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arxiv: 2604.17383 · v1 · submitted 2026-04-19 · ✦ hep-ph · astro-ph.CO· hep-th

Recognition: unknown

Hydrodynamics of Filtered Dark Matter: A Two-Component Approach

Juntaro Wada

Authors on Pith no claims yet

Pith reviewed 2026-05-10 05:47 UTC · model grok-4.3

classification ✦ hep-ph astro-ph.COhep-th
keywords filtered dark matterfirst-order phase transitionhydrodynamicstwo-component fluidrelic abundanceballistic regimelocal thermal equilibriumdeflagration
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The pith

Modeling Filtered Dark Matter and radiation as separate fluids produces distinct hydrodynamic solutions with a shifted relic abundance.

A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.

The paper sets up the hydrodynamics of Filtered Dark Matter during a first-order phase transition as a two-component fluid because the bubble wall reflects dark matter particles while letting radiation pass through. In the ballistic regime the excluded dark matter energy-momentum forms a reflected mode, whereas in local thermal equilibrium it merges into the radiation fluid. This difference in how the excluded component is handled produces independent evolution for the dark matter and radiation fluids and changes the conditions under which deflagration-like solutions can exist. The resulting hydrodynamic effects alter the final relic abundance of dark matter compared with calculations that ignore the two-fluid distinction.

Core claim

The difference in the fate of the DM fluid that cannot enter the interior of the wall leads to different hydrodynamic behaviors in the DM and radiation fluids independently and, in particular, results in different existence conditions for solutions in the deflagration-like branch. Based on these results, the impact of hydrodynamic effects on the relic abundance of Filtered DM is revisited and a change in the abundance induced by hydrodynamic effects is demonstrated.

What carries the argument

Two-component fluid equations for dark matter and radiation with a reflective boundary condition applied only to the dark matter component.

If this is right

  • Solutions fall into detonation-like and deflagration-like branches in both the ballistic regime and the local thermal equilibrium regime.
  • Existence conditions for deflagration-like solutions differ between the two regimes because of how excluded dark matter energy-momentum is treated.
  • Hydrodynamic effects produce a measurable shift in the calculated relic abundance of Filtered Dark Matter.
  • The entropy current is not conserved in the two-fluid description.

Where Pith is reading between the lines

These are editorial extensions of the paper, not claims the author makes directly.

  • The non-conservation of entropy in the two-fluid system may require revised entropy accounting when computing gravitational-wave signals from the same phase transition.
  • The approach could be applied to other dark-sector models in which only a subset of particles interacts strongly with the bubble wall.
  • Changes in relic abundance from these hydrodynamic effects would tighten or relax existing cosmological bounds on the Filtered Dark Matter parameter space.

Load-bearing premise

The bubble wall is highly reflective of the dark matter fluid but transparent to radiation.

What would settle it

Numerical integration of the two-fluid hydrodynamic equations that either confirms or rules out the predicted difference in deflagration-like solution existence between the ballistic and local thermal equilibrium regimes.

Figures

Figures reproduced from arXiv: 2604.17383 by Juntaro Wada.

Figure 1
Figure 1. Figure 1: FIG. 1. Basic concept of the filtered dark matter scenario. [PITH_FULL_IMAGE:figures/full_fig_p002_1.png] view at source ↗
Figure 2
Figure 2. Figure 2: FIG. 2. Schematic illustration of the variables: the temper [PITH_FULL_IMAGE:figures/full_fig_p007_2.png] view at source ↗
Figure 3
Figure 3. Figure 3: FIG. 3. Velocity dependence of the coefficient characterizing [PITH_FULL_IMAGE:figures/full_fig_p008_3.png] view at source ↗
Figure 4
Figure 4. Figure 4: FIG. 4. The relation between the DM fluid velocities inside and outside the wall obtained from the matching conditions. The [PITH_FULL_IMAGE:figures/full_fig_p010_4.png] view at source ↗
Figure 5
Figure 5. Figure 5: FIG. 5. The impact of hydrodynamics on the DM abundance [PITH_FULL_IMAGE:figures/full_fig_p015_5.png] view at source ↗
Figure 6
Figure 6. Figure 6: FIG. 6. The relation between the DM fluid velocities inside and outside the wall obtained from the matching conditions [PITH_FULL_IMAGE:figures/full_fig_p019_6.png] view at source ↗
read the original abstract

