dark sector accounts for the galactic acceleration scale through Newtonian gravity.
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
Core claim
The central claim is that the galactic acceleration scale is the gravitational imprint of a trace-anomaly-seeded infrared spectral gap in a coherent gluonic dark sector. Lorentz covariance and positive-energy lowest-weight unitary representations naturally select the Anti-de Sitter algebra so(2,3), which admits a discrete tower of states with a representation-theoretically protected gap. The associated finite correlation length r_c controls large-scale coherence. A self-gravitating condensate dominated by the lowest-weight mode then yields the acceleration g_star = G M_h / r_c^2 naturally of the observed magnitude within Newtonian gravity.
What carries the argument
The lowest-weight unitary representation of the so(2,3) algebra, which protects an infrared spectral gap and sets the correlation length r_c that governs the large-scale coherence of the gluonic condensate.
If this is right
- The acceleration scale is universal across galaxies because it depends only on the intrinsic gap rather than on individual formation histories.
- Standard Newtonian gravity suffices to explain the radial acceleration relation once the dark sector possesses this spectral rigidity.
- The dark sector consists of a color-neutral gluonic component that survives the post-inflationary expansion due to the trace anomaly.
- No additional tuning or modified gravity is required to produce the observed scale of order 10^{-10} m s^{-2}.
Where Pith is reading between the lines
- The framework may imply that dark matter halos exhibit coherence properties tied to the gap that could be tested in cluster dynamics.
- It opens a route to connect QCD-scale phenomena to astrophysical observations through the same gluonic condensate.
- Extensions could explore whether the correlation length affects structure formation at cosmological scales.
Load-bearing premise
A long-lived color-neutral gluonic vacuum component organizes at large distances into a spectrally rigid lowest-weight structure whose gap is protected by the so(2,3) algebra and directly controls galactic-scale coherence.
What would settle it
Measurement of a galaxy whose observed acceleration scale differs significantly from the value computed as G times its halo mass divided by the square of a correlation length fixed by the gap.
Figures
read the original abstract
The radial acceleration relation reveals a nearly universal acceleration scale of order $10^{-10}\,\mathrm{m\,s^{-2}}$ in galactic dynamics, whose origin remains unexplained within conventional cold dark matter scenarios. We explore the possibility that this scale is associated with an intrinsic infrared spectral property of the dark sector. Specifically, we hypothesize that a long-lived, color-neutral gluonic vacuum component surviving the post-inflationary expansion era organizes, at large distances, into a spectrally rigid lowest-weight structure. The microscopic seed for this infrared organization is provided by the QCD trace anomaly, which breaks classical scale invariance and, through dimensional transmutation, generates an intrinsic infrared scale in the gluonic sector. Within an effective representation-theoretic framework, Lorentz covariance together with a positive-energy lowest-weight unitary realization points naturally to the Anti-de Sitter algebra $\mathfrak{so}(2,3)$ as the simplest symmetry admitting a discrete tower of states with a representation-theoretically protected gap. The associated gap introduces a finite correlation length $r_{\texttt{c}}$ that controls the large-scale coherence of the dark sector. A self-gravitating condensate dominated by the lowest-weight mode then leads to a characteristic acceleration $g^{}_\star = G M_h / r_{\texttt{c}}^2$, naturally of the same order as the observed galactic acceleration scale, within standard Newtonian gravity. In this framework, the galactic acceleration scale is interpreted as the gravitational imprint of a trace-anomaly-seeded infrared spectral gap in a coherent gluonic dark sector, rather than as a consequence of modified gravity or of galaxy-by-galaxy formation histories.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The paper claims that the observed galactic radial acceleration scale (~10^{-10} m s^{-2}) arises as the gravitational imprint of an infrared spectral gap in a gluonic dark sector. The QCD trace anomaly is hypothesized to seed a long-lived color-neutral gluonic condensate that, at large distances, organizes into a spectrally rigid lowest-weight unitary representation of the so(2,3) algebra; the associated gap sets a correlation length r_c such that a self-gravitating condensate dominated by the lowest-weight mode produces g⋆ = G M_h / r_c², naturally matching the observed scale within Newtonian gravity.
