Home Proposal for a New Quantum Theory of Gravity III: Equations for Quantum Gravity, and the Origin of Spontaneous Localisation
Article Publicly Available

Proposal for a New Quantum Theory of Gravity III: Equations for Quantum Gravity, and the Origin of Spontaneous Localisation

  • Maithresh Palemkota and Tejinder P. Singh EMAIL logo
Published/Copyright: October 5, 2019

Abstract

We present a new, falsifiable quantum theory of gravity, which we name non-commutative matter-gravity. The commutative limit of the theory is classical general relativity. In the first two papers of this series, we have introduced the concept of an atom of space-time-matter (STM), which is described by the spectral action in non-commutative geometry, corresponding to a classical theory of gravity. We used the Connes time parameter, along with the spectral action, to incorporate gravity into trace dynamics. We then derived the spectral equation of motion for the gravity part of the STM atom, which turns out to be the Dirac equation on a non-commutative space. In the present work, we propose how to include the matter (fermionic) part and give a simple action principle for the STM atom. This leads to the equations for a quantum theory of gravity, and also to an explanation for the origin of spontaneous localisation from quantum gravity. We use spontaneous localisation to arrive at the action for classical general relativity (including matter source) from the action for STM atoms.

1 Introduction

This paper should ideally be read as a follow-up to the first two papers in this series [1], [2], which will be hereafter referred to as I and II, respectively.

In I, we have introduced the concept of an atom of space-time-matter (STM), which is described by the spectral action of non-commutative geometry. The spectral action, in the presence of a Riemannian manifold, is equal to the Einstein-Hilbert action of classical general relativity, after a heat kernel expansion of square of Dirac operator is carried out, and truncated at the second order in an expansion in Lp2. We also introduced there the four levels of gravitational dynamics. In II, we used the Connes time parameter, along with the spectral action, to incorporate gravity into trace dynamics. We then derived the spectral equation of motion for the gravity part of the STM atom, which turns out to be the Dirac equation on a non-commutative space. In the present work, we propose how to include the matter (fermionic) part and give a simple action principle for the STM atom. This leads to the equations for a quantum theory of gravity, and also to an explanation for the origin of spontaneous localisation from quantum gravity. We use spontaneous localisation to arrive at the action for classical general relativity (including matter sources) from the action for STM atoms.

2 Equations of Quantum Gravity at Level 0

In II, we have proposed the following action principle for the gravity part of the STM atom:

(1)SGTD=κcLPdτTr[χ(LP2q˙2/L2c2)].

Here, τ is what we have called the Connes time of non-commutative geometry. The q-operator, which describes gravity, is related to the operator D (which becomes the standard Dirac operator on a curved space when there is a background Riemannian manifold) as follows:

(2)D1Lcdqdτ.

The function χ(u) is so chosen as to ensure convergence of the heat kernel expansion of Tr(Lp2D2) (for a discussion on this aspect, see e.g. [3], [4]). κ is a constant so chosen that it gives the correct dimensions of action and the correct numerical coefficient for recovery of the Einstein-Hilbert action. L is a length scale associated with the STM atom, whose physical interpretation will become evident subsequently.

Our motivation behind introducing the operator q ‘particle’ is to establish contact between non-commutative geometry (and the description of gravity therein) on one hand, and trace dynamics on the other. We were seeking an action principle that can be expressed conventionally as the time-integral of a Lagrangian, with the Lagrangian being made of matrix-valued configuration variable q and its velocity q˙. Hence the action (1), and the relation (2) which relates the q-operator to gravity, via the spectral action and its heat kernel expansion.

The above description, which is the essence of what was done in II, serves as the starting point for the present paper: we will now propose an action principle for the STM atom, which includes fermions, in addition to gravity. First, we simplify the above gravity action and its notation. We will assume for now that χ(u) = u, leaving for later the considerations of convergence of the heat kernel expansion. Further, setting κC0/2, where C0 is a real constant with dimensions of action, we can write the action (1) as

(3)LPcSGTDC0=12dτTr[LP2q˙2/L2c2]

q is assumed to have dimension of length, and the expression inside the trace is dimensionless. In the spirit of trace dynamics, we shall assume that the matrix q (equivalently the operator) is made from elements that are complex numbers or anti-commuting Grassmann numbers. In particular, we shall assume that the q matrix above is made from even-grade elements of the Grassmann algebra, and is therefore a ‘bosonic’ matrix, which we shall henceforth label as qB. This assumption is natural keeping in view that the above action describes gravity, via the spectral action of non-commutative geometry, and the Dirac operator is bosonic (and self-adjoint). Thus we rewrite the action (1) as

(4)LPcSGTDC0=12dτTr[LP2q˙B2/L2c2]

and relate qB to the Dirac operator as

(5)DB1LcdqBdτ.

