ЖЭТФ, 2021, том 159, вып. 4, стр. 815-821
© 2021
DIMENSIONLESS PHYSICS
G. E. Volovik*
Low Temperature Laboratory, Aalto University
P. O. Box 15100, FI-00076 Aalto, Finland
Landau Institute for Theoretical Physics, Russian Academy of Sciences
142432, Chernogolovka, Moscow Region, Russia
Received June 30, 2020,
revised version August 11, 2020
Accepted for publication August 12, 2020
Contribution for the JETP special issue in honor of I. E. Dzyaloshinskii’s 90th birthday
DOI: 10.31857/S0044451021040246
The first one is the tetrad gravity, where the tetrad
fields emerge as bilinear combinations of the fermionic
fields by symmetry breaking. This scenario has been in-
It is not excluded that the Standard Model of parti-
vestigated by Diakonov [9], Vladimirov and Diakonov
cle physics together with general relativity are effective
[10, 11], and Obukhov and Hehl [12]. The analog
theories which emerge at low energy for the collective
of Diakonov-Vladimirov (DV) scenario takes place in
modes of the extreme ultraviolet [1]. Sakharov grav-
topological superfluid3He-B [13].
ity [2], which emerges in the fermionic vacuum, pro-
vides the characteristic example. The scenario, where
The other one is the analog of gravity in the elastici-
all the known symmetries in our Universe emerge on
ty theory of crystals [14-20], where the elastic deforma-
the macroscopic scale, but disappear in the highly
tions are described in terms of the tetrads of elasticity
trans-Planckian microscopic regime, takes place in dif-
[16]. In principle, this analogy can be extended to the
ferent many-body condensed matter systems. For ex-
real gravity, if the quantum vacuum is considered as
ample, the analogs of Lorentz invariance and the curved
a plastic (malleable) fermionic crystalline medium and
spacetime are developed for some low energy fermionic
the elasticity tetrads become the gravitational tetrads
and bosonic modes [3], but these phenomena disap-
[21, 22]. The condensed matter analog of such vacuum
pear at large energy, where the microscopic degrees of
is the quantum crystal with fermionic quasiparticles,
freedom intervene (the analog of the trans-Planckian
such as vacancies [23-25].
degrees of freedom). The condensed matter systems
The common property of these two approaches to
with topologically stable Weyl points in the fermionic
spectrum, such as Weyl semimetals and the chiral su-
quantum gravity is that the tetrad fields in both theo-
ries have dimension of inverse length. As a result, most
perfluid phase of liquid3He, demonstrate simultaneous
emergence of chiral fermions, gauge bosons, and tetrad
of the physical quantities which obey diffeomorphism
gravity [4-8], which do not survive on the high-energy
invariance become dimensionless [11, 26-28]. Since the
two very different scenarios lead to the same phe-
atomic level.
nomenon, it is natural to suggest that the gravity in
We do not know the structure of the trans-Planc-
our universe also follows this common rule. Here we
kian world, but we can try different possible scenarios
consider some consequences which come from this rule.
of emergent physics and search for the common prop-
erties in the low energy corner. Here we consider two
Let us consider the theory of the crystal elastic-
scenarios of emergent gravity, which are very different,
ity using approach of Ref. [16]. The deformed crystal
but have the important common property.
structure can be described as a system of three crystal-
lographic surfaces of a constant phase, Xa(x) = 2πna,
na ∈ Z with a = 1, 2, 3. The intersection of the sur-
* E-mail: volovik@boojum.hut.fi
faces
815
G. E. Volovik
ЖЭТФ, том 159, вып. 4, 2021
X1(r, t) = 2πn1, X2(r, t) = 2πn2,
The shift of the dimensions of the physical quanti-
(1)
X3(r, t) = 2πn3
ties leads to the new properties of the quantum vacua
and also topological insulators, which allows extending
are the nodes of the deformed crystal lattice. For the
the application of the topological anomalies. For exam-
undeformed crystal, Xa(r, t) = Ka · r, where Ka are
ple, the Chern-Simons term describing the 3+1 intrin-
the (primitive) reciprocal lattice vectors. The defor-
sic quantum Hall effect becomes dimensionless. As a
mations of the crystal can be described in terms of the
result, the prefactor of this term is given by the integer
elasticity tetrads, the gradients of the phase functions:
momentum-space topological invariants as in the case
of 2 + 1 dimension [26-28]. The shift is also important
E ai(x) =iXa(x).