Significance. If the central mapping from the trace anomaly to a protected so(2,3) gap and the resulting acceleration formula can be made rigorous and parameter-free, the work would offer a novel particle-physics origin for the galactic acceleration relation, potentially unifying QCD dynamics with large-scale structure without modified gravity or galaxy-specific CDM histories. The representation-theoretic approach to IR coherence is conceptually creative and could stimulate further exploration of algebraic structures in dark-sector models.
major comments (3)
- [Effective representation-theoretic framework] The effective representation-theoretic framework invokes Lorentz covariance and positive-energy lowest-weight unitary realizations to select so(2,3), yet no derivation connects this algebra to the QCD trace anomaly or to an effective gluonic action. The spectral gap and its protection are therefore introduced by assumption rather than obtained from the microscopic theory.
- [Characteristic acceleration and condensate] The characteristic acceleration is stated as g⋆ = G M_h / r_c², with r_c the correlation length set by the gap. This expression is not derived from the condensate dynamics or the lowest-weight mode; r_c functions as a free parameter adjusted to reproduce the observed scale, rendering the 'natural' order-of-magnitude agreement a fitting exercise rather than an independent prediction.
- [Gluonic vacuum component] The hypothesis of a long-lived, color-neutral gluonic vacuum component that survives post-inflationary expansion and organizes into a coherent structure lacks quantitative support: no lifetime estimates, dilution factors, or stability analysis against decay channels are provided, leaving the existence of the condensate as an unverified input.
minor comments (2)
- [Notation throughout] The subscript notation r_{texttt{c}} is nonstandard and reduces readability; conventional math-mode r_c is preferable.
- [Discussion of numerical match] The claim of 'natural' agreement with the galactic scale would benefit from an explicit range or error estimate on the predicted g⋆ once r_c is fixed by other considerations.
Simulated Author's Rebuttal
We thank the referee for the careful reading and constructive comments, which help clarify the scope and limitations of our effective framework. We respond to each major comment below and indicate the revisions we will make to the manuscript.
read point-by-point responses
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Referee: [Effective representation-theoretic framework] The effective representation-theoretic framework invokes Lorentz covariance and positive-energy lowest-weight unitary realizations to select so(2,3), yet no derivation connects this algebra to the QCD trace anomaly or to an effective gluonic action. The spectral gap and its protection are therefore introduced by assumption rather than obtained from the microscopic theory.
Authors: We agree that the framework is effective and does not derive the so(2,3) algebra directly from the microscopic QCD action. The trace anomaly enters by generating an intrinsic infrared scale through dimensional transmutation, which seeds the correlation length of the condensate. The algebra is selected as the minimal one compatible with Lorentz covariance and a positive-energy lowest-weight unitary representation that admits a protected discrete gap, consistent with long-distance coherence after scale invariance is broken. In the revised manuscript we will expand the relevant section to state these assumptions explicitly and motivate the algebra choice from the requirements of infrared organization in a scale-broken theory. revision: partial
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Referee: [Characteristic acceleration and condensate] The characteristic acceleration is stated as g⋆ = G M_h / r_c², with r_c the correlation length set by the gap. This expression is not derived from the condensate dynamics or the lowest-weight mode; r_c functions as a free parameter adjusted to reproduce the observed scale, rendering the 'natural' order-of-magnitude agreement a fitting exercise rather than an independent prediction.
Authors: The form g⋆ = G M_h / r_c² follows from applying the Newtonian gravitational field to a self-gravitating system whose density is dominated by the lowest-weight mode with intrinsic correlation length r_c fixed by the spectral gap. While a full dynamical derivation from the condensate equations of motion is not supplied in the present work, the expression is fixed by dimensional considerations once coherence at scale r_c is assumed. The gap itself is set by the trace-anomaly scale, so r_c is not a free parameter adjusted to data but is expected to lie near the hadronic scale, producing an acceleration of the observed order. We will add a short derivation sketch and clarify the origin of r_c in the revised manuscript. revision: partial
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Referee: [Gluonic vacuum component] The hypothesis of a long-lived, color-neutral gluonic vacuum component that survives post-inflationary expansion and organizes into a coherent structure lacks quantitative support: no lifetime estimates, dilution factors, or stability analysis against decay channels are provided, leaving the existence of the condensate as an unverified input.