Since the concept of an STM atom was introduced in I as an entity that describes both matter and gravity at Level 0, we must now introduce the fermionic/matter aspect in this action. In order to do so, we define a new q-operator as follows:

(6)q=qB+qF,

where qF is fermionic, i.e. it is made of odd-grade elements of the Grassmann algebra. However, we do not yet place any adjointness requirement on qB or qF: the Dirac operator DB will now be made from the self-adjoint part of qB. The above split of q as bosonic plus fermionic simply represents the fact that any matrix made from Grassmann elements can be written as a sum of a bosonic matrix plus a fermionic matrix. The split is significant though, as we will soon see that qF behaves very differently from qB: not only does it describe emergent fermions but it also paves the way for spontaneous localisation in a quantum gravity theory. The STM atom is assumed to be described by the following fundamental action principle, which is at the heart of all subsequent development:

(7)LPcSC0=12dτTr[LP2L2c2(q˙B+β1q˙F)(q˙B+β2q˙F)].

Here, β1 and β2 are two constant fermionic matrices. These matrices make the Lagrangian bosonic. The assumptions on these matrices are that they should not both simultaneously commute (or anti-commute) with q˙F (as justified later in the paper). These assumptions are necessary for retaining the q˙Fq˙F term in the trace Lagrangian, which would otherwise vanish. The above trace Lagrangian can be expanded and written as

(8)LPcSC0=a2dτTr[q˙B2+q˙Bβ2q˙F+β1q˙Fq˙B+β1q˙Fβ2q˙F],

where we have denoted aLP2/L2c2.

The first term inside the trace Lagrangian has the familiar structure of a kinetic energy, and in any case it is what gives rise to the Einstein-Hilbert action in the heat kernel expansion of DB2. It is the cross terms in the trace Lagrangian, which result from introducing the fermionic qF, that are a game changer and, as we shall see, responsible for causing spontaneous collapse, besides bringing in fermions. As in trace dynamics, we assume the trace Lagrangian to be an even-grade element of the Grassmann algebra. We will denote the trace Lagrangian by the symbol P, i.e. P=Tr, where is the operator polynomial that defines the Lagrangian in this matrix dynamics.

It is noteworthy that the introduction of the two constant matrices β1 and β2 seems essential for the following reasons. Our starting point for constructing the present Lagrangian is the gravity Lagrangian in (3) for the bosonic qB. It is natural that to introduce fermions, we generalise qB to q=qB+qF. We also expect the Lagrangian to be quadratic in time derivative with respect to τ, and we also ask for the Lagrangian to be bosonic. This makes it essential that a constant fermionic matrix β be brought in, and the trace Lagrangian be made from the bosonic q=qB+βqF. For instance, the trace Lagrangian could be Tr(q˙B+βq˙F)2. Intriguingly, we did not succeed in making a consistent model with only one constant matrix in the Lagrangian. On the other hand, the situation eases immediately when two constant matrices are brought in (i.e. β1 and β2). Furthermore, if we are seeking a bosonic trace Lagrangian which is at the most quadratic in q, then it will not be possible to introduce more than two constant matrices so we seem to be dealing with a generic ‘free-particle’ quadratic trace Lagrangian, which incorporates qF. Our Lagrangian is not self-adjoint (nor the action is), though, as we shall see, it becomes self-adjoint in the limit in which classical dynamics (Level III) and quantum field theory (Level II) are recovered. The anti-self-adjoint part of the Lagrangian is responsible for spontaneous localisation, and it arises quite naturally from the structure of our assumed trace Lagrangian: as soon as the fermionic part qF is introduced, spontaneous localisation becomes inevitable.

There are three universal constants in the theory: Planck length LP and Planck time τP=LP/c, where the speed of light c should be thought as the ratio Lp/τP. The third universal constant C has dimensions of action, and at Level I will be identified with the Planck constant ℏ. Newton’s gravitational constant G and Planck mass mP are emergent only at Level I. In fact, the concepts of mass and spin themselves emerge only at Level I, and are not present at Level 0. We associate only a length scale (more precisely an area L2) with the STM atom, but not mass nor spin, at Level 0.