We study the hydrodynamics of the Filtered Dark Matter (Filtered DM) scenario during a first-order phase transition (FOPT). In this scenario, the bubble wall is highly reflective of the dark matter (DM) fluid but transparent to radiation, making the hydrodynamic problem fundamentally different from that of the electroweak FOPT. Motivated by this property, we formulate the hydrodynamics of this system as a two-component fluid composed of DM and radiation, and find that the solutions can be classified into detonation-like and deflagration-like branches in the ballistic regime and in the local thermal equilibrium (LTE) regime. In the ballistic regime, the energy--momentum of DM that cannot enter the wall appears as a reflected mode, while in the LTE regime, it relaxes into the energy--momentum of radiation. We find that this difference in the fate of the DM fluid that cannot enter the interior of the wall leads to different hydrodynamic behaviors in the DM and radiation fluids independently and, in particular, results in different existence conditions for solutions in the deflagration-like branch. Based on these results, we further revisit the impact of hydrodynamic effects on the relic abundance of Filtered DM and demonstrate the change in the abundance induced by hydrodynamic effects. In addition, we also discuss the non-conservation of the entropy current from the viewpoint of the two-fluid system, and briefly comment on the similarity between the Filtered DM system and information-thermodynamic systems.

Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, simulated authors' rebuttal, and a circularity audit. Tearing a paper down is the easy half of reading it; the pith above is the substance, this is the friction.

Referee Report

0 major / 3 minor

Summary. The paper develops a two-component hydrodynamic description (DM plus radiation) for the Filtered Dark Matter scenario during a first-order phase transition. Because the bubble wall is taken to be reflective for DM but transparent to radiation, the system is treated separately in the ballistic regime (where reflected DM appears as a distinct mode) and the local thermal equilibrium regime (where reflected DM relaxes into the radiation fluid). Solutions are classified into detonation-like and deflagration-like branches; the different fate of the excluded DM fluid is shown to produce distinct hydrodynamic profiles and, in particular, different existence conditions for the deflagration-like branch. The work then re-examines the effect of these hydrodynamics on the DM relic abundance and comments on the non-conservation of the entropy current together with an analogy to information-thermodynamic systems.

Significance. If the derivations hold, the manuscript supplies a tailored hydrodynamic framework that captures the distinctive wall-interaction properties of Filtered DM, thereby refining relic-density predictions in this class of models. The explicit separation of ballistic and LTE regimes and the resulting shift in deflagration existence conditions constitute a concrete, falsifiable advance over single-fluid treatments of electroweak-scale transitions.

minor comments (3)
  1. [Introduction / §2] The abstract and introduction introduce the two-component classification but do not state the explicit matching conditions (velocity and energy-momentum continuity) used at the wall; adding a short paragraph or equation block early in the text would clarify the setup for readers.
  2. [Relic abundance section] In the relic-abundance discussion, the quantitative shift induced by the hydrodynamic treatment is described qualitatively; a brief table or plot comparing the new abundance to the standard (no-hydro) result would strengthen the claim.
  3. [Final discussion] The analogy to information-thermodynamic systems is mentioned only in passing; a single sentence linking the non-conservation of the entropy current to a specific information-theoretic quantity would make the parallel more concrete.

Simulated Author's Rebuttal

0 responses · 0 unresolved

We thank the referee for the positive assessment of our work on the two-component hydrodynamics of Filtered Dark Matter and for recommending minor revision. The summary accurately captures the distinction between ballistic and LTE regimes and the resulting impact on deflagration-like solutions and relic abundance. No major comments requiring point-by-point rebuttal were raised.

Circularity Check

0 steps flagged

No significant circularity; derivation applies standard hydrodynamics to stated two-fluid setup

full rationale

The paper's core steps consist of (1) adopting the given physical distinction that the bubble wall reflects DM but transmits radiation, (2) writing the two-component hydrodynamic equations for DM and radiation fluids separately in the ballistic and LTE regimes, and (3) classifying solutions into detonation-like and deflagration-like branches while noting the different fate of reflected DM energy-momentum. These steps follow directly from the stated boundary conditions and standard conservation laws; no equation is defined in terms of its own output, no fitted parameter is relabeled as a prediction, and no load-bearing premise rests on a self-citation chain. The subsequent relic-abundance discussion and entropy-current remark are presented as consequences of the same hydrodynamic classification rather than inputs. The derivation therefore remains self-contained against external hydrodynamic principles.

