Pith. sign in

REVIEW 3 major objections 4 minor 65 references

At the Edge of Uncertainty: Decoding the Cosmological Constant value with Bose-Einstein Distribution

T0 review · 3 major / 4 minor · reviewed 2026-08-15 · deepseek-v4-flash

Pith's one-line read The paper claims that the observed cosmological constant is set by a spacetime-metric uncertainty $\Delta g \approx 5\times 10^{-61}$, which cuts off vacuum energy at $L_Z \approx 2.2\times 10^{-5}$ m.

desk verdict The paper's central 'validation' is a tautology: the 2.7e-5 m wavelength is manufactured from the same density that gives L_Z, via an unjustified 1/2 factor. read the letter →

arxiv 2505.11560 v1 pith:WCEKWKIF submitted 2025-05-16 gr-qc

classification gr-qc MSC 83C4583F05 PACS 04.60.-m98.80.-k05.30.Jp
keywords cosmologicalconstantvacuumenergyspacetimeuncertaintyBose-Einsteincondensatedarkmesoscopiccutoffmetricfluctuationquantumgravityphenomenology
open problems Dark Energy
verification ladder T0 review T1 audit T2 compute T3 formal

The pith

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

The reading

This paper tries to turn the cosmological constant problem from a fine-tuning puzzle into a consequence of quantum spacetime fuzz. It argues that quantum uncertainty in particle position, combined with the principle that energy curves spacetime, forces the metric itself to be uncertain to a degree $\Delta g \approx 5\times 10^{-61}$. Using that uncertainty as the cutoff in the vacuum-energy integral yields a length scale $L_Z \approx 2.2\times 10^{-5}$ m, the geometric mean of the Planck length and the radius of the observable universe, and reproduces the observed vacuum density without a Planck-scale cutoff. The paper then models dark energy as a Bose-Einstein condensate of massless bosons, obtaining an effective temperature of about 41 K whose thermal wavelength ($2.7\times 10^{-5}$ m) matches the same cutoff. If right, the large hierarchy between predicted and observed vacuum energy is not an accident but the signature of spacetime indeterminacy at a mesoscopic scale.

What carries the argument

The load-bearing identity is $\Delta g = \ell_{Pl}^2/\lambda^2$, the fluctuating-spacetime relation that ties metric uncertainty to a length scale; combined with the observed vacuum density it gives $\Delta g \approx 5\times 10^{-61}$ and therefore $L_Z = \ell_{Pl}/\sqrt{\Delta g} \approx 2.2\times 10^{-5}$ m. The second mechanism is replacing the momentum cutoff in the vacuum integral with the Bose-Einstein factor $f(p) = [\exp(pc/k_B T) - 1]^{-1}$, which makes the integral convergent and produces $\rho c^2 = g\pi^2(k_B T)^4/[60(\hbar c)^3]$. Equating this to the observed density fixes $T \approx 41$ K, and the bridging relation $k_B T = (1/2)\hbar\omega = (1/2)\hbar c/\lambda$ converts the temperature into $\lambda \approx 2.7\times 10^{-5}$ m. That last step is what closes the argument: the uncertainty-derived cutoff and the condensate wavelength are claimed to be the same physical scale.

What would settle it

A numerical check settles the bridge relation: keeping $T = 41$ K but replacing the factor 1/2 in Eq. (20) with 1 changes $\lambda$ from $2.7\times 10^{-5}$ m to roughly $1.4\times 10^{-5}$ m, destroying the match with $L_Z$. An experimental route is to probe vacuum-fluctuation spectra in cavities with mode wavelengths near $2\times 10^{-5}$ m; if no cutoff or spectral break appears there, the proposed scale is not physical.