(2)
for the Nieh-Yan anomaly [28].
In the DV theory [9-12], the tetrads are composite
In the absence of dislocations, Eai(x) is an exact dif-
fields emerging as bilinear combinations of fermionic
ferential:
fields. Tetrads appear as the order parameter of the
kEal(x) - ∂lEak(x) = 0 .
(3)
symmetry breaking transition (see also Ref. [29]):
In the presence of the topological defects - dislocations,
e = i ψΓaμψ - ∇μψΓaψ
(6)
the density of dislocations plays the role of torsion:
The corresponding symmetry breaking scheme is LL ×
Takl = (kEal - ∂lEak).
(4)
× LS → LL+S, where LL and LS are two separate
symmetries under Lorentz rotations of the coordinate
Such construction can be extended to the 3+1 quan-
and spin space, respectively. These two symmetries are
tum vacuum with a = 0, 1, 2, 3, assuming that the vac-
broken to the diagonal subgroup — the Lorentz group
uum looks like the plastic crystalline medium. In this
of the combined rotations in two spaces, LL+S. In addi-
model the elasticity tetrads E become the gravita-
tion, this order parameter breaks the P T symmetry, see
tional tetrads [21, 22]. The deformed vacuum crystal
also Ref. [30]. The similar scheme of symmetry brea-
with dislocations describes the curved geometry of the
king of three-dimensional rotations in the orbital and
teleparallel Weitzenböck gravity with vanishing curva-
spin spaces takes place in the superfluid3He-B [13,31]:
ture and nonzero torsion. On the macroscopic coarse
grained level, where the separate dislocations are not
SO(3)L × SO(3)S → SO(3)S+L.
resolved, the torsion field Taμν can be considered as a
continuous function of coordinates. The metric gμν
According to Eq. (6), the frame field e transforms
originates from the elasticity tetrads:
as a derivative in the same manner as the elasticity
tetrads. That is why it has the dimension of inverse
gμν = ηabEE ,
(5)
length, [e] = 1/[l], i. e., its dimension is shifted from
= 1, see Table 2. In such vacua, it is
d = 0 to dDV
where ηab = (-, +, +, +).
natural to assume that the fermionic field ψ as well as
The important property of the elasticity tetrads is
the bosonic fields Φ are scalars under diffeomorphisms
that being the derivatives, they have the canonical di-
[9, 10], i. e., their dimensions are shifted from d = 3/2
mensions of inverse length, [E] = [l]-1. Correspond-
and d = 1 to dDV = 0, see Tables 2 and 3, respec-
ingly, the metric has dimension [gμν ] = 1/[l]2, while the
tively. For Weyl or massless Dirac fermions one has
interval is dimensionless: ds2 = -gμν dxμdxν , [Δs] = 1.
the conventional action:
The distance between the two nodes of the deformed
(
)
crystal is determined by the integer number of crys-
S = d4x|e|e
ψΓaμψ + H.c.
tal surfaces between the points of the grid and thus
does not depend on the length scale. In such quantum
This action expressed in terms of the DV tetrads re-
vacua, the size of the unit cell is not fixed and can be
mains dimensionless, since [e] = [l]-4, [e] = [l], and
arbitrary.
[ψ] = 1, see Table 2. This suggests that the DV dimen-
Let us introduce notation d for conventional dimen-
sion of tetrads is natural, which is also supported by
sion of the physical quantities and the notation dDV for
the elasticity tetrads.
the shifted dimension of the same quantities. The shift
The nontrivial dimension of the metric suggests that
of dimensions means that [l]-d [l]-dDV in the DV
metric is not the quantity, which describes the space-
approach. For the interval ds, the conventional dimen-
time, but the quantity, which determines the dynamics
sion d = -1 and the shifted dimension dDV = 0, see
of effective low energy fields in the background of mic-
Table 1. For the torsion field d = 1, and dDV = 2.
roscopic quantum vacuum.