Axiom & Free-Parameter Ledger

0 free parameters · 2 axioms · 0 invented entities

The central claim rests on standard multi-fluid relativistic hydrodynamics plus the domain-specific assumption of differential wall reflectivity. No free parameters, invented entities, or additional axioms are identifiable from the abstract alone.

axioms (2)
  • standard math Relativistic hydrodynamic equations govern the two-component (DM + radiation) fluid
    Invoked to classify detonation-like and deflagration-like solutions in ballistic and LTE regimes.
  • domain assumption Bubble wall is highly reflective to DM fluid but transparent to radiation
    This property is stated as the motivation for the two-component formulation and the difference from electroweak FOPT.

pith-pipeline@v0.9.0 · 5556 in / 1273 out tokens · 60220 ms · 2026-05-10T05:47:11.210569+00:00 · methodology

discussion (0)

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Reference graph

Works this paper leans on

81 extracted references · 44 canonical work pages

  1. [1]

    Solution in Ballistic Regime The equations to be solved, Eqs. (49) and (50), can be rewritten as ˜ωout χ,f(γout χ,f)2vout χ,f −ω in χ,f(γin χ,f)2vin χ,f = 0 (61) ˜ωout χ,f(γout χ,f)2(vout χ,f)2 −ω in χ,f(γin χ,f)2(vin χ,f)2 =p in χ,f −˜pout χ,f + ∆ϵeff,r χ ,(62) where we have introduced the following parameters: ˜ωout χ,f = ˜ρout χ,f + ˜pout χ,f ,(63) ˜ρo...

  2. [2]

    The former corresponds to a regime in which reflection is efficient,r≃1, so that only a small fraction of DM penetrates into the wall; this provides a good approximation whenv out χ,f ≪1 (see also Fig. 3). In contrast, the latter requires that a sufficient amount of DM enters the wall, which is realized only when the re- flection is suppressed,r≃0, corres...

  3. [3]

    In the ballistic regime, as already studied in the literature [29, 30, 47], the reflected component provides an important contribution to the friction

    Friction in Ballistic Regime In determining the wall velocity, an important condi- tion is the balance between the driving force, given by the difference in the effective potential across the wall, and the backreaction (friction) exerted by the surround- ing fluid. In the ballistic regime, as already studied in the literature [29, 30, 47], the reflected c...

  4. [4]

    G(vout χ,f ,˜αt χ,¯θ) ± q G(vout χ,f ,˜αt χ,¯θ)2 −4(v out χ,f)2(cinχ )2 # ,(119) vin rad = 1 2vout rad

    Solution in LTE Regime The set of equations to be solved, Eqs. (90)-(93), can be rewritten as follows: ¯ωout χ,f(γout χ,f)2vout χ,f −ω in χ,f(γin χ,f)2vin χ,f = 0,(103) ¯ωout χ,f(γout χ,f)2(vout χ,f)2 −ω in χ,f(γin χ,f)2(vin χ,f)2 =p in χ,f −¯pout χ,f + ∆ϵeff,t χ,f ,(104) ¯ωout rad(γout rad)2vout rad −ω in rad(γin rad)2vin rad = 0,(105) ¯ωout rad(γout rad...

  5. [5]

    In the LTE regime, reflection can be neglected, and thus the friction is determined by the change in momen- tum as the fluid crosses the wall [37–39]

    Friction in LTE Regime Following the ballistic regime, we examine the balance between the back reaction (friction) from the fluid and the driving force, which is crucial for determining the terminal wall velocity. In the LTE regime, reflection can be neglected, and thus the friction is determined by the change in momen- tum as the fluid crosses the wall [...

  6. [6]

    mea- sures

    Negative entropy production Finally, we comment on an interesting property related to entropy production that emerges from the analysis of two-component hydrodynamics in the LTE regime. As stated in Eq. (44) in the previous section, even in the LTE regime, once energy transfer is taken into account, the entropy current is not conserved for each component,...