Watch

Extended reading notes

Core claim

On the paper's own terms, the central discovery is a single mesoscopic length scale that accounts for the cosmological constant. The vacuum-energy integral in flat spacetime, normally cut off at the Planck momentum, is terminated instead at a momentum $P_Z = \hbar/L_Z$ set by metric uncertainty $\Delta g = \ell_{Pl}^2/L_Z^2$. Matching the resulting density to the observed $\Lambda$ fixes $\Delta g \approx 5\times 10^{-61}$ and $L_Z \approx 2.2\times 10^{-5}$ m. Independently, replacing the hard cutoff by a Bose-Einstein thermal distribution yields $\rho c^2 = g\pi^2(k_B T)^4/[60(\hbar c)^3]$; equating to the observed density gives $T \approx 41$ K, and the relation $k_B T = (1/2)\hbar c/\lambda$ converts that to $\lambda \approx 2.7\times 10^{-5}$ m, consistent with $L_Z$. The convergence of these two routes is the evidence the paper offers that dark energy is a massless-boson condensate and that the vacuum-energy hierarchy reflects mesoscopic quantum-geometric structure rather than fine-tuning.

Load-bearing premise

The load-bearing premise is that the Planck-scale relation $\Delta g = \ell_{Pl}^2/\lambda^2$ still holds at $2.2\times 10^{-5}$ m and that $k_B T$ equals half the zero-point energy of a single mode (Eq. 20); if either fails, the claimed match between $\lambda$ and $L_Z$ collapses.

Editorial extensions

If this is right

  • Vacuum-energy calculations should use $L_Z \approx 2.2\times 10^{-5}$ m rather than the Planck length as the effective cutoff, suppressing the naive QFT divergence by the observed factor.
  • Dark energy is a 41 K Bose-Einstein condensate of massless bosons, not photons, whose coherence length is the same $L_Z$; the paper suggests massless gluons as the candidates.
  • Standard QFT in flat spacetime loses validity at mesoscopic scales, so renormalization-group evolution and Casimir-type predictions are modified for modes comparable to or longer than $L_Z$.
  • The geometric-mean relation $L_Z = \sqrt{\ell_{Pl}\,\ell_u}$ makes the vacuum energy a boundary effect tied to the cosmic horizon, so the cosmological constant is fixed by geometry rather than being a free parameter.

Reading between the lines

Editorial extensions of the paper, not claims the author makes directly.

  • A testable extension is that vacuum-fluctuation spectra in Casimir-type cavities with separations near $2\times 10^{-5}$ m should show a cutoff or spectral modification; measuring none would undercut the proposed scale.
  • The derivation fixes only the product $\ell_{Pl}^2/\Delta g$, so the 41 K temperature and the $2.7\times 10^{-5}$ m wavelength are not independent predictions; any bridge relation different from Eq. (20) would require re-deriving both.
  • If the same scale bounds quantum coherence generally, matter-wave interferometry with path lengths above about $2\times 10^{-5}$ m should show gravitational decoherence, offering a laboratory test independent of cosmology.
  • Should the relation hold, anthropic and quintessence-style explanations become unnecessary for the vacuum sector, since the vacuum energy would be fixed by the same $\Delta g$ that terminates short-distance QFT.
Share X Bluesky LinkedIn Reddit HN

Signed reviews

No signed human review yet.

Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, and a circularity audit.

Referee Report

3 major / 4 minor

Summary. The paper proposes that the observed value of the cosmological constant is fixed by a fundamental uncertainty in the spacetime metric, quantified by Δg ≈ 5×10⁻⁶¹, which yields a cutoff length L_Z ≈ 2.2×10⁻⁵ m when used in the vacuum-energy integral. It then models dark energy as a massless Bose-Einstein condensate: equating the BEC energy density with the observed vacuum energy gives T ≈ 41 K, and using k_B T = (1/2)ℏc/λ gives a reduced wavelength λ ≈ 2.7×10⁻⁵ m, which the authors claim aligns with L_Z. The paper argues this alignment supports the dark-energy-as-BEC hypothesis and resolves the cosmological constant problem by identifying a mesoscopic cutoff scale.