One can now derive the Lagrange equations of motion, as is done in trace dynamics. The derivative of the trace Lagrangian P (note that P is a complex number) with respect to an operator 𝒪 in is defined as

(9)δP=TrδPδ𝒪δ𝒪.

This so-called trace derivative is obtained by varying P with respect to 𝒪 and then cyclically permuting 𝒪 inside the trace, so that δ𝒪 sits to the right of the polynomial . While permuting cyclically inside the trace, one has to keep in mind the change in sign when permuting two fermionic matrices χ1, χ2, and no change in sign when a bosonic matrix B is permuted with any other matrix:

(10)Tr[B1,B2]=Tr[B2,B1],Tr[B,χ]=Tr[χ,B],Tr[χ1,χ2]=Tr[χ2χ1].

The extra sign that appears in the commutator of fermionic matrices in (10) causes these matrices to follow different adjointness properties. If 𝒪1g1,,𝒪ngn are n matrices with grades g1,..,gn, respectively, then

(11)(𝒪1g1𝒪ngn)=(1)i<jgigj𝒪ngn𝒪.1g1

So, two fermionic matrices χ1 and χ2 obey (χ1χ2)=χ2χ1. This minus sign is not there if one or both matrices are bosonic.

We can now vary the action (8) with respect to qB and qF, in the spirit of trace dynamics, and obtain the Lagrange equations of motion:

(12)ddτ(δPδq˙B)(δPδqB)=0

and an analogous equation for qF. Since the trace Lagrangian is independent of q, the conjugate momenta pB=δP/δq˙B and pF=δP/δq˙F are constant. From the trace derivative of the trace Lagrangian with respect to q˙B and q˙F, we get the momenta to be

(13)pB=δLδq˙B=a2[2q˙B+(β1+β2)q˙F],
(14)pF=δLδq˙F=a2[q˙B(β1+β2)+β1q˙Fβ2+β2q˙Fβ1].

We note that all the degrees of freedom qB, qF, pB, pF obey arbitrary time-dependent commutation relations with each other. Quantum commutation relations emerge after constructing a statistical thermodynamics for an ensemble of STM atoms [5].

The momenta pB and pF are, respectively, bosonic/fermionic. Both the momenta are constant, because the trace Lagrangian does not depend on q. This implies

(15)2q˙B+(β1+β2)q˙F=c1,
(16)q˙B(β1+β2)+β1q˙Fβ2+β2q˙Fβ1=c2,

where c1 and c2 are constant bosonic and fermionic matrices, respectively. These equations yield the following solutions for qB and qF:

(17)q˙B=12[c1(β1+β2)(β1β2)1[2c2c1(β1+β2)](β2β1)1],
(18)q˙F=(β1β2)1[2c2c1(β1+β2)](β2β1)1.

This means that the velocities q˙B and q˙F are constant, and qB and qF evolve linearly in Connes time.

Since pB=a2c1 and pF=a2c2, (17) and (18) can be written as

(19)q˙B=1a[pB(β1+β2)(β1β2)1[2pFpB(β1+β2)](β2β1)1],
(20)q˙F=2a(β1β2)1[2pFpB(β1+β2)](β2β1)1.

The trace Hamiltonian H can be constructed as

(21)H=Tr[pFq˙F]+Tr[pBq˙B]Tr,

which becomes, after substituting for momenta and the Lagrangian

(22)H=Tr[a2(q˙B+β1q˙F)(q˙B+β2q˙F)]

and in terms of the momenta

(23)H=Tr2a[(pBβ1pF)(β2β1)1(pBβ2pF)(β1β2)1].

In trace dynamics, Hamilton’s equations of motion are

(24)δHδqr=p˙r,δHδpr=εrq˙r,

where εr = 1(−1) when qr is bosonic(fermionic). For our case, the Hamilton equations for bosonic variables are

(25)q˙B=2a[β1(β2β1)1(pBβ2pF)(β1β2)1+β2(β1β2)1(pBβ1pF)(β2β1)1],
(26)p˙B=0.

The Hamilton equations for fermionic variables are

(27)q˙F=2a[(β2β1)1(pBβ2pF)(β1β2)1+(β1β2)1(pBβ1pF)(β2β1)1],
(28)p˙F=0.

It can be verified that these equations are identical with those solutions above, which come from Lagrange’s equations.

