Reuse & Permissions

It is not necessary to obtain permission to reuse this article or its components as it is available under the terms of the Creative Commons Attribution 4.0 International license. This license permits unrestricted use, distribution, and reproduction in any medium, provided attribution to the author(s) and the published article's title, journal citation, and DOI are maintained. Please note that some figures may have been included with permission from other third parties. It is your responsibility to obtain the proper permission from the rights holder directly for these figures.

Export citation

Export citation

Choose format for download:

Download Citation
  • Open Access

Freezing lakes as analog models of ΛCDM cosmology and beyond

Lorens F. Niehof*,†

Ananya Venkatasubramanian*,‡ and Federico Toschi§

Stefano Liberati∥

  • *These authors contributed equally to this work.
  • †Contact author: l.f.niehof@student.tue.nl
  • ‡Contact author: a.venkatasubramanian@student.tue.nl
  • §Contact author: f.toschi@tue.nl
  • ∥Contact author: liberati@sissa.it

Phys. Rev. D 113, 123523 – Published 11 June, 2026

DOI: https://doi.org/10.1103/cw4j-q9ch

Abstract

We extend previous conduction-based analogies between ice growth in a lake and cosmological expansion by incorporating buoyancy-driven heat transport. Reformulating the Stefan problem with both conductive and convective fluxes yields an evolution equation for the ice thickness s(t) that is structurally analogous to the Friedmann equations for the cosmological scale factor a(t). Beyond reproducing radiation-, matter-, and curvaturelike behaviors, we introduce a reduced description of convection in which the vertically integrated heat flux reaching the moving ice-water interface is modeled as a power-law function of the instantaneous liquid-layer thickness, generating two additional effective contributions. The first is a constant term, directly analogous to a cosmological constant, arising from the persistence of buoyancy-driven transport under geometric confinement. The second is an s−1 contribution originating from the coupling between the moving ice boundary and the convective boundary layer. This term reflects the specific reduced flux-height ansatz adopted, rather than a universal physical prediction. When expressed in Friedmann-like cosmological form, this term entails a fluid with negative energy density and equation-of-state parameter w=−2/3. In cosmology this term may be an effective one associated to a network of domain walls made of exotic energy/matter, but it might also arise from an energy exchange between cosmological components. Overall, the results should be interpreted as a structural analogy between evolution equations, showing how nonlinear transport mechanisms in a classical moving-boundary problem can reproduce the hierarchy of scaling terms familiar from cosmology within a reduced and analytically tractable framework.

View figure in article

Physics Subject Headings (PhySH)

Article Text

References (52)

