Recognition: unknown
Emergence of Complex Structures
Pith reviewed 2026-05-10 15:36 UTC · model grok-4.3
The pith
A Lagrangian-Eulerian transport map governs density amplification through its Jacobian while anisotropic collapse follows from the eigenvalues of successive deformation tensors.
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
Core claim
Using the Lagrangian-Eulerian transport map, density amplification is controlled by the Jacobian of the deformation, and anisotropic collapse arises from the eigenvalues of a hierarchy of deformation tensors. Long-range interactions are encoded directly in the displacement field, so nonlocality enters through transport. This geometric picture connects to a maximum-entropy Gaussian baseline; nonlinear transport and nonlocal coupling then produce scale coupling, higher-order correlations, and non-Gaussianity. A Landau-Ginzburg description interprets the growth of seed anisotropies as the activation of lower effective free-energy branches, realizing self-organization at the coarse-grained level
What carries the argument
The Lagrangian-Eulerian transport map, which encodes density change via the Jacobian of the deformation and anisotropic directions via the eigenvalues of a hierarchy of deformation tensors.
If this is right
- Coarse-grained spatial fields become more ordered as structure forms even as the full phase-space description increases in complexity through multistreaming and velocity degrees of freedom.
- Nonlinear transport from an initial Gaussian field generates scale coupling, higher-order correlations, and non-Gaussianity.
- Self-organization appears in the coarse-grained description as the activation of lower free-energy branches in the effective Landau-Ginzburg model.
- In cosmology the nonlocal tidal field influences structure formation already at moderate rather than only at high overdensities.
Where Pith is reading between the lines
- The same transport-based separation of description levels could be applied to other systems where apparent ordering occurs alongside entropy growth, such as galaxy clustering or certain fluid instabilities.
- If the onset of tidal relevance at moderate overdensity holds, simulations could test it directly by isolating the tidal term in the density evolution equation at different density thresholds.
- The framework suggests that non-Gaussian statistics in large-scale structure can be derived from geometry rather than introduced by hand.
Load-bearing premise
The proposed transport geometry plus its link to a maximum-entropy Gaussian baseline and Landau-Ginzburg effective description accurately captures the dynamics and entropy behavior across scales without additional unstated assumptions about microscopic interactions.
What would settle it
A measurement in N-body simulations or observational data of the tidal field's contribution to density evolution showing whether its effect on structure growth becomes significant already at moderate overdensities (delta approximately 1 to 5) rather than only at high overdensities.
read the original abstract
Complex structures often emerge from initially homogeneous or weakly correlated states. We address the apparent tension between this ordering and entropy growth through a unified framework combining semi-microscopic phase-space dynamics, transport geometry, information theory, and coarse-grained effective modeling. The key point is that entropy depends on the level of description: a coarse-grained spatial field may become more ordered as structure forms, even while the full phase-space description becomes more complex through shell crossing, multistreaming, and the activation of velocity degrees of freedom. Using a Lagrangian--Eulerian transport map, we show how density amplification is governed by the Jacobian of the deformation and how anisotropic collapse arises from the eigenvalues of a hierarchy of deformation tensors. Long-range interaction or information flow is encoded in the displacement field, so that nonlocality enters directly through transport. We connect this geometric description to a maximum-entropy Gaussian baseline and show how nonlinear transport and nonlocal coupling generate scale coupling, higher-order correlations, and non-Gaussianity. We then formulate a Landau--Ginzburg description in which the growth of seed anisotropies is interpreted as the activation of lower effective free-energy branches, providing a coarse-grained realization of self-organization. Applied to generated cosmological fields, this framework indicates that the nonlocal tidal level becomes relevant already at moderate overdensity. Although cosmological structure formation is the main realization considered here, the framework is intended more broadly as a mesoscopic language for systems in which transport, anisotropy, nonlocality, and self-organization are central.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The manuscript proposes a unified conceptual framework for the emergence of complex structures from initially homogeneous states, with a focus on cosmological density fields. It combines Lagrangian-Eulerian transport geometry, phase-space dynamics, information theory, and a Landau-Ginzburg effective description to argue that entropy is level-dependent, allowing coarse-grained ordering to coexist with increasing microscopic complexity via shell crossing and multistreaming. Density amplification is governed by the Jacobian of the deformation map, anisotropic collapse follows from the eigenvalues of a hierarchy of deformation tensors, and nonlocality enters through the displacement field. Nonlinear transport and coupling to a maximum-entropy Gaussian baseline are said to generate scale coupling, higher-order correlations, and non-Gaussianity, with seed anisotropies activating lower free-energy branches; the framework concludes that nonlocal tidal effects become relevant already at moderate overdensity in generated cosmological fields.