Taking cue from the expression for pB, we can define the generalised (bosonic) Dirac operator D given by

(29)1LcdqdτDDB+DF;DB1LcdqBdτ;DFβ1+β22LcdqFdτ.

We note that it is a constant operator, and we can also express this as an eigenvalue equation

(30)[DB+DF]ψ=λψ,

where the eigenvalues λ, assumed to be c-numbers, are independent of Connes time τ, and the state ψ can depend on τ at most through a multiplicative factor.

In trace dynamics, there is a conserved charge, known as the Adler-Millard charge, corresponding to a global unitary invariance of the trace Lagrangian/Hamiltonian. Assume a dynamical operator xr that undergoes a transformation as xrUxrU, where U is a constant N × N matrix, given by U=expΛ, where Λ is an anti-self-adjoint bosonic generator matrix. Under such a transformation of operators, the trace Hamiltonian remains invariant.

Thus, the Adler-Millard charge is conserved under the transformations, which obey

(31)L({UqrU},{Uq˙rU})=L({qr},{q˙r}),

where U is a constant unitary matrix, which is written as U=expΛ, where Λ is an anti-self-adjoint bosonic generator matrix. Applying the above condition on our Lagrangian gives

(32)L({UqrU},{Uq˙rU})=Tr[Uq˙B2U+Uq˙BUβ2Uq˙FU+β1Uq˙Fq˙BU+β1Uq˙FUβ2Uq˙FU].

The above equation satisfies (31) if we choose

(33)Uβ2U=β2andUβ1U=β1.

This condition also means that β1 and β2 commute with U (or Λ equivalently).

The Adler-Millard charge in trace dynamics can be shown to be [5]

(34)C~=rB[qr,pr]rF{qr,pr}.

Substituting the momenta in the above equation, we get

(35)(2/a)C~=[qB,2q˙B+(β1+β2)q˙F]{qF,q˙B(β1+β2)+β1q˙Fβ2+β2q˙Fβ1}=[qB,2q˙B]+[qB,(β1+β2)q˙F]{qF,q˙B(β1+β2)}{qF,β1q˙Fβ2+β2q˙Fβ1}.

The cross terms in the charge are expected to vanish at equilibrium when one constructs a statistical thermodynamics for this matrix dynamics. The important terms that lead to the emergence of statistical thermodynamics, and cause spontaneous collapse, are 2[qB,q˙B] and {qF,β1q˙Fβ2+β2q˙Fβ1}. Splitting qB into its self-adjoint and anti-self-adjoint parts, i.e. qB=qBS+qBAS, we get

(36)2[qB,q˙B]=2([qBS,q˙BS]+[qBS,q˙BAS]+[qBAS,q˙BS]+[qBAS,q˙BAS])

The terms [qBS,q˙BAS] and [qBAS,q˙BS] are self-adjoint, and the terms [qBS,q˙BS], [qBAS,q˙BAS] are anti-self-adjoint. Now writing pFf=β1q˙Fβ2+β2q˙Fβ1 and splitting qF and pFf into their self-adjoint and anti-self-adjoint parts, i.e. qF=qFS+qFAS and pF=pFSf+pFASf, we have

(37){qF,pFf}={qFS,pFSf}+{qFS,pFASf}+{qFAS,pFSf}+{qFAS,pFASf}.

The terms {qFS,pFASf}, {qFAS,pFSf} are self-adjoint, and the terms {qFS,pFSf}, {qFAS,pFASf} are anti-self-adjoint. The anti-self-adjoint part of C~ determines the emergent quantum commutators at equilibrium [5].

2.1 Adjointness Properties

The Hamiltonian is

(38)H=Tr[a2(q˙B+β1q˙F)(q˙B+β2q˙F)].

It is very important to retain Tr[β1q˙Fβ2q˙F] in the trace Hamiltonian to get fermionic anti-commutator in the conserved charge:

(39)Tr[β1q˙Fβ2q˙F]=Tr[q˙Fβ1q˙Fβ2]
(40)=Tr[β1q˙Fβ2q˙F+[q˙F,β1]β2q˙F+β1q˙F[q˙F,β2]+[q˙F,β1][q˙F,β2]]
(41)=Tr[β1q˙Fβ2q˙Fβ1q˙F{q˙F,β2}{q˙F,β1}β2q˙f+{q˙F,β1}{q˙F,β2}]

From (40) and (41), to retain the Tr[β1q˙Fβ2q˙F], both β1 and β2 cannot simultaneously commute or anti-commute with q˙F.