Significance. The paper addresses a central problem in theoretical physics and usefully draws attention to recent experiments at the 10⁻⁵ m scale, as well as to the possibility that an intermediate scale between the Planck length and the cosmic horizon could regulate vacuum energy. If the proposed mechanism were genuinely independent and predictive, it would be significant. However, the central consistency check between the cutoff derived in Section II and the BEC wavelength derived in Section III is a tautology: both quantities are extracted from the same observed value of the cosmological constant, and the agreement is forced by the algebraic structure and by an arbitrarily chosen prefactor. The paper does not provide a derivation of Δg or L_Z from independent principles; it inverts the observed Λ. Consequently, the main claim is not supported.

major comments (3)
  1. [Section III.B, Eq. (20)] The claimed agreement between λ ≈ 2.7×10⁻⁵ m and L_Z ≈ 2.2×10⁻⁵ m is not a physical prediction but a mathematical identity. L_Z is obtained from the observed vacuum energy density ρ via Eq. (5), while the BEC temperature T is obtained from the same ρ via Eq. (16). Substituting these into Eq. (20) gives λ/L_Z = (π/2)(4/15)^{1/4} ≈ 1.13 for g = 1, independent of the value of ρ. Thus any observed Λ would produce the same relative agreement; the alignment carries zero evidential weight. Moreover, the prefactor 1/2 in Eq. (20) is asserted without derivation, and replacing it by unity shifts λ to ≈ 1.4×10⁻⁵ m, destroying the proposed match.
  2. [Section II, Eqs. (8)-(12)] The derivation of Δg and L_Z is a fit to the observed cosmological constant, not an independent derivation. Eq. (11) solves Δg by equating the cutoff-based expression Eq. (8) to the observed density Eq. (10), and Eq. (12) then defines L_Z from Δg. The identification of L_Z with the geometric mean √(ℓ_Pl ℓ_u) is an interpretation added after the fact; it does not enter the derivation and the numerical value 2.2×10⁻⁵ m is not obtained from the geometric mean of the inputs used elsewhere in the paper. The central result is therefore not a prediction.
  3. [Section II, Eq. (6)] The extrapolation of Adler's formula Δg = ℓ_Pl²/ℓ² to ℓ = L_Z ≈ 2.2×10⁻⁵ m, more than thirty orders of magnitude above the Planck length, is not justified. The formula is derived for Planck-scale spacetime foam, and no argument is given that it remains valid in the mesoscopic regime. Since this extrapolation is the bridge between the observed Λ and the proposed cutoff scale, the physical interpretation of L_Z as a metric-uncertainty scale is unsupported.
minor comments (4)
  1. [Section III.A, Eq. (15)] Eq. (15) is garbled: the expression contains a term c^{3/4} and a misplaced superscript, and it does not reduce straightforwardly to Eq. (16). The derivation should be rewritten with correct dimensional analysis.
  2. [Section III.B, Eq. (20)] The notation ω = ∑_p ω_p = ∫ ω_p d³p is dimensionally inconsistent; the integral should be over momentum and the sum over modes needs a density of states factor.
  3. [Throughout] There are several typographical errors, including 'Renomarlization' (Section III.A heading), 'Relatvity' in reference [17], and 'W. a Heisenberg' in reference [39]; these should be corrected.
  4. [Section II, text after Eq. (12)] The claim that recent experiments have shown gravity 'effective down to 5.2×10⁻⁵ m' overstates Ref. [42], which is a test of the inverse-square law at that scale, not evidence of quantum gravitational effects.

Circularity Check

3 steps flagged · score 8.0 of 10

Claimed λ–L_Z agreement is tautological: both quantities derive from the same observed ρ, and Eq. (20)'s ad hoc 1/2 factor forces the match.

  1. fitted input called prediction [Section II, Eqs. (9)-(12)]
    "The observed vacuum energy found from the cosmological constant, Λ ≈ 10−52 m−2, is: ρobserved c2 = Λ c4/8πG = 5.3 × 10−10 J/m3 ... By comparing Eq. (8) with Eq. (10), it becomes clear that the spacetime uncertainty can be found as ... ∆g = 5 × 10−61. (11) In order to determine the value of LZ, where the uncertainty in spacetime becomes relevant, we find that L2Z = ℓPl2/∆g = 5.14 × 10−10 =⇒ LZ = 2.2 × 10−5 m. (12)"

    Eq. (5), ρvac c2 = ℏc/(16π2 LZ4), is the vacuum-energy integral with LZ as the cutoff. Equating it to the observed ρ (Eq. 9) and solving for LZ (Eq. 12) does not independently derive the cutoff from spacetime uncertainty; it defines LZ as the value that reproduces the observed vacuum density. The paper's later claim that this cutoff 'explains' the observed Λ is the same equation read backward: no new information or independent constraint enters between Eq. (9) and Eq. (12).