816
ЖЭТФ, том 159, вып. 4, 2021
Dimensionless physics
The shifts of dimensions are shown in Tables 1, 2,
energy scale [38,39] and the neutrino mass scale [40] en-
and 3 correspondingly for gravity, fermions, and scalar
ter, ΛG2 ∼ M8W G4 and ΛG2 ∼ M4nG2, respectively.
fields. Many quantities, which obey diffeomorphism
The spacetime volume V =
d4x√-g is dimen-
invariance, become dimensionless. The action is di-
sionless, [V ] = 1, and may have quantized values. Then
mensionless and remains dimensionless in the DV di-
Λ as the corresponding Lagrange multiplier may have
mensions, since the action is a diffeomorphism invari-
universal quantized values with Λ = 0 in the equilib-
ant. Another example of the diffeomorphism invariant
rium Minkowski vacuum.
quantity is the rest mass M of particles. In the case of
The dimensionless Lagrange multiplier appears also
mass, the dimension is shifted from d = 1 to dDV = 0.
in the q-theory of the quantum vacuum [41], if the
That the DV dimension of mass is [M] = 1 can be
q-theory is based on the 4-form gauge field introduced
seen from the classical equation for the particle spec-
by Hawking for phenomenological description of the
trum: gμν pμpν = M2. According to Table 1, M2 has
quantum vacuum [42],
dimension dDV = -2 + 1 + 1 = 0, i. e., [M] = 1, and
q2 = FμναβFμναβ.
the action and the mass terms in fermionic and bosonic
actions are dimensionless:
In the DV units the vacuum variable q and the La-
grange multiplier μq (the corresponding chemical po-
S = M ds,
(7)
tential of the conserved quantity) are dimensionless,
see Table 3. If μq is fundamental, it becomes the gen-
eral characteristics of the quantum vacuum. While
S = d4x|e|Mψψ ,
(8)
the variable q determines the variable vacuum energy
Λ(q) = ϵ(q)qq, the universal chemical potential pro-
vides the nullification of Λ in the Minkowski vacuum.
At this value of μq, all the initial states (even those
S= d4x√-g(gμνμΦνΦ + M2Φ2) ,
(9)
with the Planck scale Λ) finally relax to Minkowski
vacuum with Λ = 0 [41], thus providing the solution of
the cosmological constant problems.
1
S =
d4x√-g(Fμν Fμν + M2gμν AμAν ) .
(10)
In the DV approach, mass and energy have differ-
4
ent dimensions. While mass is dimensionless, [M] = 1,
This follows from the DV dimensions
the energy has dimension of frequency, [E] = [ω] =
=[√g00] = 1/[l]. Correspondingly, the temperature is
[e] = [√-g] = [l]-4, [Φ] = [ψ] = 1,
[gμν ] = [l]-2,
dimensionless, [T ] = 1, while the constant temperature,
which enters the Tolman law [43], T (r)
-g00(r) =
[ds] = [M] = 1,
[Aμ] = [l]-1.
= TTolman, has dimension of frequency, [TTolman] =
Since the scalar curvature in general relativity is
= [ω] = [√g00] = 1/[l], see Table 1. Tolman tempe-
diffeomorphism invariant, it is dimensionless in the DV
rature is the integration constant in equilibrium in a
approach, [R] = 1. Its dimension is shifted from d = 2
stationary spacetime [44].
to dDV = 0. Other examples of the diffeomorphism in-
The Unruh temperature of the accelerated body is
variant quantities are the Newton constant G and the
TU = a/2π [45], where a is covariant acceleration,
cosmological constant Λ in the Einstein-Hilbert action:
d2xμ d2xν
a2
=gμν
1
SGR =
d4x
-g R + d4x√-g Λ .
(11)
ds2
ds2
16πG
Since a is diffeomorphism-invariant, it is dimensionless
The dimensions of G and Λ are shifted from corre-
together with the Unruh temperature, [a] = [TU ] = 1.