  7. [7]

    Witten,Cosmic Separation of Phases, Phys

    E. Witten,Cosmic Separation of Phases, Phys. Rev. D 30(1984) 272–285. 12 In models where the sound speed inside the wall is strictly con- stant (the so-called template model orνmodel) [32–34], this parameter is related to the dimensionless latent heatα out = 3∆ϵ/4ωout as α¯θ = 1 12(cins )2 h (3cin s )2 −1 + 3αout 1 + (cin s )2 i .(B21)

  8. [8]

    C. J. Hogan,Gravitational radiation from cosmological phase transitions, Mon. Not. Roy. Astron. Soc.218 (1986) 629–636

  9. [9]

    M. S. Turner and F. Wilczek,Relic gravitational waves and extended inflation, Phys. Rev. Lett.65(1990) 3080–3083

  10. [10]

    Kosowsky and M.S

    A. Kosowsky and M. S. Turner,Gravitational radiation from colliding vacuum bubbles: envelope approximation to many bubble collisions, Phys. Rev. D47(1993) 4372–4391[astro-ph/9211004]

  11. [11]

    Kosowsky, M

    A. Kosowsky, M. S. Turner, and R. Watkins, Gravitational waves from first order cosmological phase 19 0.0 0.2 0.4 0.6 0.8 1.0 0.0 0.2 0.4 0.6 0.8 1.0 vin vout detonation branch αθ _=0 αθ _=0.001 αθ _=0.01 αθ _=1 deflagration branch αθ _=0 αθ _=0.001 αθ _=0.01 (left) Non-relativistic sound speedc in χ = q T out χ,f /minχ with the benchmark choicem in χ /T ...

  12. [12]

    Kamionkowski, A

    M. Kamionkowski, A. Kosowsky, and M. S. Turner, Gravitational radiation from first order phase transitions, Phys. Rev. D49(1994) 2837–2851 [astro-ph/9310044]

  13. [13]

    V. A. Kuzmin, V. A. Rubakov, and M. E. Shaposhnikov,On the Anomalous Electroweak Baryon Number Nonconservation in the Early Universe, Phys. Lett. B155(1985) 36

  14. [14]

    A. G. Cohen, D. B. Kaplan, and A. E. Nelson,Progress in electroweak baryogenesis, Ann. Rev. Nucl. Part. Sci. 43(1993) 27–70[hep-ph/9302210]

  15. [15]

    V. A. Rubakov and M. E. Shaposhnikov,Electroweak baryon number nonconservation in the early universe and in high-energy collisions, Usp. Fiz. Nauk166 (1996) 493–537[hep-ph/9603208]

  16. [16]

    Falkowski and J.M

    A. Falkowski and J. M. No,Non-thermal Dark Matter Production from the Electroweak Phase Transition: Multi-TeV WIMPs and ’Baby-Zillas’, JHEP02(2013) 034[arXiv:1211.5615]

  17. [17]

    Super-cool Dark Matter,

    T. Hambye, A. Strumia, and D. Teresi,Super-cool Dark Matter, JHEP08(2018) 188[arXiv:1805.01473]

  18. [18]

    M. J. Baker, J. Kopp, and A. J. Long,Filtered Dark Matter at a First Order Phase Transition, Phys. Rev. Lett.125(2020) 151102[arXiv:1912.02830]

  19. [19]

    Chway, T.H

    D. Chway, T. H. Jung, and C. S. Shin,Dark matter filtering-out effect during a first-order phase transition, Phys. Rev. D101(2020) 095019[arXiv:1912.04238]

  20. [20]

    Azatov, M

    A. Azatov, M. Vanvlasselaer, and W. Yin,Dark Matter production from relativistic bubble walls, JHEP03 (2021) 288[arXiv:2101.05721]

  21. [21]

    Azatov, G

    A. Azatov, G. Barni, S. Chakraborty, M. Vanvlasselaer, and W. Yin,Ultra-relativistic bubbles from the simplest Higgs portal and their cosmological consequences, JHEP 10(2022) 017[arXiv:2207.02230]

  22. [22]

    Jiang, F.P

    S. Jiang, F. P. Huang, and C. S. Li,Hydrodynamic effects on the filtered dark matter produced by a first-order phase transition, Phys. Rev. D108(2023) 063508[arXiv:2305.02218]

  23. [23]