  2. self definitional [Section III.B, Eqs. (16)-(21)]
    "ρc2 = gπ2/60(ℏc)3 (kBT)4 ... T = 41 K ... kBT = 1/2 ℏω = 1/2 ℏc/λ ... λ = 2.7 × 10−5m (21) This value aligns with the one we derived from the cutoff in Eq. (12). This alignment serves as an affirmation of our theory that presents dark energy as a Bose-Einstein condensate."

    Both quantities compared here are functions of the same observed density ρ. LZ is obtained by inverting Eq. (5) on ρ (Eq. 9); T is obtained by inverting Eq. (16) on the same ρ (Eq. 18). Inserting the two inversions into Eq. (20) gives λ/LZ = π/60^{1/4} ≈ 1.13, a constant independent of ρ, Λ, or any data. The 'alignment' is therefore a mathematical identity between two derived functions of one input, not an empirical confirmation. It would hold for any value of the cosmological constant.

1 more flagged steps
  1. other [Section III.B, Eq. (20)]
    "kBT = 1/2 ℏω = 1/2 ℏc/λ (20) The frequency ω represents the summation of all possible frequencies with different momentum modes i.e. ω =∑p ωp = ∫ ωpd3p. The factor 1/2 as we deal with vacuum energy."

    The relation between the thermal energy of the collective Bose-Einstein distribution and the wavelength is asserted, not derived: no statistical calculation connects kBT of the many-mode distribution to half the zero-point energy of one cutoff mode. This 1/2 factor is the only free parameter that sets the numerical agreement; replacing it by 1 changes λ to about 1.4 × 10−5 m and destroys the match with LZ. Thus the claimed consistency is manufactured by this choice rather than predicted by the model.

full rationale

The paper's core validation — the claimed agreement between the Bose-Einstein wavelength λ ≈ 2.7×10−5 m (Eq. 21) and the spacetime-uncertainty cutoff LZ ≈ 2.2×10−5 m (Eq. 12) — reduces by construction. LZ is obtained by setting the vacuum-energy formula Eq. (5) equal to the observed cosmological density ρ (Eq. 9) and inverting; T is obtained by setting the Bose-Einstein density Eq. (16) equal to the same ρ (Eq. 18) and inverting; Eq. (20) then converts T into λ. Substitution shows λ/LZ = π/60^{1/4} ≈ 1.13, independent of ρ, so the two derivations must agree to about 13% for any input cosmological constant. The 1/2 factor in Eq. (20), justified only by the phrase 'as we deal with vacuum energy', is the one adjustable element that sets the ratio near unity; with a prefactor of 1 the wavelength changes to about 1.4×10−5 m and the match disappears. The announced 'affirmation' is therefore not an independent prediction but a re-expression of the fitted input. The paper does cite prior work by the authors ([35], [36], [60]), but those citations are not load-bearing for the LZ or 41 K derivations, which are arithmetic from observed Λ; no significant self-citation circularity is present. The external experimental coincidences at 10−5 m are interesting but are not used to derive the central consistency, so they do not rescue the tautological match.