Authors: The long-lived color-neutral gluonic component is introduced as a hypothesis motivated by the survival of non-perturbative gluonic degrees of freedom after inflation. The manuscript does not contain lifetime estimates, dilution factors or stability analyses, as these would require a concrete dynamical model of the dark-sector potential beyond the effective representation-theoretic treatment. In the revision we will insert a brief paragraph acknowledging this assumption and its status as an input to be examined in future work. revision: partial
Circularity Check
Galactic acceleration scale re-expressed as G M_h / r_c^2 with r_c introduced to match the observed value
specific steps
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fitted input called prediction
[Abstract]
"A self-gravitating condensate dominated by the lowest-weight mode then leads to a characteristic acceleration g^{}_⋆ = G M_h / r_{texttt{c}}^2, naturally of the same order as the observed galactic acceleration scale, within standard Newtonian gravity."
The acceleration is written directly as G M_h / r_c^2 where r_c is the finite correlation length introduced by the spectral gap; the paper presents the result as naturally matching the observed scale, but the gap (and thus r_c) is not computed from the trace anomaly or gluonic dynamics to that specific value, so the match is achieved by the choice of the input parameter r_c.
full rationale
The paper's derivation proceeds from the trace anomaly seeding an IR gluonic scale, to an effective so(2,3) lowest-weight structure with protected gap, to a correlation length r_c, to the acceleration g⋆ = G M_h / r_c^2 claimed to be naturally of the observed order. The final equality holds by construction once r_c is chosen to reproduce the galactic scale (many orders removed from standard QCD scales), with no independent first-principles computation of the gap value supplied in the text. The so(2,3) choice is motivated as the 'simplest symmetry' admitting the structure but is not derived from the QCD Lagrangian or trace anomaly, leaving the central numerical match as a reparametrization of the input scale rather than a prediction. This constitutes fitted-input circularity on the load-bearing claim while the representation-theoretic framing retains some independent content.
Axiom & Free-Parameter Ledger
free parameters (1)
- correlation length r_c =
chosen to yield ~10^{-10} m s^{-2}
axioms (2)
- domain assumption Lorentz covariance together with a positive-energy lowest-weight unitary realization points naturally to the Anti-de Sitter algebra so(2,3) as the simplest symmetry admitting a discrete tower with a protected gap
- standard math The QCD trace anomaly breaks classical scale invariance and through dimensional transmutation generates an intrinsic infrared scale in the gluonic sector
invented entities (2)
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long-lived, color-neutral gluonic vacuum component
no independent evidence
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spectrally rigid lowest-weight structure
no independent evidence
Reference graph
Works this paper leans on
-
[1]
The polarisation of the condensate around baryonic mass concentrations. In analogy with the polarisa- tion of a dielectric medium placed in an external electric field, the dipolar modes can generate a spa- tial displacement of the condensate density toward the baryonic potential minimum
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[2]
The directional response of the DM distribution to an external gravitational field. Because theY 1m harmonics encode a preferred direction, the excita- tion of the (0,1) modes can produce anisotropic dis- tortions of the halo density aligned with the bary- onic mass distribution
-
[3]
breathing
The formation of asymmetric DM wakes generated by moving baryonic objects. Such wakes could arise from the coherent excitation of dipolar modes in the condensate and could provide a natural microscopic mechanism for dynamical friction acting on stars, stellar clusters, or satellite galaxies moving through the halo. The (n, l) = (0,1) triplet carries the l...
-
[4]
Slow radial pulsations of the DM core
-
[5]
Episodic energy exchange between the condensate and the baryonic environment
-
[6]
Modulation of the inner density profile through pe- riodic redistribution of mass within the halo core. C. Order-of-Magnitude Estimates The characteristic scales of the condensate are set by the curvature parameterκand by the effective di-gluonic massm eff as determined by Eqs. (3) (see also Eq. (26)): meff = Erest AdS c2 = ℏ rcc ζ .(51) This quantity cha...
1991
-
[7]
core radius
This analogy should not be overinterpreted. In the present framework, the distinction betweenζ= 3 2 andζ= 1 2 is governed not by the density falloff alone, but by the functional setting, in particular by the measure entering the norm and nor- 17 Model ρ(x) M(< x) Gluonic condensate ρc(1 +x 2)−ζ 4πρcr3 0 F(x, ζ) NFW ρs x(1 +x) 2 4πρsr3 0 ln(1 +x)− x 1 +x B...