Significance. If the interpretive mappings from transport geometry to the effective model are valid and can be made quantitative, the work could supply a mesoscopic language that bridges geometric descriptions of collapse with information-theoretic and coarse-grained field-theoretic ideas, offering a fresh perspective on the onset of non-Gaussianity and self-organization in gravitational systems beyond standard perturbation theory.
major comments (2)
- [Abstract] Abstract: the central claim that 'the nonlocal tidal level becomes relevant already at moderate overdensity' rests on an interpretive step linking the nonlocal displacement field and deformation-tensor eigenvalue hierarchy to the activation of lower free-energy branches in the Landau-Ginzburg description; no explicit derivation of how nonlocality enters the effective potential coefficients or any controlled isolation of the tidal contribution at a specific overdensity threshold is supplied.
- [Abstract] Abstract and framework description: the connection between the maximum-entropy Gaussian baseline, nonlinear transport, and the generation of non-Gaussianity is asserted without supporting equations, error analysis, or comparison against standard results (e.g., known thresholds for tidal influence in N-body or perturbation-theory calculations), rendering the quantitative aspect of the conclusion difficult to verify.
minor comments (1)
- [Abstract] The abstract refers to 'generated cosmological fields' without indicating the generation method, resolution, or cosmological parameters employed, which would aid reproducibility and assessment of the claimed moderate-overdensity regime.
Simulated Author's Rebuttal
We thank the referee for the careful reading and constructive feedback on our manuscript. We address each major comment point by point below, clarifying the conceptual nature of the framework while incorporating revisions to improve transparency and verifiability where feasible.
read point-by-point responses
-
Referee: [Abstract] Abstract: the central claim that 'the nonlocal tidal level becomes relevant already at moderate overdensity' rests on an interpretive step linking the nonlocal displacement field and deformation-tensor eigenvalue hierarchy to the activation of lower free-energy branches in the Landau-Ginzburg description; no explicit derivation of how nonlocality enters the effective potential coefficients or any controlled isolation of the tidal contribution at a specific overdensity threshold is supplied.
Authors: We agree that the indicated connection is interpretive rather than derived from first principles in the current text, and that no explicit mapping of nonlocality into the effective potential coefficients or isolation of a precise overdensity threshold is provided. The framework is intended as a mesoscopic conceptual bridge, not a quantitative derivation. In revision we have expanded the relevant discussion (new paragraph in Section 3) to spell out the interpretive steps more explicitly, added a clarifying sentence in the abstract noting the qualitative character of the 'moderate overdensity' statement, and inserted a forward-looking remark that a controlled quantitative isolation would require further work. We do not claim to have performed such an isolation. revision: partial
-
Referee: [Abstract] Abstract and framework description: the connection between the maximum-entropy Gaussian baseline, nonlinear transport, and the generation of non-Gaussianity is asserted without supporting equations, error analysis, or comparison against standard results (e.g., known thresholds for tidal influence in N-body or perturbation-theory calculations), rendering the quantitative aspect of the conclusion difficult to verify.
Authors: The manuscript presents a unifying conceptual framework in which the stated connections are described at a descriptive level. We acknowledge that the original abstract and framework overview contain no supporting equations, error analysis, or direct comparisons to N-body or perturbation-theory thresholds. To address this we have added explicit transport equations in Section 2 illustrating how nonlinear displacement from a Gaussian baseline produces higher-order correlations, and we have inserted a short comparative paragraph (with citations) relating the onset of tidal relevance to known results from standard perturbation theory and N-body work. A full error analysis lies outside the scope of this perspective-style paper and is not supplied. revision: partial
Circularity Check
No circularity: geometric and effective-model steps remain independent
full rationale
The abstract and framework description derive density amplification from the Jacobian of a Lagrangian-Eulerian transport map, anisotropic collapse from deformation-tensor eigenvalues, and non-Gaussianity from nonlinear transport plus nonlocal coupling. These steps are presented as direct consequences of the transport geometry and information-theoretic baseline rather than fitted parameters renamed as predictions or self-definitional loops. The Landau-Ginzburg interpretation of anisotropy growth is introduced as a coarse-grained realization, not as a reduction to prior self-cited results. No equations or claims in the provided text exhibit a quantity being defined in terms of itself or a central result forced by self-citation. The overall chain is therefore self-contained against external benchmarks.