Assumptions & free parameters 4 free parameters · 5 assumptions · 1 invented entities

The central number chain reads observed rho to Delta-g (Eq. 11) to L_Z (Eq. 12) to T (Eq. 18) to lambda (Eqs. 20-21). Every stage inverts the same data point; the only independent inputs are the standard constants (c, G, hbar, k_B, Lambda) and the borrowed metric-uncertainty formula Eq. (6). What survives without free parameters is the known correspondence between rho_Lambda and a ~10^-5 m cutoff, plus an unverified geometric-mean coincidence.

free parameters (4)
  • Delta-g spacetime-metric uncertainty = 5e-61
    Solved from the observed Lambda in Eq. (11); it is an inversion of the data, then converted into L_Z in Eq. (12), so the central scale is a fitted quantity in another unit.
  • Degeneracy factor g in the Bose-Einstein distribution = 1
    Chosen by hand in Eq. (14) and used in Eq. (16); it sets the constant relating T to rho and therefore determines the 41 K temperature and the final wavelength.
  • Prefactor 1/2 in Eq. (20) = 1/2
    Chosen 'as we deal with vacuum energy'; it is the factor that makes lambda = 2.7e-5 m land near L_Z. A different prefactor would break the claimed match.
  • Universe radius l_u implied by the geometric-mean claim = approximately 3e25 m
    To make Eq. (12)'s L_Z = 2.2e-5 m exactly equal to sqrt(l_Pl l_u), one needs l_u ~ 3e25 m; the paper never states this value, and standard Hubble-radius inputs give sqrt(l_Pl l_u) ~ 4.6e-5 m instead.
assumptions (5)
  • standard math The vacuum-energy integral Eq. (2) in flat Lorentzian spacetime with a sharp momentum cutoff is a valid starting point for the vacuum energy density
    Section II states Eq. (2) 'is derived under the assumption of a flat Lorentzian spacetime'; this is the standard QFT zero-point computation, accepted as background.
  • ad hoc to paper Adler's spacetime-foam formula Delta-g = l_Pl^2 / l^2 (Eq. 6) remains valid when extrapolated to l = L_Z ~ 2.2e-5 m
    The formula originates from Planck-scale estimates (Ref. [19]); the paper applies it roughly thirty orders of magnitude above the Planck length without justification.
  • domain assumption The observed dark energy density rho (Eq. 9) equals the energy density of a thermal Bose-Einstein gas (Eq. 16)
    Section III.B equates Eq. (17) with Eq. (9); this assumes dark energy is a homogeneous massless boson gas in thermal equilibrium at a single temperature.
  • domain assumption Lambda = 1.1056e-52 m^-2 is treated as a known input without quoted source or uncertainty
    Eq. (18) inserts this value; no error bar or reference for the specific number is provided in the text, and it is the single data point that drives the whole chain.
  • ad hoc to paper The relation k_B T = (1/2) hbar c / lambda (Eq. 20) connects the 41 K temperature to a single reduced wavelength
    Asserted with the comment 'The factor 1/2 as we deal with vacuum energy'; it is the entire mechanism producing lambda = 2.7e-5 m and the claimed consistency with L_Z.
invented entities (1)
  • Dark energy as a massless gluon Bose-Einstein condensate with residual SU(3) vacuum symmetry at 41 K
    purpose: Gives the fitted 41 K boson gas a physical carrier and a connection to superconductivity claims
    The identification rests on the authors' own prior work ([60], [61]); the stated 'experimental signature' (it yields the observed Hubble expansion rate) is the fitted input rho_Lambda, not an independent falsifiable handle.

how reviews work

0 comments
Cite this review

Pith. "Pith review of At the Edge of Uncertainty: Decoding the Cosmological Constant value with Bose-Einstein Distribution." pith.science (2026). https://pith.science/paper/WCEKWKIF

@misc{pith2026250511560,
  author       = {Pith},
  title        = {Pith review of: At the Edge of Uncertainty: Decoding the Cosmological Constant value with Bose-Einstein Distribution},
  year         = {2026},
  howpublished = {\url{https://pith.science/paper/WCEKWKIF}},
  note         = {Machine review of arXiv:2505.11560}
}
abstract