The Hamiltonian can be split into its self-adjoint and anti-self-adjoint parts as follows:

(42)HS=Tr[q˙B2+[(β1q˙F)S+(β2q˙F)S]q˙B+(β1q˙Fβ2q˙F)S],
(43)HAS=Tr[[(β1q˙F)AS+(β2q˙F)AS]q˙B+(β1q˙Fβ2q˙F)AS].

Let us consider the adjointness property of the momentum pB. For the remainder of our analysis, we shall assume that qB is self-adjoint: this is consistent with the assumption that the bosonic Dirac operator DB made from qB is required to be self-adjoint in the spectral action. pB is

(44)pB=a2(2q˙B+(β1+β2)q˙F).

Assuming that qB is self adjoint, pB becomes self-adjoint when

(45)[(β1q˙F)AS+(β2q˙F)AS]=0,

which also means

(46)(β1+β2)q˙F+q˙F(β1+β2)=0.

Equation (46) does not say anything about the adjointness of β1 and β2 individually. We may assume for simplicity that β1 and β2 are self-adjoint:

(47)β1=β1&β2=β2.

Using (47) and (46), (45) becomes

(48){(β1+β2),q˙FS}+[(β1+β2),q˙FAS]=0.

This is the condition for the adjointness of pB. Next, the self- and anti-self-adjoint parts of pF are given as

(49)pFS=a4[{q˙B,(β1+β2)}+2(β1q˙FASβ2+β2q˙FASβ1)],
(50)pFAS=a4[[q˙B,(β1+β2)]+2(β1q˙FSβ2+β2q˙FSβ1)].

The self-adjoint and anti-self-adjoint parts of the fermionic anti-commutator in the Adler-Millard charge are

(51)C~FS={qS,(β1q˙ASβ2+β2q˙ASβ1)}+{qAS,(β1q˙Sβ2+β2q˙Sβ1)},
(52)C~FAS={qS,(β1q˙Sβ2+β2q˙Sβ1)}+{qAS,(β1q˙ASβ2+β2q˙ASβ1)}.

In these two equations, q stands for qF. In (46), the sum of the terms is zero. However, if the terms are independently zero, i.e. (β1q˙F)AS=0 and (β2q˙F)AS=0, then HAS will vanish.

In summary, we see that while it is reasonable to take q˙B as self-adjoint, it is not really necessary to assume pB, pF, and H to be self-adjoint, at Level 0. All that we should require is that at Levels II and III, i.e. in quantum field theory and classical dynamics, these quantities should become self-adjoint. We will see in the next section that this can be ensured. However, we do not make our measurements at Level 0; hence there is no reason to require these quantities to be self-adjoint at Level 0. In fact, it is their anti-self-adjoint component, which arises very naturally, that is responsible for a dynamical origin of the quantum-to-classical transition (spontaneous localisation). Thus, in this theory, it is not necessary to ascribe any interpretation to quantum theory to get the classical world to emerge from quantum theory. It is the presence of these anti-self-adjoint terms that gets missed when we construct a quantum theory of gravity by quantizing a classical theory of gravity. The bottom-up approach to quantum gravity has more information than a top-down approach.

The fact that the STM atom evolves like a free particle, inspite of the Hamiltonian not being self-adjoint, suggests that we could think of its motion in the Hilbert space as ‘geodesic’ motion in a non-commutative geometry. We can associate a state vector with the STM atom, analogous to the four-velocity vector in special relativity, whose length remains unchanged during geodesic (i.e. free) motion. This observation will help us in the next section to motivate the constancy of the norm of the state vector in the emergent theory. This overcomes a limitation of collapse models, in which norm preservation in the presence of stochastic noise has to be added by hand as an ad hoc assumption, so as to be able to derive the Born probability rule.

Our theory also enables us to construct a relativistic quantum (field) theory of spontaneous localisation. It is our contention that a relativistic theory of spontaneous collapse must treat time at the same footing as three-space. This implies that there must take place spontaneous localisation in coordinate time, besides in space. This requires us to treat coordinate time, besides the spatial position of a particle, as an operator. The role of time as an evolution parameter has to be then played by something else, and Connes time does precisely that. A relativistic quantum field theory must treat coordinate time also as an operator, but so long as spontaneous collapse in time can be neglected, treating operator time as a classical Lorentz invariant coordinate time is an excellent approximation as is assumed in conventional quantum field theory. It is well known though, that one can also develop an equivalent version of quantum field theory (the so-called Stueckelberg-Horwitz relativistic quantum mechanics [6]), which treats time as an operator and introduces, alongwith, a new absolute time parameter for defining evolution.

