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Erratum to: Quantum-Phase-Field Concept of Matter: Emergent Gravity in the Dynamic Universe

This erratum corrects the original online version which can be found here: https://doi.org/10.1515/zna-2016-0270
  • Ingo Steinbach EMAIL logo
Published/Copyright: December 14, 2019

Erratum to: Ingo Steinbach. Quantum-Phase-Field Concept of Matter: Emergent Gravity in the Dynamic Universe. Zeitschrift für Naturforschung A. Volume 72, Issue 1, pages 51–58. (DOI:10.1515/zna-2016-0270):

PACS numbers: 04.20.Cv; 04.50.Kd; 05.70.Fh.

The work “Quantum-phase-field concept of matter: Emergent gravity in the dynamic universe”, published in [1], outlines a framework to describe physical matter from the solution of a one-dimensional non-linear wave equation. Unfortunately, a central result, the presented analytic form of this solution, (13) in [1] is incorrect. The corrected form can be found on arXiv [2]. In the present Erratum, besides the correct solution, some background information about these types of non-linear wave equations and their solutions is added. We start from a functional fDW, the famous “double-well potential”, according to Landau’s theory of phase transitions [3] with positive constants r and u, expanded in temperature T around the critical temperature Tc. ϕ~ is the “order parameter” in the original Ginzburg-Landau theory. In this theory the potential function is expanded to the fourth order, keeping only even contributions of the order parameter ϕ~:

(1)fDW=r(TTc)ϕ~2+u2ϕ~4.

The potential has a minimum at ϕ~=0 for T > Tc and two minima at ϕ~m=±r(TcT)u for T < Tc. These minima describe the disordered and ordered state of the system, respectively. Here only the ordered state T < Tc is discussed and to be consistent with conventions in the phase-field literature the order parameter is normalized to 0 ≤ ϕ ≤ 1, ϕ=12(ϕ~|ϕ~m|+1), see Figure 1.

(2)fDW=γ4ϕ2(1ϕ)2.
Figure 1: The “double-well” vs. the “double-obstackle” potential.
Figure 1:

The “double-well” vs. the “double-obstackle” potential.

Also, we will understand ϕ = ϕ(s, t) as a field variable in space s and time t and define the Hamiltonian H as an integral over the potential density and the Ginsburg gradient operators accounting for fluctuations:

(3)H=U+ds[ϵ(ϕs)2+fDW].

U is a constant with dimension of energy, ϵ is a constant with dimension of length and γ an inverse length.

The well-known minimum solution δδϕG=0 is for the boundary conditions ϕ(−∞) = 0 and ϕ(+∞) = 1:

(4)ϕ(s,t)=12[1+tanh{3(s+vt)η}],

with η=72ϵγ for a traveling wave with speed v. Note that for v ≠ 0 a symmetry breaking contribution has to be added to the potential (2), which is omitted here to keep the focus on the type of potential. Details can be found in appendix of [4]. For the boundary conditions ϕ()=ϕ(+)=0 we have, besides the trivial solution ϕ ≡ 0:

(5)ϕ(s,t)=12[tanh{3(ss1+vt)η}tanh{3(ss2vt)η}],

where the waves, peaked at s1 and s2 at t = 0, respectively, s1 < s2, travel with opposite speed, see Figure 2.

Figure 2: Traveling wave solution for the double-well and double obstacle potential. Note, that for the double-obstacle potential the width η is sharply defined whereas the for the double-well potential the 95 % decay is evaluated for the width.
Figure 2:

Traveling wave solution for the double-well and double obstacle potential. Note, that for the double-obstacle potential the width η is sharply defined whereas the for the double-well potential the 95 % decay is evaluated for the width.

It is also well established that the special form of the potential (1) or (2) is not fixed from basic principles, besides that, between the two minima there should be a potential barrier to separate the minima with a given activation energy ∝ U. Only close to the critical point, i.e. where the activation energy U → 0, a rigorous renormalization group treatment may be applied to show that higher order contributions will become irrelevant [5]. Aside from the critical point, no argument exists to truncate the Landau expansion of the potential to the fourth order or to select the given form. In the “multi-phase-field theory” [6] there arises, however, an additional constraint for the potential. In this theory a set of fields ϕI, I=1N is defined which form junctions by the condition I=1NϕI=1. The functional is replaced by H=I=1NHI where each term HI has the special form (3). In the center of the junction, where ϕI=ϕJ=1N for all I, J, the maximum of the potential fmDW can be evaluated:

(6)I=1NfmDW=γ4N(1N)2(11N)2γ41NforN1,

i.e. for N > 3 the energy of the junction decreases with the order N and approaches 0 for large N. This must be termed “unphysical”, as junctions between objects loose their penalty and the system would return to the disordered state. To remedy this problem, the so-called “double-obstacle potential” is introduced [6]:

(7)fDO=γ~2|ϕ(1ϕ)|.

It has the same topology as (2) (see Fig. 1) but a maximum power of 2. Further on it has the advantage that it defies a linear wave aside from the breakpoints. We calculate the maximum potential of the junction fmDO:

(8)I=1NfmDO=γ~2N1N(11N)γ~2forN1,

i.e. the energy of the junction increases with the order N and approaches a constant γ~ for large N, as it should. The main drawback of this potential is the non-analytical form with the absolute signs. The “non-linearity” of (2) is hidden in the breakpoints at ϕ = 0 and ϕ = 1. Only a piece-wise solution is possible for the boundary conditions ϕ(−∞) = 0 and ϕ(+∞) = 1, η=πϵγ~,

(9)ϕ={0fors<vtη2,12+12sin(π(s+vt)η)forvtη2s<vt+η2,1fors>vt+η2.

For ϕ(−∞) = ϕ(+∞) = 0, one finds (see Fig. 2):

(10)ϕ={0fors<s1vtη2,12+12sin(π(ss1+vt)η)fors1vtη2s<s1vt+η2,1fors1vt+η2s<s2+vtη2,1212sin(π(ss2vt)η)fors2+vtη2s<s2+vt+η2,0forss2+vt+η2.

The last (10) replaces (13) in [1].

References

[1] I. Steinbach, Z. Naturforsch. A 72, 51 (2017).10.1515/zna-2016-0270Search in Google Scholar

[2] I. Steinbach, arXiv:1703.05583v2 (2017).Search in Google Scholar

[3] L. D. Landau and E. M. Lifshitz, Statistical Physics Part 1, third revised edition 1980, Pergamon, Oxford 1959.10.1016/B978-0-08-057046-4.50008-7Search in Google Scholar

[4] I. Steinbach, Model. Simul. Mater. Sci. Eng. 17, 073001 (2009).10.1088/0965-0393/17/7/073001Search in Google Scholar

[5] K. G. Wilson, Phys. Rev. B 9, 3174 (1971).10.1103/PhysRevB.4.3174Search in Google Scholar

[6] I. Steinbach and F. Pezzolla, Phys. D 134, 385 (1999).10.1016/S0167-2789(99)00129-3Search in Google Scholar

Published Online: 2019-12-14
Published in Print: 2019-12-18

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