    Chao, X.-F

    W. Chao, X.-F. Li, and L. Wang,Filtered pseudo-scalar dark matter and gravitational waves from first order phase transition, JCAP06(2021) 038 [arXiv:2012.15113]

  24. [24]

    Ahmadvand,Filtered asymmetric dark matter during the Peccei-Quinn phase transition, JHEP10 (2021) 109[arXiv:2108.00958]

    M. Ahmadvand,Filtered asymmetric dark matter during the Peccei-Quinn phase transition, JHEP10 (2021) 109[arXiv:2108.00958]

  25. [25]

    Hosseini, S

    M. Hosseini, S. Y. Ayazi, and A. Mohamadnejad, Gravitational wave in a filtered vector dark matter model, Phys. Dark Univ.48(2025) 101952 [arXiv:2405.10662]

  26. [26]

    Griest and M

    K. Griest and M. Kamionkowski,Unitarity Limits on the Mass and Radius of Dark Matter Particles, Phys. Rev. Lett.64(1990) 615

  27. [27]

    P. J. Steinhardt,Relativistic Detonation Waves and Bubble Growth in False Vacuum Decay, Phys. Rev. D 25(1982) 2074

  28. [28]

    Kurki-Suonio,Deflagration Bubbles in the Quark - Hadron Phase Transition, Nucl

    H. Kurki-Suonio,Deflagration Bubbles in the Quark - Hadron Phase Transition, Nucl. Phys. B255(1985) 231–252

  29. [29]

    L. D. Landau and E. M. Lifshitz,Fluid Mechanics. Pergamon Press, New York, 1989

  30. [30]

    Laine,Bubble growth as a detonation, Phys

    M. Laine,Bubble growth as a detonation, Phys. Rev. D 49(1994) 3847–3853[hep-ph/9309242]

  31. [31]

    Ignatius, K

    J. Ignatius, K. Kajantie, H. Kurki-Suonio, and M. Laine,The growth of bubbles in cosmological phase transitions, Phys. Rev. D49(1994) 3854–3868 [astro-ph/9309059]

  32. [32]

    Bodeker and G.D

    D. Bodeker and G. D. Moore,Can electroweak bubble walls run away?, JCAP05(2009) 009 [arXiv:0903.4099]. 20

  33. [33]

    Bodeker and G.D

    D. Bodeker and G. D. Moore,Electroweak Bubble Wall Speed Limit, JCAP05(2017) 025[arXiv:1703.08215]

  34. [34]

    H¨ oche, J

    S. H¨ oche, J. Kozaczuk, A. J. Long, J. Turner, and Y. Wang,Towards an all-orders calculation of the electroweak bubble wall velocity, JCAP03(2021) 009 [arXiv:2007.10343]

  35. [35]

    Gouttenoire, R

    Y. Gouttenoire, R. Jinno, and F. Sala,Friction pressure on relativistic bubble walls, JHEP05(2022) 004 [arXiv:2112.07686]

  36. [36]

    W.-Y. Ai, B. Laurent, and J. van de Vis,Bounds on the bubble wall velocity, JHEP02(2025) 119 [arXiv:2411.13641]

  37. [37]

    Krajewski,et al.,Thermalization effects on the dynamics of growing vacuum bubbles, JHEP03(2025) 178[arXiv:2411.15094]

    T. Krajewski,et al.,Thermalization effects on the dynamics of growing vacuum bubbles, JHEP03(2025) 178[arXiv:2411.15094]

  38. [38]

    Leitao and A

    L. Leitao and A. Megevand,Hydrodynamics of phase transition fronts and the speed of sound in the plasma, Nucl. Phys. B891(2015) 159–199[arXiv:1410.3875]

  39. [39]

    Giese, T

    F. Giese, T. Konstandin, and J. van de Vis, Model-independent energy budget of cosmological first-order phase transitions—A sound argument to go beyond the bag model, JCAP07(2020) 057 [arXiv:2004.06995]

  40. [40]

    Giese, T

    F. Giese, T. Konstandin, K. Schmitz, and J. van de Vis, Model-independent energy budget for LISA, JCAP01 (2021) 072[arXiv:2010.09744]

  41. [41]

    W.-Y. Ai, B. Laurent, and J. van de Vis, Model-independent bubble wall velocities in local thermal equilibrium, JCAP07(2023) 002[arXiv:2303.10171]