  1. C. Barceló, S. Liberati, and M. Visser, Int. J. Mod. Phys. D 12, 1641 (2003).
  2. C. Barceló, S. Liberati, and M. Visser, Living Rev. Relativity 14, 3 (2011).
  3. G. E. Volovik, The Universe in a Helium Droplet (Clarendon Press, Oxford, 2003).
  4. V. Faraoni, Cosmic Analogies: How Natural Systems Emulate the Universe (World Scientific, Singapore, 2024).
  5. M. Vollmer, Eur. J. Phys. 40, 035101 (2019).
  6. V. Faraoni, Phys. Rev. Res. 1, 013187 (2020).
  7. S. Weinberg, Gravitation and Cosmology (Wiley, New York, 1972).
  8. P. J. E. Peebles, Principles of Physical Cosmology (Princeton University Press, Princeton, NJ, 1993).
  9. V. Mukhanov, Physical Foundations of Cosmology (Cambridge University Press, Cambridge, England, 2005).
  10. S. Dodelson and F. Schmidt, Modern Cosmology, 2nd ed. (Academic Press, New York, 2020).
  11. Planck Collaboration, Astron. Astrophys. 641, A6 (2020).
  12. J. Stefan, Sitzungsber. Kais. Akad. Wiss. Math.-Naturwiss. Cl. 98, 965 (1889).
  13. H. S. Carslaw and J. C. Jaeger, Conduction of Heat in Solids, 2nd ed. (Oxford University Press, New York, 1959).
  14. V. Alexiades and A. D. Solomon, Mathematical Modeling of Melting and Freezing Processes (Hemisphere, Washington, 1993).
  15. V. Faraoni, Eur. Phys. J. C 80, 445 (2020).
  16. A. Friedmann, Z. Phys. 10, 377 (1922).
  17. H. P. Robertson, Astrophys. J. 82, 284 (1935).
  18. A. G. Walker, Proc. London Math. Soc. 42, 90 (1936).
  19. R. Hagedorn, Nuovo Cimento Suppl. 3, 147 (1965).
  20. R. Brandenberger and C. Vafa, Nucl. Phys. B316 (1989).
  21. R. Brandenberger, String Gas Cosmology (Cambridge University Press, Cambridge, England, 2008).
  22. T. Padmanabhan, Int. J. Mod. Phys. D 17, 367 (2008).
  23. E. P. Verlinde, J. High Energy Phys. 04 (2011) 029.
  24. S. Gielen, D. Oriti, and L. Sindoni, Phys. Rev. Lett. 111, 031301 (2013).
  25. S. Gielen, D. Oriti, and L. Sindoni, J. High Energy Phys. 06 (2014) 013.
  26. C. Doering and P. Constantin, Phys. Rev. E 53, 5957 (1996).
  27. A. Vilenkin and E. P. S. Shellard, Cosmic Strings and Other Topological Defects (Cambridge University Press, Cambridge, England, 1994).
  28. S. C. Jaryal and A. Chatterjee, Eur. Phys. J. C 81, 273 (2021).
  29. Y. B. Zel’dovich, I. Y. Kobzarev, and L. B. Okun, Zh. Eksp. Teor. Fiz. 67, 3 (1974) [Sov. Phys. JETP 40, 1 (1975)].
  30. T. W. B. Kibble, J. Phys. A 9, 1387 (1976).
  31. A. Vilenkin, Phys. Rev. D 23, 852 (1981).
  32. A. Vilenkin, Phys. Rep. 121, 263 (1985).
  33. T. Tanaka and M. Sasaki, Phys. Rev. D 59, 023506 (1999).
  34. W. H. Press, B. S. Ryden, and D. N. Spergel, Astrophys. J. 347, 590 (1989).
  35. S. E. Larsson, S. Sarkar, and P. L. White, Phys. Rev. D 55, 5129 (1997).
  36. L. Sousa and P. P. Avelino, Phys. Rev. D 92, 083520 (2015).
  37. L. Sousa, P. P. Avelino, and G. S. F. Guedes, Phys. Rev. D 101, 103508 (2020).
  38. L. Caloni et al., arXiv:2602.20050.
  39. M. Bucher, K. Moodley, and N. Turok, Phys. Rev. D 62, 083508 (2000).
  40. P. P. Avelino, C. J. A. P. Martins, and J. C. R. E. Oliveira, Phys. Rev. D 72, 083506 (2005).
  41. M. Eto, T. Fujimori, T. Nagashima, M. Nitta, K. Ohashi, and N. Sakai, Phys. Rev. D 76, 125025 (2007).
  42. L. Sousa and P. P. Avelino, Phys. Rev. D 94, 063529 (2016).
  43. C. Barcelo, JETP Lett. 84, 635 (2007).
  44. M. A. van der Westhuizen and A. Abebe, J. Cosmol. Astropart. Phys. 01 (2024) 048.
  45. J. S. Wettlaufer, J. Geophys. Res. 96, 7215 (1991).
  46. A. H. Harvey, in CRC Handbook of Chemistry and Physics, 97th ed., edited by W. M. Haynes, D. R. Lide, and T. J. Bruno (CRC Press, Boca Raton, FL, 2017).
  47. W. M. J. Lazeroms, A. Jenkins, G. H. Gudmundsson, and R. S. W. van de Wal, Cryosphere 12, 49 (2018).
  48. K. F. Voitkovskii, The Mechanical Properties of Ice (Defense Technical Information Center, Washington, DC, 1960); Translation of: Mekhanicheskie svoistva l’da, Academy of Sciences (USSR).
  49. M. L. Huber, R. A. Perkins, D. G. Friend, J. V. Sengers, M. J. Assael, I. N. Metaxa, K. Miyagawa, R. Hellmann, and E. Vogel, J. Phys. Chem. Ref. Data 41, 033102 (2012).
  50. CRC Handbook of Chemistry and Physics, 99th ed. (Internet Version 2018), edited by J. R. Rumble (CRC Press/Taylor & Francis, Boca Raton, FL, 2018).
  51. J. Blumm and A. Lindemann, High Temp. High Press. 35/36, 627 (2007).
  52. M. Escudier and T. Atkins, A Dictionary of Mechanical Engineering, 2nd ed. (Oxford University Press, Oxford, UK, 2019), current Online Version: 2019.

Outline

Information

Sign In to Your Journals Account

Filter

Filter

Article Lookup

Enter a citation