At Level 0, the Hilbert space is populated by a large number of STM atoms, each of which is a free particle described by the dynamics described above. Interaction between atoms is via entanglement of their individual states. Each q-particle carries its own set of non-commuting space-time coordinates (see I). There is no classical space-time, only a Hilbert space in which evolution is with respect to Connes time τ. There is a conserved Adler-Millard charge for the collection of atoms, as given by (34), where the index r indicates sum over all STM atoms. Classical space-time emerges after one carries out a statistical thermodynamics of a large number of STM atoms, and spontaneous localisation arises away from thermodynamical equilibrium. This is described in the next section. Note that we do not quantise this matrix dynamics; rather, quantum theory emerges from it, just like in trace dynamics.

3 Origin of Spontaneous Localisation

Once the matrix dynamics at Level 0 has been specified by prescribing the Lagrangian, one constructs the statistical thermodynamics of a large number of STM atoms. The motivation is that if one is not observing the microscopic dynamics at the Planck scale, it is then the emergent coarse-grained dynamics that is of interest. To do this, one applies the standard principles of statistical mechanics to an ensemble of STM atoms, as is done in trace dynamics (see e.g. Chapter 4 of Adler’s book [5]). One starts by setting up an integration measure in the operator phase space for the bosonic and fermionic matrices. Then a Liouville theorem is derived. Next, given the operator phase space measure, one defines an equilibrium phase space density ρ, which is used to define the probability of finding the system in the phase space volume element dμ. A canonical ensemble and an entropy function are constructed, as a function of the conserved charges: the trace Hamiltonian and the Adler-Millard charge. The equilibrium distribution is constructed by maximising the entropy function. While we will describe this analysis in detail in a forthcoming work, the analysis essentially follows that in trace dynamics. All that we have done in the present paper is to propose a specific trace dynamics Lagrangian that brings gravity into the trace dynamics framework and unifies it with matter fermions. And although classical space-time is lost at Level 0, Connes time enables us to define evolution.

This sets the stage for the emergence of the coarse-grained quantum gravitational dynamics at thermodynamic equilibrium. A Ward identity, which is the equivalent of the equipartition theorem, is derived. As in trace dynamics, the anti-self-adjoint part of the conserved Adler-Millard charge is equipartitioned over all the degrees of freedom, and the equipartitioned value per degree of freedom is identified with the Planck constant ℏ. At thermodynamic equilibrium, the standard quantum commutation relations of (an equivalent of) quantum general relativity emerge, for the canonical averages of the various degrees of freedom:

(53)[qB,pB]=i;{qFS,pFASf}=i;{qFAS,pFSf}=i.

All the other commutators and anti-commutators amongst the canonical degrees of freedom vanish at thermodynamic equilibrium. The above set of commutation relations hold for every STM atom. We note that we describe quantum general relativity in terms of these q-operators, and not in terms of the metric and its conjugate momenta, which are emergent concepts of Levels II and III.

The mass m of the STM atom is defined by m=/Lc; and L is interpreted to be its Compton wavelength. Newton’s gravitational constant G is defined by GLp2c3/, and Planck mass mP by mP=/LPc. Mass and spin are both emergent concepts of Level I; at Level 0, the STM atom only has an associated length L.

As a consequence of Hamilton’s equations at Level 0, and as a consequence of the Ward identity mentioned above, the canonical thermal averages of the canonical variables obey the Heisenberg equations of motion of quantum theory, these being determined by HS, the canonical average of the self-adjoint part of the Hamiltonian:

(54)iqBτ=[qB,HS];ipBτ=[pB,HS];iqFτ=[qF,HS];ipFfτ=[pFf,HS].

In analogy with quantum field theory, one can transform from the above Heisenberg picture, and write a Schrödinger equation for the wave function Ψ(τ) of the full system:

(55)iΨτ=HStotΨ(τ),

where HStot is the sum of the self-adjoint parts of the Hamiltonians of the individual STM atoms. Since the Hamiltonian is self-adjoint, the norm of the state vector is preserved during evolution. This equation is the analog of the Wheeler-DeWitt equation in our theory, the equation being valid at thermodynamic equilibrium at Level I. This equation can possibly resolve the problem of time in quantum general relativity, because to our understanding it does not seem necessary that the physical state must be annihilated by HStot. We have not arrived at this theory by quantising classical general relativity; rather, the classical theory will emerge from here after spontaneous localisation, as we now describe.