Axiom & Free-Parameter Ledger
axioms (2)
- domain assumption Maximum-entropy Gaussian baseline provides the reference state for connecting geometric transport to information measures
- domain assumption Lagrangian-Eulerian transport map and its Jacobian fully govern density amplification and anisotropy via deformation tensor eigenvalues
Reference graph
Works this paper leans on
-
[1]
Padmanabhan, T.: Thermodynamical aspects of gravity: new insights. Reports on Progress in Physics73(4), 046901 (2010) https://doi.org/10.1088/0034-4885/ 73/4/046901 arXiv:0911.5004 [gr-qc]
-
[2]
Susskind, L.: The world as a hologram. Journal of Mathematical Physics36(11), 6377–6396 (1995) https://doi.org/10.1063/1.531249 arXiv:hep-th/9409089 [hep- th]
-
[3]
Thermodynamics of Spacetime: The Einstein Equation of State
Jacobson, T.: Thermodynamics of Spacetime: The Einstein Equation of State. Physical Review Letters75(7), 1260–1263 (1995) https://doi.org/10.1103/ PhysRevLett.75.1260 arXiv:gr-qc/9504004 [gr-qc]
work page Pith review arXiv 1995
-
[4]
On the origin of gravity and the laws of Newton
Verlinde, E.: On the origin of gravity and the laws of Newton. Journal of High Energy Physics2011, 29 (2011) https://doi.org/10.1007/JHEP04(2011)029 arXiv:1001.0785 [hep-th]
-
[5]
Bianconi, G.: Gravity from entropy. Physical Review D111(6), 066001 (2025) https://doi.org/10.1103/PhysRevD.111.066001 arXiv:2408.14391 [gr-qc]
-
[6]
The Thermodynamics of the Gravity from Entropy Theory
Bianconi, G.: The Thermodynamics of the Gravity from Entropy Theory. arXiv e-prints, 2510–22545 (2025) https://doi.org/10.48550/arXiv.2510.22545 arXiv:2510.22545 [gr-qc]
work page internal anchor Pith review Pith/arXiv arXiv doi:10.48550/arxiv.2510.22545 2025
-
[7]
Carroll, S.M., Remmen, G.N.: What is the entropy in entropic gravity? Physical Review D93(12), 124052 (2016) https://doi.org/10.1103/PhysRevD.93.124052 arXiv:1601.07558 [hep-th]
-
[8]
Bekenstein, J.D.: Black Holes and Entropy. Physical Review D7(8), 2333–2346 (1973) https://doi.org/10.1103/PhysRevD.7.2333
-
[9]
Physical Review D13(2), 191–197 (1976) https://doi.org/10.1103/PhysRevD.13.191
Hawking, S.W.: Black holes and thermodynamics. Physical Review D13(2), 191–197 (1976) https://doi.org/10.1103/PhysRevD.13.191
-
[10]
Cosmological event horizons, thermodynamics, and particle creation,
Gibbons, G.W., Hawking, S.W.: Cosmological event horizons, thermodynamics, and particle creation. Physical Review D15(10), 2738–2751 (1977) https://doi. org/10.1103/PhysRevD.15.2738
-
[11]
Communications in Mathematical Physics31(2), 161–170 (1973) https://doi
Bardeen, J.M., Carter, B., Hawking, S.W.: The four laws of black hole mechanics. Communications in Mathematical Physics31(2), 161–170 (1973) https://doi. org/10.1007/BF01645742 31
-
[12]
ACS Nano14(5), 5417–5425 (2020) https: //doi.org/10.1021/acsnano.9b08984
Carrithers, A.D., Brown, M.J.V., Rashed, M.Z., Islam, S., Velev, O.D., Williams, S.J.: Multiscale self-assembly of distinctive weblike structures from evaporated drops of dilute american whiskeys. ACS Nano14(5), 5417–5425 (2020) https: //doi.org/10.1021/acsnano.9b08984
-
[13]
Journal of Fluid Mechanics749, 649–665 (2014) https://doi.org/ 10.1017/jfm.2014.220
Bennacer, R., Sefiane, K.: Vortices, dissipation and flow transition in volatile binary drops. Journal of Fluid Mechanics749, 649–665 (2014) https://doi.org/ 10.1017/jfm.2014.220
-
[14]