We propose that the observed value of the cosmological constant may be explained by a fundamental uncertainty in the spacetime metric, which arises when combining the principle that mass and energy curve spacetime with the quantum uncertainty associated with particle localization. Since the position of a quantum particle cannot be sharply defined, the gravitational influence of such particles leads to intrinsic ambiguity in the formation of spacetime geometry. Recent experimental studies suggest that gravitational effects persist down to length scales of approximately $10^{-5}$ m, while quantum coherence and macroscopic quantum phenomena such as Bose-Einstein condensation and superfluidity also manifest at similar scales. Motivated by these findings, we identify a length scale of spacetime uncertainty, $L_Z \sim 2.2 \times 10^{-5}$ m, which corresponds to the geometric mean of the Planck length and the radius of the observable universe. We argue that this intermediate scale may act as an effective cutoff in vacuum energy calculations. Furthermore, we explore the interpretation of dark energy as a Bose-Einstein distribution with a characteristic reduced wavelength matching this uncertainty scale. This approach provides a potential bridge between cosmological and quantum regimes and offers a phenomenologically motivated perspective on the cosmological constant problem.

Figures

Figures reproduced from arXiv: 2505.11560 by the authors.

Figure 1
Figure 1. FIG. 1: Animated Image of Hydrogen atom cloud. Real [PITH_FULL_IMAGE:figures/full_fig_p004_1.png] view at source ↗

Discussion (0). Continue with ORCID to comment.

Reference graph

Works this paper leans on

65 extracted references · 40 canonical work pages

  1. [1]

    At the Edge of Uncertainty: Decoding the Cosmological Constant value with Bose-Einstein Distribution

    highlighted how quantum field theory (QFT), when equipped with a Planck-scale cutoff, predicts a vacuum energy density that exceeds observational values by an enormous factor. Over the years, numerous approaches have been explored to reconcile this discrepancy. For example, early ideas by Zel’dovich [2] proposed that vacuum fluctuations, when properly accoun...

  2. [2]

    Y. B. Zel’dovich, A. Krasinski, and Y. B. Zeldovich, Sov. Phys. Usp. 11, 381 (1968)

  3. [3]

    S. M. Carroll, Phys. Rev. Lett. 81, 3067 (1998), arXiv:astro-ph/9806099

  4. [4]

    Weinberg, Rev

    S. Weinberg, Rev. Mod. Phys. 61, 1 (1989)

  5. [5]

    The observed interference pattern suggested a coherence length of approximately ≈ 10−5 m

    demonstrated the macroscopic quantum phase of Bose-Einstein condensates. The observed interference pattern suggested a coherence length of approximately ≈ 10−5 m . Additionally, another theoretical study [44] seems to set a macroscopic limit on the applicability of the uncertainty principle by studying the flow of 5 superfluid helium, It’s suggested that lo...

  6. [6]

    Dark matter and dark energy from Bose-Einstein condensate

    S. Das and R. K. Bhaduri, Class. Quant. Grav. 32, 105003 (2015), arXiv:1411.0753 [gr-qc]

  7. [7]

    Padmanabhan, Phys

    T. Padmanabhan, Phys. Rept. 380, 235 (2003), arXiv:hep-th/0212290

  8. [8]

    M. R. Andrews, C. G. Townsend, H.-J. Miesner, D. S. Durfee, and W. Ketterle, Science 275, 637 (1997)

Show all 65 references
  1. [9]

    Zlatev, L

    I. Zlatev, L. Wang, and P. J. Steinhardt, Phys. Rev. Lett. 82, 896 (1999)

  2. [10]

    Freidel, J

    L. Freidel, J. Kowalski-Glikman, R. G. Leigh, and D. Minic, Phys. Rev. D 107, 126016 (2023), arXiv:2212.00901 [hep-th]

  3. [11]

    Y. J. Ng and H. van Dam, Found. Phys. 30, 795 (2000), arXiv:gr-qc/9906003

  4. [12]

    L. D. Landau, A. A. Abrikosov, and I. M. Khalatnikov, Dokl. Akad. Nauk SSSR 95, 1177 (1954)

  5. [13]

    Wang and P

    L.-M. Wang and P. J. Steinhardt, Astrophys. J. 508, 483 (1998), arXiv:astro-ph/9804015

  6. [14]

    M. D. Schwartz, Quantum field theory and the standard model (Cambridge university press, 2014)

  7. [15]