We can now describe how spontaneous localisation comes about. It is known that the above emergence of quantum dynamics arises at equilibrium in the approximation that the Adler-Millard conserved charge is anti-self-adjoint, and its sef-adjoint part can be neglected. In this approximation, the Hamiltonian is self-adjoint. Another way of saying this is that quantum dynamics arises when statistical fluctuations around equilibrium (which are governed by the self-adjoint part of C~) can be neglected. When the thermodynamical fluctuations are important, one must represent them by adding a stochastic anti-self-adjoint operator function to the total self-adjoint Hamiltonian (note that one cannot simply add the anti-self-adjoint part of the Hamiltonian to the above Schrödinger equation because that equation is defined for canonically averaged quantities; the only way to bring in fluctuations about equilibrium is to represent them by stochastic functions). This way of motivating spontaneous collapse is just as in trace dynamics (see Chapter 6 of [5]), except that we are not restricted to the non-relativistic case and evolution is with respect to Connes time τ. Also, we do not have a classical space-time background yet; this will emerge now, as a consequence of spontaneous localisation (see also our earlier related paper ‘ Space-time from collapse of the wave function’ [7]).

Thus we can represent the inclusion of the anti-self-adjoint fluctuations in the above Schrödinger equation by a stochastic function (τ) as

(56)iΨτ=[HStot+(τ)]Ψ(τ).

In general, this equation will not preserve the norm of the state vector during evolution. However, as we noted above, every STM atom is in free-particle geodesic motion. Hence it is very reasonable to demand that the state vector should preserve the norm during evolution, even after the stochastic fluctuations have been added. Then, exactly as in collapse models and in trace dynamics, a new state vector is defined, by dividing Ψ by its norm, so that the new state vector preserves norm. Then it follows that the new norm-preserving state vector obeys an equation that gives rise to spontaneous localisation, just as in trace dynamics and collapse models (see Chapter 6 of [5]). We should also mention that the gravitational origin of the anti-self-adjoint fluctuations presented here (DF is likely of gravitational origin, and relates to the anti-symmetric part of an asymmetric metric) agrees with Adler’s proposal that the stochastic noise in collapse models is seeded by an imaginary component of the metric [8], [9].

It turns out to be rewarding to work in the momentum basis where the state vector is labelled by the eigenvalues of the momenta pB and pF. Since the Hamiltonian depends only on the momenta, the anti-self-adjoint fluctuation is determined by the anti-self-adjoint part of pF. Hence it is reasonable to assume that spontaneous localisation takes place onto one or the other eigenvalue of pFf. No localisation takes place in pB: this helps in understanding the long-range nature of gravity (which results from qB and the bosonic Dirac operator DB). We assume that the localisation of pFf is accompanied by the localisation of qF and, hence, that an emergent classical space-time is defined using the eigenvalues of qF as reference points. Space-time emerges only as a consequence of the spontaneous localisation of matter fermions. Thus we are proposing that the eigenvalues of qF serve to define the space-time manifold. It is not clear to us at this stage as to what exactly is the relation between the q-operator and the classical space-time metric: as of now we assume that when spontaneous localisation leads to the emergence of a classical space-time, it also (somehow) defines the space-time metric. As in collapse models, the rate of localisation becomes significant only for objects that comprise a large number of matter fermions; hence the emergence of a classical space-time is possible only when a sufficiently macroscopic object comprising many STM atoms undergoes spontaneous localisation. It is evident that such localisation is far from an equilibrium process, consequent upon a sufficiently large statistical fluctuation coming into play. We now give a quantitative estimate as to what qualifies as sufficiently macroscopic.

To arrive at these estimates, we recall the following two earlier equations, the action principle for the STM atom itself and the eigenvalue equation for the full Dirac operator D:

(57)LPcS=a2dτTr[q˙B2+q˙Bβ2q˙F+β1q˙Fq˙B+β1q˙Fβ2q˙F],
(58)[DB+DF]ψ=λψ(λR+iλI)ψ(1L+i1LI)ψ.

In the second equation, since D is bosonic, we have assumed that the eigenvalues λ are complex numbers and separated each eigenvalue into its real and imaginary part. Furthermore, this will be taken as the definition of the length scale L introduced earlier. We come back to LI below. There will be one such pair of equations for each STM atom, and the total action of all STM atoms will be the sum of their individual actions, with the individual action given as above.