Papo, D., Buld´ u, J.M.: Does the brain behave like a (complex) network? I. Dynamics. Physics of Life Reviews48, 47–98 (2024) https://doi.org/10.1016/j. plrev.2023.12.006 arXiv:2412.15711 [q-bio.NC]
work page doi:10.1016/j 2024
-
[15]
Warren, D.E., Power, J.D., Bruss, J., Denburg, N.L., Waldron, E.J., Sun, H., Petersen, S.E., Tranel, D.: Network measures predict neuropsychological outcome after brain injury. Proceedings of the National Academy of Science 111(39), 14247–14252 (2014) https://doi.org/10.1073/pnas.1322173111
-
[16]
Proceedings of the National Academy of Sciences120(33) (2023) https://doi.org/10.1073/pnas
Giusti, C., Pastalkova, E., Curto, C., Itskov, V.: Clique topology reveals intrin- sic geometric structure in neural correlations. Proceedings of the National Academy of Science112(44), 13455–13460 (2015) https://doi.org/10.1073/pnas. 1506407112 arXiv:1502.06172 [q-bio.NC]
-
[17]
Frontiers in Physics8(2020) https://doi.org/10.3389/ fphy.2020.525731
Vazza, F., Feletti, A.: The quantitative comparison between the neuronal net- work and the cosmic web. Frontiers in Physics8(2020) https://doi.org/10.3389/ fphy.2020.525731
-
[18]
NeuroImage321, 121500 (2025) https://doi.org/10.1016/j.neuroimage.2025.121500
Rosell, A.C., Janssen, N., Maselli, A., Pereda, E., Huertas-Company, M., Kitaura, F.-S.: Scale-dependent brain age with cosmological higher-order statis- tics from structural magnetic resonance imaging. NeuroImage321, 121500 (2025) https://doi.org/10.1016/j.neuroimage.2025.121500
-
[19]
Scientific Reports 15(1), 42309 (2025) https://doi.org/10.1038/s41598-025-26438-7
Kitaura, F.-S., Kitaura, E.-P., Janssen, N., Maselli, A., Pereda, E., Carnero Rosell, A.: Higher-order sonification of the human brain. Scientific Reports 15(1), 42309 (2025) https://doi.org/10.1038/s41598-025-26438-7
-
[20]
Journal of Forestry Research 33(4), 1301–1315 (2022) https://doi.org/10.1007/s11676-021-01417-6
Xin, H., Jackson, T., Cao, Y., Zhang, H., Lin, Y., Shenkin, A.: Spatial pattern analysis of forest trees based on the vectorial mark. Journal of Forestry Research 33(4), 1301–1315 (2022) https://doi.org/10.1007/s11676-021-01417-6
-
[21]
an application to mediterranean fir abies pinsapo boiss stands
Abellanas, B., Abellanas, M., Pommerening, A., Lodares, D., Cuadros, S.: A forest simulation approach using weighted voronoi diagrams. an application to mediterranean fir abies pinsapo boiss stands. Forest Systems25(2), 062 (2016) https://doi.org/10.5424/fs/2016252-08021
-
[22]
MNRAS502(3), 3456–3475 (2021) https://doi.org/10.1093/mnras/staa3774 arXiv:1911.00284 [astro-ph.CO]
Kitaura, F.-S., Ata, M., Rodr´ ıguez-Torres, S.A., Hern´ andez-S´ anchez, M., 32 Balaguera-Antol´ ınez, A., Yepes, G.: COSMIC BIRTH: efficient Bayesian infer- ence of the evolving cosmic web from galaxy surveys. MNRAS502(3), 3456–3475 (2021) https://doi.org/10.1093/mnras/staa3774 arXiv:1911.00284 [astro-ph.CO]
-
[23]
Jasche, J., Lavaux, G.: Physical Bayesian modelling of the non-linear matter distribution: New insights into the nearby universe. Astronomy & Astrophysics 625, 64 (2019) https://doi.org/10.1051/0004-6361/201833710 arXiv:1806.11117 [astro-ph.CO]
-
[24]
Libeskind, N.I., Van de Weygaert, R., Cautun, M., Falck, B., Tempel, E., Abel, T., Alpaslan, M., Arag´ on-Calvo, M.A., Forero-Romero, J.E., Gonzalez, R., Gottl¨ ober, S., Hahn, O., Hellwing, W.A., Hoffman, Y., Jones, B.J.T., Kitaura, F.-S., Knebe, A., Manti, S., Neyrinck, M., Nuza, S.E., Padilla, N., Platen, E., Ramachandra, N., Robotham, A., Saar, E., Sh...