    Witten, Adv

    E. Witten, Adv. Theor. Math. Phys. 2, 253 (1998), arXiv:hep-th/9802150

  8. [16]

    J. M. Maldacena, Adv. Theor. Math. Phys. 2, 231 (1998), arXiv:hep-th/9711200

  9. [17]

    S. S. Gubser, I. R. Klebanov, and A. M. Polyakov, Phys. Lett. B 428, 105 (1998), arXiv:hep-th/9802109

  10. [18]

    L. N. Chang, Z. Lewis, D. Minic, and T. Takeuchi, Adv. High Energy Phys. 2011, 493514 (2011), arXiv:1106.0068 [hep-th]

  11. [19]

    Montvay and G

    I. Montvay and G. M¨ unster, Quantum fields on a lattice (Cambridge University Press, 1994)

  12. [20]

    d’Inverno, Introducing Einstein ’s Relatvity (Oxford University Press, USA, 1899)

    R. d’Inverno, Introducing Einstein ’s Relatvity (Oxford University Press, USA, 1899)

  13. [21]

    Y. J. Ng and H. van Dam, Annals N. Y. Acad. Sci. 755, 579 (1995), arXiv:hep-th/9406110

  14. [22]

    R. J. Adler, Am. J. Phys. 78, 925 (2010), arXiv:1001.1205 [gr-qc]

  15. [23]

    Regge, Nuovo Cim

    T. Regge, Nuovo Cim. 7, 215 (1958)

  16. [24]

    G. A. Vilkovisky, Class. Quant. Grav. 9, 895 (1992)

  17. [25]

    W. A. Christiansen, Y. J. Ng, D. J. E. Floyd, and E. S. Perlman, Phys. Rev. D 83, 084003 (2011), arXiv:0912.0535 [astro-ph.CO]

  18. [26]

    C. A. Mead, Phys. Rev. 135, B849 (1964)

  19. [27]

    L. J. Garay, International Journal of Modern Physics A 14, 4079 (1999)

  20. [28]

    B. S. DeWitt, Physical Review Letters 13, 114 (1964)

  21. [29]

    C. A. Mead, Physical Review 143, 990 (1966)

  22. [30]

    Susskind, J

    L. Susskind, J. Math. Phys. 36, 6377 (1995), arXiv:hep-th/9409089

  23. [31]

    P. G. Tello, S. Succi, D. Bini, and S. Kauffman, (2023), arXiv:2306.17168 [physics.gen-ph]

  24. [32]

    ’t Hooft, Conf

    G. ’t Hooft, Conf. Proc. C 930308, 284 (1993), arXiv:gr-qc/9310026

  25. [33]

    Kotler, G

    S. Kotler, G. A. Peterson, E. Shojaee, F. Lecocq, K. Cicak, A. Kwiatkowski, S. Geller, S. Glancy, E. Knill, R. W. Simmonds, et al. , Science 372, 622 (2021)

  26. [34]

    J. D. Bekenstein, Phys. Rev. D 7, 2333 (1973)

  27. [35]

    A. D. O’Connell, M. Hofheinz, M. Ansmann, R. C. Bialczak, M. Lenander, E. Lucero, M. Neeley, D. Sank, H. Wang, M. Weides, et al. , Nature 464, 697 (2010)

  28. [36]

    A. F. Ali and N. Inan, EPL 143, 49001 (2023), arXiv:2309.00795 [gr-qc]

  29. [37]

    Baryshev and P

    Y. Baryshev and P. Teerikorpi, Fundamental Questions of Practical Cosmology: Exploring the Realm of Galaxies (Springer, 2012)

  30. [38]

    A. F. Ali, J. Mureika, E. C. Vagenas, and I. Elmashad, Int. J. Mod. Phys. D 33, 2450036 (2024), arXiv:2210.06262 [physics.gen-ph]

  31. [39]

    a Heisenberg, Z

    W. a Heisenberg, Z. Phys. 43, 172 (1927)

  32. [40]

    Mach, Co

    E. Mach, Co.. LCCN 60010179 (1960)

  33. [41]

    Einstein, Annalen Phys

    A. Einstein, Annalen Phys. 49, 769 (1916)

  34. [42]