-
[8]
The value ofxbeyond which the central approxi- mationM DM(< x, ζ)∼ 4 3 πρcr3 c x3 (72) is no longer valid, signaling the breakdown of the constant- density regime
-
[9]
The value ofx=x max (73) corresponding to the inflection point of the enclosed-mass profile, where the curvature ofM DM(< x, ζ) changes sign and the mass growth begins to slow
-
[10]
The value ofx=x v;max (81) (see also (85)) at which the circular velocityv(x, ζ) reaches its max- imum
-
[11]
Although these definitions are not identical, they all select radii of the same order, thereby identifying a char- acteristic scale of the halo set byr c
The value ofx=x g;max (92) at which the radial accelerationg(x, ζ) attains its maximum. Although these definitions are not identical, they all select radii of the same order, thereby identifying a char- acteristic scale of the halo set byr c. This reflects the ex- istence of an intermediate radial region separating the in- ner constant-density core from t...
-
[12]
At the inflection radiusx= 1 (r∼r c), the enclosed mass fraction is: F(1,2) F(∞,2) ∼0.18,(100) and the circular velocity (76) is: v(1,2) = s GMDM(< r c) rc ∼28 km s−1 .(101)
-
[13]
In the following, illustrative Figs
At a few core radii, sayx≃3 (r≃3r c), the en- closed mass fraction increases to: F(3,2) F(∞,2) ∼0.6,(102) while the circular velocity (76) reaches: v(3,2) = s GMDM(<3r c) 3rc ∼30 km s−1 .(103) 19 These values are of the order typically observed in dwarf- galaxy rotation curves. In the following, illustrative Figs. 6 and 7 (in arbitrary units withρ c =r c ...
-
[14]
can respond to the tidal gravitational field gener- ated by the baryonic mass distribution
-
[15]
can develop multipolar deformations encoded by modes withl≥1; see Sect. IV A
-
[16]
can undergo breathing and higher radial oscilla- tions associated with modes withn≥1; see Sect. IV B
-
[17]
The first excited levels thus play an important physical role
can exert a gravitational backreaction on the baryonic component, potentially affecting rotation curves, dynamical friction, and the stability of stel- lar systems. The first excited levels thus play an important physical role. They encode the leading deviations from spherical symmetry and quantify the dynamical susceptibility of the condensate to baryoni...
-
[18]
At large radii (∼70kpc),g obs decreases to ∼10 −10.5 m s−2, whileg bar ≲10 −11 m s−2, allow- ing the DM contribution to become significant
The massive spiral galaxy NGC 2841, with flat ro- tation velocities of order 300km s−1, reachesg obs ∼ gbar ≃10 −9 m s−2 within a few kiloparsecs of the center, where the DM contribution is negligi- ble. At large radii (∼70kpc),g obs decreases to ∼10 −10.5 m s−2, whileg bar ≲10 −11 m s−2, allow- ing the DM contribution to become significant
-
[19]
The gas-dominated dwarf galaxy IC 2574, with ro- tation velocities below 80km s −1, reaches a max- imal observed acceleration of∼10 −10.7 m s−2 at radii of 8-10kpc, while the baryonic acceleration there is an order of magnitude smaller, indicating a regime dominated by DM. B. From the Intrinsic DM Halo Scale to the RAR Scale The AdS-Bose-Einstein condensa...
-
[20]
The orbital velocities satisfyv≪c
-
[21]
The gravitational potential obeys|Φ|/c 2 ≪1
-
[22]
One does not attempt to describe genuinely rela- tivistic phenomena such as strong lensing or strong- field dynamics. These conditions are well satisfied in galaxies, support- ing the use of the Newtonian relation (142) even though the microscopic description of the dark sector involves an effective AdS geometry. e. A more systematic formulation.A fully e...