-
[25]
Cautun, M., Weygaert, R., Jones, B.J.T., Frenk, C.S.: Evolution of the cosmic web. Monthly Notices of the Royal Astronomical Soci- ety441(4), 2923–2973 (2014) https://doi.org/10.1093/mnras/stu768 https://academic.oup.com/mnras/article-pdf/441/4/2923/4046922/stu768.pdf
-
[28]
Accessed 2025-05-17
Jasche, J., Leclercq, F., Wandelt, B.D.: Past and present cosmic structure in the SDSS DR7 main sample2015(01), 036 (2015) https://doi.org/10.1088/ 1475-7516/2015/01/036 . Accessed 2025-05-17
2015
-
[29]
Astrophysical Journal723(1), 364–382 (2010) https://doi
Arag´ on-Calvo, M.A., Platen, E., Van de Weygaert, R., Szalay, A.S.: The Spine of the Cosmic Web. Astrophysical Journal723(1), 364–382 (2010) https://doi. org/10.1088/0004-637X/723/1/364 arXiv:0809.5104 [astro-ph]
-
[30]
Reports on Progress in Physics61(4), 353–430 (1998) https://doi.org/10.1088/ 0034-4885/61/4/002
Ermentrout, B.: Neural networks as spatio-temporal pattern-forming systems. Reports on Progress in Physics61(4), 353–430 (1998) https://doi.org/10.1088/ 0034-4885/61/4/002
1998
-
[31]
Physical Review X5(2), 021028 (2015) https://doi.org/10
Montbri´ o, E., Paz´ o, D., Roxin, A.: Macroscopic Description for Networks of Spiking Neurons. Physical Review X5(2), 021028 (2015) https://doi.org/10. 33 1103/PhysRevX.5.021028 arXiv:1506.06581 [q-bio.NC]
-
[32]
Journal of Physics A Mathematical General45(3), 033001 (2012) https://doi.org/10.1088/ 1751-8113/45/3/033001
Bressloff, P.C.: Spatiotemporal dynamics of continuum neural fields. Journal of Physics A Mathematical General45(3), 033001 (2012) https://doi.org/10.1088/ 1751-8113/45/3/033001
2012
-
[33]
Yoshikawa, K., Yoshida, N., Umemura, M.: Direct Integration of the Collisionless Boltzmann Equation in Six-dimensional Phase Space: Self-gravitating Systems. Astrophysical Journal762(2), 116 (2013) https://doi.org/10.1088/0004-637X/ 762/2/116 arXiv:1206.6152 [astro-ph.IM]
-
[34]
Sousbie, T., Colombi, S.: ColDICE: A parallel Vlasov-Poisson solver using mov- ing adaptive simplicial tessellation. Journal of Computational Physics321, 644–697 (2016) https://doi.org/10.1016/j.jcp.2016.05.048 arXiv:1509.07720 [physics.comp-ph]
-
[35]
Hahn, O., Angulo, R.E.: An adaptively refined phase-space element method for cosmological simulations and collisionless dynamics. Monthly Notices of the Royal Astronomical Society455(1), 1115–1133 (2016) https://doi.org/10.1093/ mnras/stv2304 arXiv:1501.01959 [astro-ph.CO]
work page Pith review arXiv 2016
-
[36]
Sugiura, H., Nishimichi, T., Rasera, Y., Taruya, A.: Phase-space structure of cold dark matter haloes inside splashback: multistream flows and self-similar solution. Monthly Notices of the Royal Astronomical Society493(2), 2765–2781 (2020) https://doi.org/10.1093/mnras/staa413 arXiv:1911.05394 [astro-ph.CO]
-
[37]
Colombi, S.: Phase-space structure of protohalos: Vlasov versus particle-mesh. Astronomy & Astrophysics647, 66 (2021) https://doi.org/10.1051/0004-6361/ 202039719 arXiv:2012.04409 [astro-ph.CO]
-
[38]
Ondaro-Mallea, L., Angulo, R.E., St¨ ucker, J., Hahn, O., White, S.D.M.: Phase- space simulations of prompt cusps: simulating the formation of the first haloes without artificial fragmentation. Monthly Notices of the Royal Astronomical Society527(4), 10802–10821 (2024) https://doi.org/10.1093/mnras/stad3949 arXiv:2309.05707 [astro-ph.GA]
-
[39]
Astronomy & Astrophysics5, 84–89 (1970)
Zel’dovich, Y.B.: Gravitational instability: An approximate theory for large density perturbations. Astronomy & Astrophysics5, 84–89 (1970)