  42. [42]

    Sanchez-Garitaonandia and J

    M. Sanchez-Garitaonandia and J. van de Vis,Prediction of the bubble wall velocity for a large jump in degrees of freedom, Phys. Rev. D110(2024) 023509 [arXiv:2312.09964]

  43. [43]

    Barroso Mancha, T

    M. Barroso Mancha, T. Prokopec, and B. Swiezewska, Field-theoretic derivation of bubble-wall force, JHEP01 (2021) 070[arXiv:2005.10875]

  44. [44]

    Balaji, M

    S. Balaji, M. Spannowsky, and C. Tamarit, Cosmological bubble friction in local equilibrium, JCAP 03(2021) 051[arXiv:2010.08013]

  45. [45]

    W.-Y. Ai, B. Garbrecht, and C. Tamarit,Bubble wall velocities in local equilibrium, JCAP03(2022) 015 [arXiv:2109.13710]

  46. [46]

    T. C. Gehrman, B. Shams Es Haghi, K. Sinha, and T. Xu,Recycled dark matter, JCAP03(2024) 044 [arXiv:2310.08526]. [41]PlanckCollaboration,Planck 2018 results. VI. Cosmological parameters, Astron. Astrophys.641 (2020) A6[arXiv:1807.06209]. [Erratum: Astron.Astrophys. 652, C4 (2021)]

  47. [47]

    W.-Y. Ai, M. Fairbairn, K. Mimasu, and T. You, Non-thermal production of heavy vector dark matter from relativistic bubble walls, JHEP05(2025) 225 [arXiv:2406.20051]

  48. [48]

    M. J. Ramsey-Musolf and J. Zhu,Bubble wall velocity from Kadanoff-Baym equations: fluid dynamics and microscopic interactions,arXiv:2504.13724(2025)

  49. [49]

    W.-Y. Ai, M. Carosi, B. Garbrecht, C. Tamarit, and M. Vanvlasselaer,Bubble wall dynamics from nonequilibrium quantum field theory, JHEP08(2025) 077[arXiv:2504.13725]

  50. [50]

    G. D. Moore and T. Prokopec,Bubble wall velocity in a first order electroweak phase transition, Phys. Rev. Lett. 75(1995) 777–780[hep-ph/9503296]

  51. [51]

    G. D. Moore and T. Prokopec,How fast can the wall move? A Study of the electroweak phase transition dynamics, Phys. Rev. D52(1995) 7182–7204 [hep-ph/9506475]

  52. [52]

    Garcia Garcia, G

    I. Garcia Garcia, G. Koszegi, and R. Petrossian-Byrne, Reflections on bubble walls, JHEP09(2023) 013 [arXiv:2212.10572]

  53. [53]

    Brillouin,Maxwell’s Demon Cannot Operate: Information and Entropy

    L. Brillouin,Maxwell’s Demon Cannot Operate: Information and Entropy. I, Journal of Applied Physics 22(1951) 334–337

  54. [54]

    C. H. Bennett,The thermodynamics of computation—a review, International Journal of Theoretical Physics21 (1982) 905–940

  55. [55]

    Landauer,Irreversibility and Heat Generation in the Computing Process, IBM Journal of Research and Development5(1961) 183–191

    R. Landauer,Irreversibility and Heat Generation in the Computing Process, IBM Journal of Research and Development5(1961) 183–191

  56. [56]

    The origin of the matter-antimatter asymmetry

    M. Dine and A. Kusenko,The Origin of the matter - antimatter asymmetry, Rev. Mod. Phys.76(2003) 1 [hep-ph/0303065]

  57. [57]

    D. E. Morrissey and M. J. Ramsey-Musolf,Electroweak baryogenesis, New J. Phys.14(2012) 125003 [arXiv:1206.2942]

  58. [58]

    J. C. Maxwell,Theory of Heat. Appleton, London, 1871

  59. [59]

    Shizume,Heat generation required by information erasure, Phys

    K. Shizume,Heat generation required by information erasure, Phys. Rev. E52(1995) 3495–3499

  60. [60]

    Piechocinska,Information erasure, Phys

    B. Piechocinska,Information erasure, Phys. Rev. A61 (2000) 062314

  61. [61]