spondingly d = -2 and d = 4 to dDV = 0, i. e., [Λ] =
The same is with the Hawking temperature of a black
= [G] = 1. These dimensionless quantitites are deter-
hole. For the Schwartzschild black hole with rest energy
mined by the ratio of the mass scales [32] or by the
MBH, Bekenstein entropy SBH, Hawking temperature
functions of scalar fields [33]. In principle, only the ra-
TBH, and horizon area ABH:
tio between the mass parameters makes sense [10]. In
1
a given case, only the combination ΛG2 matters. Ac-
TBH =
,
8πGMBH
cording to Zeldovich [32], this combination is expressed
(12)
in terms of QCD mass scale: ΛG2 Λ6QCDG3 (see also
ABH
Refs. [34-37]). In the other approaches, the electroweak
SBH = 4πGM2BH =
4G
817
16
ЖЭТФ, вып. 4
G. E. Volovik
ЖЭТФ, том 159, вып. 4, 2021
Table 1. Dimension shifts for gravity
Table 2. Dimension shifts for fermions
General relativity
Dimension d
dDV
Fermions
Dimension d dDV
gμν
0
-2
e
0
1
gμν
0
2
eμa
0
-1
√-g
0
4
e=
√-g
0
4
d4x
√-g
-4
0
ψ
3/2
0
ds2 = gμν dxμdxν
-2
0
ψψ
4
0
dA =
dSμν dSμν
-2
0
ψΓaeμaDμψ
4
0
M
1
0
Ta
1
2
S=M
ds
0
0
TaTa
2
4
μ
1
1
2
0
λ2Nieh-Y an
pμ
1
1
eAν
Fμν
3
4
R=gμνRμν
2
0
ieμaeνbψaΓb-ΓbΓa)ψFμν
5
0
GNewton
-2
0
QQQL
6
0
R/GNewton
4
0
Λcosmological
4
0
Since
THawking
1
0
TTolman
1
1
[Sμν ] = [l]2 and
[Sμν ] = [Sμν ][gμν ]2 = 1/[l]2,
TTolman/
√g00
1
0
one obtains [A] = 1, which supports the idea that the
area of the black hole horizon is quantized [46-48].
Table 3. Dimension shifts for scalar fields
Similar quantization may occur for the de Sit-
ter spacetime, which is the submanifold of Minkowski
spacetime in the 4 + 1 dimension:
Scalar/Vector
Dimension d
dDV
Φ
1
0
g4+1Minkμνxμxν = α2.
gμνμΦνΦ
4
0
Since [gμν ] = [l]-2, the parameter α is dimensionless
M2φ2
4
0
as well as the scalar curvature R = 122, i. e., in the
Aμ
1
1
DV dimensions [R] = [α] = 1. The dimensionless pa-
rameter α of the de Sitter spacetime emphasizes the
Fμν
2
2
unique symmetry of this spacetime and supports quan-
FμνFμν
4
0
tization of this parameter (see, e. g., [49]), which could
(Fμν Fμν )k
4k
0
be similar to the Bekenstein quantization of the black
Fμν
Fμν
4
4
hole area [46]. However, in case of the superplastic
Fμναβ
4
4
vacuum, the quantization of area can be very different
from the quantization in terms of the Planck area, be-
Fμναβ
4
-4
cause the elementary cell of the underlying lattice may
q2 = FμναβFμναβ
8
0
have nothing to do with the Planck scale.
μq
0
0
Table 2 contains the operators with the mass dimen-
sions 3, 5, and 6. The non-renormalisable dimension 5
operator gives a contribution to the electron magnetic
All the quantities, that enter Eq. (12), are dimension-
moment [1]:
less in the DV approach, [TBH ] = [SBH ] = [MBH ] =
G5 = ieμaeνb
ψaΓb - ΓbΓa)ψFμν ,
= [ABH ] = [G] = 1. The area of the black hole is
dimensionless, because the covariant form of the scalar
and the non-renormalisable dimension 6 four-fermion
area element is
operator describes the baryon number violation:
dA =
dSμν dSμν .
G6 = QQQL,
818
ЖЭТФ, том 159, вып. 4, 2021
Dimensionless physics
where L and Q are the lepton and quark doublets.
contains the nonuniversal prefactor — the ultraviolet
Since in the DV approach the mass is dimensionless,
cut-off parameter λ with dimension of inverse length,
these operators become dimensionless: their dDV = 0.