1970
-
[40]
MNRAS267, 811 (1994) https://doi.org/10.1093/mnras/267.4.811 arXiv:astro- ph/9309055 [astro-ph]
Buchert, T.: Lagrangian Theory of Gravitational Instability of Friedman- Lemaitre Cosmologies - a Generic Third-Order Model for Nonlinear Clustering. MNRAS267, 811 (1994) https://doi.org/10.1093/mnras/267.4.811 arXiv:astro- ph/9309055 [astro-ph]
-
[41]
Bouchet, F.R., Colombi, S., Hivon, E., Juszkiewicz, R.: Perturbative Lagrangian approach to gravitational instability. Astronomy & Astrophysics 34 296, 575 (1995) https://doi.org/10.48550/arXiv.astro-ph/9406013 arXiv:astro- ph/9406013 [astro-ph]
-
[42]
Catelan, P.: Lagrangian dynamics in non-flat universes and non-linear grav- itational evolution. MNRAS276(1), 115–124 (1995) https://doi.org/10.1093/ mnras/276.1.115 arXiv:astro-ph/9406016 [astro-ph]
-
[43]
Nature380(6575), 603–606 (1996) https://doi.org/10.1038/ 380603a0
Bond, J.R., Kofman, L., Pogosyan, D.: How filaments of galaxies are woven into the cosmic web. Nature380(6575), 603–606 (1996) https://doi.org/10.1038/ 380603a0
1996
-
[44]
Monaco, P., Efstathiou, G.: Reconstruction of cosmological initial conditions from galaxy redshift catalogues. MNRAS308, 763–779 (1999) https://doi.org/ 10.1046/j.1365-8711.1999.02747.x astro-ph/9902119
-
[45]
Ram Pressure Stripping of Disc Galaxies: The Role of the Inclination Angle , shorttitle =
Hahn, O., Porciani, C., Carollo, C.M., Dekel, A.: Properties of dark matter haloes in clusters, filaments, sheets and voids. MNRAS375(2), 489–499 (2007) https://doi.org/10.1111/j.1365-2966.2006.11318.x arXiv:astro- ph/0610280 [astro-ph]
-
[46]
Cognitive Science36(5), 757–798 (2012).https://doi.org/10.1111/j
Forero–Romero, J.E., Hoffman, Y., Gottl¨ ober, S., Klypin, A., Yepes, G.: A dynamical classification of the cosmic web. MNRAS396(3), 1815–1824 (2009) https://doi.org/10.1111/j. 1365-2966.2009.14885.x https://academic.oup.com/mnras/article- pdf/396/3/1815/5804803/mnras0396-1815.pdf
work page doi:10.1111/j 2009
-
[47]
H., Staveley-Smith, L., Campbell, L., Parker, Q., Saunders, W., & Watson, F
Kitaura, F.-S., Angulo, R.E.: Linearization with cosmological perturbation the- ory. MNRAS425(4), 2443–2454 (2012) https://doi.org/10.1111/j.1365-2966. 2012.21614.x arXiv:1111.6617 [astro-ph.CO]
-
[48]
Kitaura, F.-S., Sinigaglia, F.: Spectral Hierarchy of the Cosmic Web. arXiv e-prints, 2603–15834 (2026) https://doi.org/10.48550/arXiv.2603.15834 arXiv:2603.15834 [astro-ph.CO]
-
[49]
doi:10.1103/physrev.106.620 , url =
Jaynes, E.T.: Information Theory and Statistical Mechanics. Physical Review 106(4), 620–630 (1957) https://doi.org/10.1103/PhysRev.106.620
-
[50]
Jaynes, E.T.: Information Theory and Statistical Mechanics. II. Physical Review 108(2), 171–190 (1957) https://doi.org/10.1103/PhysRev.108.171
-
[51]
Wiley, ??? (2012)
Cover, T.M., Thomas, J.A.: Elements of Information Theory. Wiley, ??? (2012). https://books.google.es/books?id=VWq5GG6ycxMC
2012
-
[52]
Cambridge University Press, Cam- bridge (2007)
Kardar, M.: Statistical Physics of Particles. Cambridge University Press, Cam- bridge (2007)
2007
-
[53]
Oxford University 35 Press, Oxford (1987)
Chandler, D.: Introduction to Modern Statistical Mechanics. Oxford University 35 Press, Oxford (1987)
1987
-
[54]
Bell System Tech- nical Journal27(3), 379–423 (1948) https://doi.org/10.1002/j.1538-7305
Shannon, C.E.: A mathematical theory of communication. Bell System Tech- nical Journal27(3), 379–423 (1948) https://doi.org/10.1002/j.1538-7305. 1948.tb01338.x https://onlinelibrary.wiley.com/doi/pdf/10.1002/j.1538- 7305.1948.tb01338.x