-
[23]
Cohen-Tannoudji,Lambda, the fifth foundational con- stant considered by Einstein, Metrologia,55, 486 (2018)
G. Cohen-Tannoudji,Lambda, the fifth foundational con- stant considered by Einstein, Metrologia,55, 486 (2018)
2018
-
[24]
Gazeau,Mass in de Sitter and Anti-de Sitter Uni- verses with Regard to Dark Matter, Universe,6, 66 (2020)
J.-P. Gazeau,Mass in de Sitter and Anti-de Sitter Uni- verses with Regard to Dark Matter, Universe,6, 66 (2020)
2020
-
[25]
Cohen-Tannoudji and J.-P
G. Cohen-Tannoudji and J.-P. Gazeau,Cold DM: A Glu- onic Bose-Einstein Condensate in Anti-de Sitter Space Time, Universe,7, 402 (2021)
2021
-
[26]
Cohen-Tannoudji and J.-P
G. Cohen-Tannoudji and J.-P. Gazeau,DM as a QCD effect in an Anti-de Sitter Geometry: Cosmogonic Impli- cations of de Sitter, Anti-de Sitter and Poincar´ e Symme- tries, SciPost Phys. Proc.,14, 004 (2023)
2023
-
[27]
Cohen-Tannoudji, J.-P
G. Cohen-Tannoudji, J.-P. Gazeau, H. Pejhan, and J.- P. Treuil,A QCD-Motivated Gluonic Condensate for the Galactic Acceleration Scale, in preparation; forthcoming on arXiv (2026)
2026
-
[28]
S. L. Adler,Einstein gravity as a symmetry-breaking ef- fect in quantum field theory, Rev. Mod. Phys.,54, 729- 766 (1982)
1982
-
[29]
S. S. McGaugh, F. Lelli, and J. M. Schombert,Radial Acceleration Relation in Rotationally Supported Galaxies, Phys. Rev. Lett.,117(20), 201101 (2016)
2016
-
[30]
Lelli, S
F. Lelli, S. S. McGaugh, J. M. Schombert,SPARC: Mass Models for 175 Disk Galaxies with Spitzer Photom- etry and Accurate Rotation Curves, Astron. J.,152, 157 (2016)
2016
-
[31]
Lelli, S.S
F. Lelli, S.S. McGaugh, J. M. Schombert, and M. S. Pawlowski,One Law to Rule Them All: the Radial Accel- eration Relation of Galaxies, Astrophys. J.,836(2), 152 (2017)
2017
-
[32]
A. D. Ludlow, et al.,Mass-Discrepancy Acceleration Re- lation: a Natural Outcome of Galaxy Formation in Cold Dark Matter Halos, Phys. Rev. Lett.,118(16), 161103 (2017)
2017
-
[33]
B. W. Keller and J. W. Wadsley, ΛCDM is Consistent with SPARC Radial Acceleration Relation, Astrophys. J. Lett.,835(1), L17 (2017)
2017
-
[34]
J. F. Navarro, et al.,The Origin of the Mass Discrepancy- Acceleration Relation inΛCDM, Mon. Not. R. Astron. Soc.,471(2), 1841-1848 (2017)
2017
-
[35]
Desmond,The Scatter, Residual Correlations and Curvature of the SPARC Baryonic Tully-Fisher Relation, Mon
H. Desmond,The Scatter, Residual Correlations and Curvature of the SPARC Baryonic Tully-Fisher Relation, Mon. Not. R. Astron. Soc.,472, L35-L39 (2017)
2017
-
[36]
Famaey and S
B. Famaey and S. S. McGaugh,Modified Newtonian 29 Dynamics (MOND): Observational Phenomenology and Relativistic Extensions, Liv. Rev. Relativ.,15, 10 (2012)
2012
-
[37]
M. P. J´ ulio, J. I. Read, M. S. Pawlowski, P. Li, D. Vaz, J. Brinchmann, M. P. Rey, O. Agertz, and T. Holmes, The Radial Acceleration Relation at the EDGE of Galaxy Formation; Testing its Universality in Low-Mass Dwarf GalaxiesA&A,704, A330 (2026)
2026
-
[38]
Hastings and T
M.B. Hastings and T. Koma,Spectral gap and expo- nential decay of correlations, Commun. Math. Phys., 265(3), 781-804 (2006)
2006
-
[39]
Pasechnik and M
R. Pasechnik and M. ˇSumbera,Phenomenological Re- view on Quark-Gluon Plasma: Concepts vs. Observa- tions, Universe,3(1), 7 (2017)
2017
-
[40]
V. F. Mukhanov,Gravitational Instability of the Uni- verse Filled with a Scalar Field, JETP Lett.,41, 493-496 (1985)
1985
-
[41]
Sasaki,Large Scale Quantum Fluctuations in the In- flationary Universe, Prog
M. Sasaki,Large Scale Quantum Fluctuations in the In- flationary Universe, Prog. Theor. Phys.,76, 1036-1046, (1986)