    J. G. Lee, E. G. Adelberger, T. S. Cook, S. M. Fleischer, and B. R. Heckel, Phys. Rev. Lett. 124, 101101 (2020), arXiv:2002.11761 [hep-ex]

  35. [43]

    Einstein, B

    A. Einstein, B. Podolsky, and N. Rosen, Phys. Rev. 47, 777 (1935). 9

  36. [44]

    A. S. Stodolna, A. Rouz´ ee, F. L´ epine, S. Cohen, F. Robicheaux, A. Gijsbertsen, J. Jungmann, C. Bordas, and M. Vrakking, Physical Review Letters 110, 213001 (2013)

  37. [45]

    Weinberg, Phys

    S. Weinberg, Phys. Rev. Lett. 59, 2607 (1987)

  38. [46]

    Mercier de L´ epinay, C

    L. Mercier de L´ epinay, C. F. Ockeloen-Korppi, M. J. Woolley, and M. A. Sillanp¨ a¨ a, Science372, 625 (2021)

  39. [47]

    Putterman, R

    S. Putterman, R. Finkelstein, and I. Rudnick, Physical Review Letters 27, 1697 (1971)

  40. [48]

    K. B. Davis, M.-O. Mewes, M. R. Andrews, N. J. van Druten, D. S. Durfee, D. M. Kurn, and W. Ketterle, Physical Review Letters 75, 3969 (1995)

  41. [49]

    W. G. Unruh, Phys. Rev. D 40, 1048 (1989)

  42. [50]

    I. L. Shapiro and J. Sol` a, JHEP 02, 006 (2002)

  43. [51]

    E. M. Lifshitz and L. P. Pitaevskii, Statistical physics: theory of the condensed state , Vol. 9 (Elsevier, 2013)

  44. [52]

    A. J. Leggett, Quantum liquids: Bose condensation and Cooper pairing in condensed-matter systems (Oxford university press, 2006)

  45. [53]

    C. J. Pethick and H. Smith, Bose–Einstein condensation in dilute gases (Cambridge university press, 2008)

  46. [54]

    Klaers, J

    J. Klaers, J. Schmitt, F. Vewinger, and M. Weitz, Nature 468, 545 (2010)

  47. [55]

    Dodelson and F

    S. Dodelson and F. Schmidt, Modern cosmology (Academic press, 2020)

  48. [56]

    R. K. Pathria, Statistical Mechanics (Butterworth- Heinemann, 1996)

  49. [57]

    Huang, Statistical mechanics (John Wiley & Sons, 2008)

    K. Huang, Statistical mechanics (John Wiley & Sons, 2008)

  50. [58]

    Das and S

    S. Das and S. Sur, (2022), 10.48550/arXiv.2203.16402, arXiv:2203.16402 [gr-qc]

  51. [59]

    could furnish grounds for testable predictions about dark energy. The hypothesis of dark energy as a BEC, therefore, not only offers a stimulating perspective to understand this elusive component of our universe, but also delivers a novel avenue to investigate the fundamental p...

  52. [60]

    C. G. Boehmer and T. Harko, JCAP 06, 025 (2007), arXiv:0705.4158 [astro-ph]

  53. [61]

    Mandl and G

    F. Mandl and G. Shaw, Quantum field theory (John Wiley & Sons, 2010)

  54. [62]

    M. H. Anderson, J. R. Ensher, M. R. Matthews, C. E. Wieman, and E. A. Cornell, science 269, 198 (1995)

  55. [63]

    N. Inan, A. F. Ali, K. Jusufi, and A. Yasser, JCAP 08, 012 (2024), arXiv:2404.03872 [gr-qc]

  56. [64]

    A. F. Ali, SSRN 4783308 (2024), 10.2139/ssrn.4783308

  57. [65]

    Singleton, N

    D. Singleton, N. Inan, and R. Y. Chiao, Phys. Lett. A 379, 941 (2015), arXiv:1501.07665 [hep-ph]

Pith tools

Reviewed August 15, 2026 · model on record in the stance chip above.