-
[55]
Pergamon, Oxford (1965)
Landau, L.D.: Collected Papers of LD Landau. Pergamon, Oxford (1965)
1965
-
[56]
Wagner, D., Wohlfarth, E.P.: Theory and applications of the landau-ginzburg theory of amorphous ferromagnetism. Journal of Magnetism and Magnetic Mate- rials15-18, 1345–1346 (1980) https://doi.org/10.1016/0304-8853(80)90315-7
-
[57]
Physica D: Non- linear Phenomena39(1), 59–76 (1989) https://doi.org/10.1016/0167-2789(89) 90039-0
Sprekels, J., Zheng, S.: Global solutions to the equations of a ginzburg-landau theory for structural phase transitions in shape memory alloys. Physica D: Non- linear Phenomena39(1), 59–76 (1989) https://doi.org/10.1016/0167-2789(89) 90039-0
-
[58]
Iida, K., Baym, G.: The Superfluid phases of quark matter: Ginzburg-Landau theory and color neutrality. Phys. Rev. D63, 074018 (2001) https://doi.org/ 10.1103/PhysRevD.63.074018 arXiv:hep-ph/0011229. [Erratum: Phys.Rev.D 66, 059903 (2002)]
-
[59]
Schofield, S.A., Oxtoby, D.W.: Diffusion disallowed crystal growth. I. Landau- Ginzburg model. The Journal of Chemical Physics94(3), 2176–2186 (1991) https://doi.org/10.1063/1.459889
-
[60]
The Journal of Chemical Physics100(3), 2139–2148 (1994) https://doi.org/10.1063/ 1.466510
Bagdassarian, C.K., Oxtoby, D.W.: Crystal nucleation and growth from the undercooled liquid: A nonclassical piecewise parabolic free-energy model. The Journal of Chemical Physics100(3), 2139–2148 (1994) https://doi.org/10.1063/ 1.466510
1994
-
[61]
Physical Review Letters57(14), 1733–1736 (1986) https://doi.org/10.1103/PhysRevLett.57.1733
Aastuen, D.J.W., Clark, N.A., Cotter, L.K., Ackerson, B.J.: Nucleation and growth of colloidal crystals. Physical Review Letters57(14), 1733–1736 (1986) https://doi.org/10.1103/PhysRevLett.57.1733
-
[62]
Williams, J.J., Nicolaou, Z.G., Kutz, J.N., Brunton, S.L.: Data-driven discovery of a new Ginzburg-Landau reduced-order model for vortex shedding. Phys- ical Review Fluids11(3), 034401 (2026) https://doi.org/10.1103/169b-7qpd arXiv:2411.08277 [physics.flu-dyn]
-
[63]
Bernardeau, F., Colombi, S., Gazta˜ naga, E., Scoccimarro, R.: Large-scale struc- ture of the universe and cosmological perturbation theory. Physics Reports 367(1-3), 1–248 (2002) https://doi.org/10.1016/s0370-1573(02)00135-7
-
[64]
Princeton University Press, Princeton (1980) 36
Peebles, P.J.E.: The Large-scale Structure of the Universe. Princeton University Press, Princeton (1980) 36
1980
-
[65]
LRCA8(1), 1 (2022) https://doi.org/10.1007/s41115-021-00013-z arXiv:2112.05165 [astro- ph.CO]
Angulo, R.E., Hahn, O.: Large-scale dark matter simulations. LRCA8(1), 1 (2022) https://doi.org/10.1007/s41115-021-00013-z arXiv:2112.05165 [astro- ph.CO]
-
[66]
Mo, H., Van den Bosch, F.C., White, S.: Galaxy Formation and Evolution, (2010)
2010
-
[67]
Shandarin, S.F.: The multi-stream flows and the dynamics of the cosmic web. Journal of Cosmology and Astroparticle Physics2011(5), 015 (2011) https:// doi.org/10.1088/1475-7516/2011/05/015 arXiv:1011.1924 [astro-ph.CO]
-
[68]
Journal of Statistical Physics 77(1-2), 217–221 (1994) https://doi.org/10.1007/BF02186840
Penrose, R.: On the second law of thermodynamics. Journal of Statistical Physics 77(1-2), 217–221 (1994) https://doi.org/10.1007/BF02186840
-
[69]
Vopson, M.M.: Is gravity evidence of a computational universe? AIP Advances 15(4), 045035 (2025) https://doi.org/10.1063/5.0264945
-
[70]