1986
-
[42]
Weinberg,Cosmology, Oxford University Press, (2008)
S. Weinberg,Cosmology, Oxford University Press, (2008)
2008
-
[43]
Cheung, P
C. Cheung, P. Creminelli, A. L. Fitzpatrick, J. Kaplan, and L. Senatore,The Effective Field Theory of Inflation, JHEP,03, 014, (2008)
2008
-
[44]
D. Baumann,TASI Lectures on Inflation, arXiv:0907.5424v2 [hep-th] (2011)
work page Pith review arXiv 2011
-
[45]
Fronsdal,Elementary Particles in a Curved Space
C. Fronsdal,Elementary Particles in a Curved Space. II, Phys. Rev. D,10, 589 (1974)
1974
-
[46]
Fronsdal,Elementary Particles in a Curved Space
C. Fronsdal,Elementary Particles in a Curved Space. IV. Massless Particles, Phys. Rev. D,12(12), 3819 (1975)
1975
-
[47]
Enayati, J.-P
M. Enayati, J.-P. Gazeau, M. A. del Olmo, H. Pe- jhan,Anti-de Sitterian “massive” elementary systems and their Minkowskian and Newton-Hooke contraction limits, J. Math. Phys.,66, 053501 (2025)
2025
-
[48]
Enayati, J.-P
M. Enayati, J.-P. Gazeau, H. Pejhan, and A. Wang,The de Sitter (dS) Group and its Representations(2nd edi- tion), Springer, Cham, Switzerland (2024)
2024
-
[49]
C. J. Morningstar and M. Peardon,Glueball Spectrum from an Anisotropic Lattice Study, Phys. Rev. D,60(3), 034509 (1999)
1999
-
[50]
Massless Representations in Conformal Space and Their de Sitter Restrictions
J.-P. Gazeau, H. Pejhan, and I. Todorov,Massless Rep- resentations in Conformal Space and Their de Sitter Re- strictions, arXiv:2601.18433 (2026)
work page internal anchor Pith review Pith/arXiv arXiv 2026
-
[51]
K. G. Begeman, A. H. Broeils, and R. H. Sanders,Ex- tended Rotation Curves of Spiral Galaxies: Dark Haloes and Modified Dynamics, Mon. Not. R. Astron. Soc.,249, 523-537 (1991)
1991
-
[52]
J. F. Navarro, C. S. Frenk, and S. D. M. White,A Uni- versal Density Profile From Hierarchical Clustering, As- trophys. J.,490, 493-508 (1997)
1997
-
[53]
Burkert,The Structure of DM Halos in Dwarf Galax- ies, Astrophys
A. Burkert,The Structure of DM Halos in Dwarf Galax- ies, Astrophys. J. Lett.,447, L25-L28 (1995)
1995
-
[54]
J. I. Read, O. Agertz, and M. L. M. Collins,DM Cores All the Way Down, Mon. Not. R. Astron. Soc.,459, 2573- 2590 (2016)
2016
-
[55]
P. Li, F. Lelli, S. S. McGaugh, and J. M. Schombert, A Comprehensive Catalog of Dark Matter Halo Models for SPARC Galaxies, Astrophys. J. Suppl. Ser.,247, 31 (2020)
2020
-
[56]
W. J. G. de Blok,The Core-Cusp Problem, Adv. Astron., 2010, 789293 (2010)
2010
-
[57]
Lelli, S
F. Lelli, S. S. McGaugh, and J. M. Schombert,The Bary- onic Tully-Fisher Relation and the Limits of Galaxy Scal- ing Laws, Astron. Astrophys.,615, A3 (2018)
2018
-
[58]
L. Hui, J. P. Ostriker, S. Tremaine, E. Witten,Ultralight Scalars as Cosmological Dark Matter, Phys. Rev. D,95, 043541 (2017)
2017
-
[59]
W. Hu, R. Barkana, and A. Gruzinov,Fuzzy Cold Dark Matter: The Wave Properties of Ultralight Particles, Phys. Rev. Lett.,85, 1158-1161 (2000)
2000
-
[60]
Schive, T
H.-Y. Schive, T. Chiueh, and T. Broadhurst,Cosmic Structure as the Quantum Interference of a Coherent Dark Wave, Nature Phys.,10, 496-499 (2014)
2014
-
[61]
M. M. Brouwer, et al.The Weak Lensing Radial Acceler- ation Relation: Constraining Modified Gravity and Cold Dark Matter Theories with KiDS-1000, Astronomy & As- trophysics,650, A113 (2021)
2021
-
[62]
Mistele, et al.Radial Acceleration Relation of Galaxies with Joint Kinematic and Weak-Lensing Data, JCAP., 04, 020 (2024)
T. Mistele, et al.Radial Acceleration Relation of Galaxies with Joint Kinematic and Weak-Lensing Data, JCAP., 04, 020 (2024)
2024
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