    Touchette and S

    H. Touchette and S. Lloyd,Information-Theoretic Limits of Control, Phys. Rev. Lett.84(2000) 1156–1159

  62. [62]

    Touchette and S

    H. Touchette and S. Lloyd,Information-theoretic approach to the study of control systems, Physica A: Statistical Mechanics and its Applications331(2004) 140–172

  63. [63]

    M. M. Barkeshli,Dissipationless Information Erasure and Landauer’s Principle, 2005. https://arxiv.org/abs/cond-mat/0504323

  64. [64]

    K. H. Kim and H. Qian,Fluctuation theorems for a molecular refrigerator, Phys. Rev. E75(2007) 022102

  65. [65]

    Sagawa and M

    T. Sagawa and M. Ueda,Second Law of Thermodynamics with Discrete Quantum Feedback Control, Phys. Rev. Lett.100(2008) 080403

  66. [66]

    Dillenschneider and E

    R. Dillenschneider and E. Lutz,Memory Erasure in Small Systems, Phys. Rev. Lett.102(2009) 210601

  67. [67]

    Turgut,Relations between entropies produced in nondeterministic thermodynamic processes, Phys

    S. Turgut,Relations between entropies produced in nondeterministic thermodynamic processes, Phys. Rev. E79(2009) 041102

  68. [68]

    Sagawa and M

    T. Sagawa and M. Ueda,Minimal Energy Cost for Thermodynamic Information Processing: Measurement and Information Erasure, Phys. Rev. Lett.102(2009) 250602

  69. [69]

    J. M. Horowitz and S. Vaikuntanathan,Nonequilibrium detailed fluctuation theorem for repeated discrete feedback, Phys. Rev. E82(2010) 061120

  70. [70]

    Reeb and M

    D. Reeb and M. M. Wolf,An improved Landauer principle with finite-size corrections, New J. Phys.16 (2014) 103011

  71. [71]

    Sagawa,Thermodynamics of Information Processing in Small Systems, Progress of Theoretical Physics127 (2012) 1–56

    T. Sagawa,Thermodynamics of Information Processing in Small Systems, Progress of Theoretical Physics127 (2012) 1–56

  72. [72]

    Sagawa and M

    T. Sagawa and M. Ueda,Nonequilibrium thermodynamics of feedback control, Phys. Rev. E85 (2012) 021104

  73. [73]

    Abreu and U

    D. Abreu and U. Seifert,Thermodynamics of Genuine Nonequilibrium States under Feedback Control, Phys. 21 Rev. Lett.108(2012) 030601

  74. [74]

    Lahiri, S

    S. Lahiri, S. Rana, and A. M. Jayannavar,Fluctuation theorems in the presence of information gain and feedback, Journal of Physics A: Mathematical and Theoretical45(2012) 065002

  75. [75]

    Still, D

    S. Still, D. A. Sivak, A. J. Bell, and G. E. Crooks,The thermodynamics of prediction, Phys. Rev. Lett.109 (2012) 120604[arXiv:1203.3271]

  76. [76]

    Sagawa and M

    T. Sagawa and M. Ueda,Fluctuation Theorem with Information Exchange: Role of Correlations in Stochastic Thermodynamics, Phys. Rev. Lett.109 (2012) 180602

  77. [77]

    Sagawa and M

    T. Sagawa and M. Ueda,Role of mutual information in entropy production under information exchanges, New Journal of Physics15(2013) 125012

  78. [78]

    Sagawa,Thermodynamic and logical reversibilities revisited, Journal of Statistical Mechanics: Theory and Experiment2014(2014) P03025

    T. Sagawa,Thermodynamic and logical reversibilities revisited, Journal of Statistical Mechanics: Theory and Experiment2014(2014) P03025

  79. [79]

    Maruyama, F

    K. Maruyama, F. Nori, and V. Vedral,Colloquium: The physics of Maxwell’s demon and information, Rev. Mod. Phys.81(2009) 1–23[arXiv:0707.3400]

  80. [80]

    M. J. Baker, M. Breitbach, J. Kopp, and L. Mittnacht, Primordial black holes from first-order cosmological phase transitions, Phys. Lett. B868(2025) 139625 [arXiv:2105.07481]

Showing first 80 references.