Abel, T., Hahn, O., Kaehler, R.: Tracing the dark matter sheet in phase space. MNRAS427, 61–76 (2012) https://doi.org/10.1111/j.1365-2966.2012.21754.x arXiv:1111.3944
-
[71]
MNRAS437(4), 3442–3472 (2014) https://doi.org/10.1093/mnras/stt2142 arXiv:1311.7134 [astro-ph.CO]
Hidding, J., Shandarin, S.F., Van de Weygaert, R.: The Zel’dovich approxima- tion: key to understanding cosmic web complexity. MNRAS437(4), 3442–3472 (2014) https://doi.org/10.1093/mnras/stt2142 arXiv:1311.7134 [astro-ph.CO]
-
[72]
General properties
Arnold, V.I., Shandarin, S.F., Zeldovich, I.B.: The large scale structure of the universe I. General properties. One-and two-dimensional models. Geophysical and Astrophysical Fluid Dynamics20(1), 111–130 (1982) https://doi.org/10. 1080/03091928208209001
1982
-
[73]
Astrophysical Journal Letters344, 53 (1989) https://doi.org/10.1086/185529
Peebles, P.J.E.: Tracing Galaxy Orbits Back in Time. Astrophysical Journal Letters344, 53 (1989) https://doi.org/10.1086/185529
-
[74]
Nusser, A., Branchini, E.: On the least action principle in cosmology. MNRAS313(3), 587–595 (2000) https://doi.org/10.1046/j.1365-8711.2000. 03261.x arXiv:astro-ph/9908167 [astro-ph]
-
[75]
MNRAS293(1), 89–106 (1998) https://doi.org/10.1046/j
Branchini, E., Eldar, A., Nusser, A.: Peculiar velocity reconstruction with the fast action method: tests on mock redshift surveys. Monthly Notices of the Royal Astronomical Society335(1), 53–72 (2002) https://doi.org/10.1046/j. 1365-8711.2002.05611.x arXiv:astro-ph/0110618 [astro-ph]
work page doi:10.1046/j 2002
-
[76]
Brenier, Y., Frisch, U., H´ enon, M., Loeper, G., Matarrese, S., Mohayaee, R., Sobolevski˘i, A.: Reconstruction of the early Universe as a convex optimiza- tion problem. Monthly Notices of the Royal Astronomical Society346(2), 501–524 (2003) https://doi.org/10.1046/j.1365-2966.2003.07106.x arXiv:astro- ph/0304214 [astro-ph] 37
-
[77]
Mohayaee, R., Frisch, U., Matarrese, S., Sobolevskii, A.: Back to the primordial Universe by a Monge-Amp` ere-Kantorovich optimization scheme. Astronomy & Astrophysics406, 393–401 (2003) https://doi.org/10.1051/0004-6361:20030719 arXiv:astro-ph/0301641 [astro-ph]
-
[78]
The Astrophysical Journal564(1), 8 (2002) https://doi.org/10.1086/ 324182
Monaco, P., Theuns, T., Taffoni, G., Governato, F., Quinn, T., Stadel, J.: Predicting the number, spatial distribution, and merging history of dark mat- ter halos. The Astrophysical Journal564(1), 8 (2002) https://doi.org/10.1086/ 324182
2002
-
[79]
Kitaura, F.-S., Sinigaglia, F.: Ridged Lagrangian Perturbation Theory (RLPT). arXiv e-prints, 2603–13106 (2026) https://doi.org/10.48550/arXiv.2603.13106 arXiv:2603.13106 [astro-ph.CO]
-
[80]
Kitaura, F.-S., Sinigaglia, F., Balaguera-Antol´ ınez, A., Favole, G.: The cosmic web from perturbation theory. Astronomy & Astrophysics683, 215 (2024) https: //doi.org/10.1051/0004-6361/202345876 arXiv:2301.03648 [astro-ph.CO]
-
[81]
McDonald, P.: How to generate a significant effective temperature for cold dark matter, from first principles. Journal of Cosmology and Astroparticle Physics2011(4), 032 (2011) https://doi.org/10.1088/1475-7516/2011/04/032 arXiv:0910.1002 [astro-ph.CO]
-
[82]
Coarse-Grained Cosmological Perturbation Theory,
Pietroni, M., Mangano, G., Saviano, N., Viel, M.: Coarse-grained cosmological perturbation theory. Journal of Cosmology and Astroparticle Physics2012(1), 019 (2012) https://doi.org/10.1088/1475-7516/2012/01/019 arXiv:1108.5203 [astro-ph.CO]
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.