[λ] = 1/[l]. Since λ may depend on coordinates, which
The prefactors in these terms are determined either
explicitly violates the topology, the Nie-Yan contribu-
by the ratio of the mass scales (“ultraviolet” and “in-
tion to the anomaly is still rather subtle (see recent
frared”) or by the functions of scalar fields. The same
literature [27, 61-65]). In the DV tetrads, the torsion
is with the 4k mass operator for k > 1 in Table 3:
in Eq. (4) has dimension [Takl] = 1/[l]2, and the prefac-
G4k = (FμνFμν)k.
tor λ2 becomes dimensionless, [λ] = 1, which suggests
In terms of the DV dimensionalities, the operators
that the prefactor is universal and is quantized.
with dDV = 4 are topological. The operators of the
The Chern-Simons term describing the 3+1 quan-
type G4 = FμνFμν are topological in both classes of
tum Hall effect can be extended to the
3+1+1
dimensions, since for them d = dDV = 4. They are
Wess-Zumino actions:
accompanied by the fundamental integer or fractional
1
prefactors. There are also operators, which have orig-
SaabWZ =
d4xdτ ϵμναβγeFaμνFbαβ .
(17)
8π2
inal dimension d = 4 but acquire dimension dDV = 4
X5
in the DV approach. This means that they are not
topological in conventional approach, but may become
SabcNY ∝ d4xdτ ϵμναβγeTbμνTcαβ .
(18)
topological in the DV dimensions.
X5
The former dimension d = 2 operator TaTa and the
dimension d = 3 operator eAνFμν acquire dimension
SabWZ ∝ d4xdτ ϵμναβγeTbμνFαβ .
(19)
dDV = 4 in the DV dimensionalities. As a result, they
X
5
become topological and their prefactors become the
In terms of DV tetrads, these dimensionless terms are
topological quantum numbers. The operator eAνFμν
universal and do not depend on the cut-off parameters.
determines the quantum Hall response in 3 + 1 topo-
In two scenarios of emergent gravity, the superplas-
logical insulators [26, 27, 50] described by the following
tic vacuum and the DV theory with bilinear tetrad
Chern-Simons topological term [27]:
field, the invariance under diffeomorphisms leads to the
dimensionless physics. In the DV theory, this invari-
S4D[Aμ] =
ance is assumed as fundamental. In the superplastic
vacuum, the diffeomorphism invariance corresponds to
1
=
Na d4x EϵμναβAναAβ .
(13)
the proposed invariance under arbitrary deformations
4π2
a=1
of the 4D vacuum crystal. In words oft Hooft (ap-
plied originally to the local conformal symmetry) “this
It explicitly contains the elasticity tetrads E. The
could be a way to make distance and time scales rel-
integer coefficients Na are three topological invariants
ative, so that what was dubbed as “small distances”
in terms of the Green’s functions:
ceases to have an absolute meaning” [66]. This suggests
that the dimensionless physics can be the natural con-
1
sequence of the diffeomorphism invariance, and can be
Na =
ϵijk
dω dSia ×
8π2
the general property of any gravity emerging in quan-
-∞ BZ
tum vacuum. The dimensionless physics leads to new
× Tr[(Gω G-1)(Gki G-1)(Gkj G-1)] .
(14)
topological terms in action with the universal integer
valued topological quantum numbers of the quantum
Invariants Na describe the quantized response of Hall
vacuum.
conductivity to crystal deformations:
The universality takes place only for the topologi-
cal numbers and the symmetry parameters. The other
ij
e2
dimensionless quantitites are not universal, being de-
=
ϵijkNa .
(15)
dEak
2πh
scribed by the functions of the ratios of different mass
scales. In this respect, the answer to the question of
In terms of the conventional tetrads, the gravita-
how many fundamental constants are there in physics
tional Nieh-Yan anomaly related to torsion [51-61],
[67-70] can be trivial: there are no fundamental con-
stants, and the ratios of parameters and the ratio of the
(
)
μjμ5 = λ2
Ta ∧Ta -ea ∧eb ∧Rab
,
(16)
length scales are the only meaningful quantities [10].
819
16*
G. E. Volovik
ЖЭТФ, том 159, вып. 4, 2021
Funding. This work has been supported by the
20.
F. W. Hehl and Y. N. Obukhov, Ann. de la Fond.
European Research Council (ERC) under the Euro-
Louis de Broglie 32, 157 (2007).
pean Unions Horizon 2020 research and innovation
21.
F. R. Klinkhamer and G. E. Volovik, JETP Lett. 109,
programme (Grant Agreement No. 694248).
362 (2019).
22.
M. A. Zubkov, arXiv:1909.08412.
The full text of this paper is published in the English
version of JETP.
23.
A. F. Andreev and I. M. Lifshitz, JETP 29, 1107
(1969).
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