When an STM atom undergoes spontaneous localisation, pFf localises to a specific eigenvalue. Since DF is also made from q˙F, just as pFf is, we assume that DF also localises to a specific eigenvalue, whose imaginary part is the LI introduced above. Correspondingly, the DB associated with this STM atom acquires a real eigenvalue, which we identify with the λR1/L above (setting aside for the moment the otherwise plausible situation that, in general, pF will also contribute to λR).

The spontaneous localisation of each STM atom to a specific eigenvalue reduces the first term of the trace Lagrangian to

(59)Tr[q˙B2]λR2.

If sufficiently many STM atoms undergo spontaneous localisation to occupy the various eigenvalues λRi of the Dirac operator DB, then we can conclude, from our knowledge of the spectral action in non-commutative geometry [4], that their net contribution to the trace is

(60)a2Tr[q˙B2]=2Tr[Lp2DB2]=2Lp2(λRi)2=2Lp2d4xgR.

Thus we conclude that the Einstein-Hilbert action emerges after spontaneous localisation of the matter fermions. In that sense, gravitation is indeed an emergent phenomenon. Also, the eigenvalues of the Dirac operator DB have been proposed as dynamical observables for general relativity [10], which in our opinion is a result of great significance.

Let us now examine how the matter part of the general relativity action arises from the trace Lagrangian (its second and third terms) after spontaneous localisation. These terms are

(61)a2Tr[q˙Bβ2q˙F+β1q˙Fq˙B]=Tr[Lp2DFDB].

Spontaneous localisation sends this term to Lp2×1/Li×1/L. There will be one such term for each STM atom and, analogous to the case of TrDB2, we anticipate that the trace over all STM atoms gives rise to the ‘source term’

(62)gd4xi[Lp2×1/LIi×1/Li].

Consider the term for one atom. We make the assumption (which becomes plausible shortly) that spontaneous localisation localises the STM atom to a spatial volume L3 such that Lp2LI=L3. We note that it is natural to identify L with the Compton wavelength ℏ/mc of the STM atom. Moreover, we may say that the classical approximation consists of replacing the inverse of the spatial volume of the localised particle, i.e. 1/L3, by the spatial delta function δ3(xx0) so that the contribution to the matter source action becomes

(63)gd4x[Lp2×1/LI×1/L]=mcds,

which of course is the action for a relativistic point particle.

Putting everything together, we conclude that, upon spontaneous localisation, the fundamental trace-based action for a collection of STM atoms becomes

(64)S=d4xg[c32GR+cimiδ3(xx0)].

In this way, we recover general relativity at Level III, as a result of spontaneous localisation of quantum general relativity at Level I. We should not think of the gravitational field of the STM atom as being disjoint from its related fermionic source: they both come from the same eigenvalue λ, being, respectively, the real and imaginary parts of this eigenvalue.

Strictly speaking, the Connes time integral should also be displayed in the action principle:

(65)S=cLPdτd4xg[c32GR+cimiδ3(xx0)].

It is as if the observed universe is an enormous, spontaneously collapsed bubble that evolves ‘inside of a sea of’ uncollapsed STM atoms. Inside the bubble there is a space-time, with its own time evolution parameter, with no direct indicator of Connes time. ‘Outside’ of the bubble, there is no space-time, but only a Hilbert space populated with other STM atoms, evolving in Connes time. Could it be that the Big Bang represents an exceedingly huge spontaneous collapse event, involving an entangled state of an astronomical number of STM atoms? Is such spontaneous localisation accompanied by the expansion of the resulting classical space-time? And could it be that there are very many other spontaneously collapsing bubble universes forming all the (Connes) time, in the Hilbert space of STM atoms? The far-from-equilibrium dynamics of such spontaneous fluctuations in an ensemble of STM atoms should be an interesting aspect to explore.

We have not been able to come to a definite conclusion as regards what happens to the last term in the trace Lagrangian (57) (i.e. β1q˙Fβ2q˙F) after spontaneous localisation. It roughly has the structure Tr[DF2]. Adding the contribution of the eigenvalues qF ⁢ 1 and qF ⁢ 2 of β1q˙F and β2q˙F from all STM atoms, we get Tr[qF1iqF2i]. While we do not have a proof, we suggest that this could give rise to the cosmological constant term of general relativity. If this were to be true, then we can schematically sum up the overall picture as

(66)SNMG=dτiTrDi2dτ[c32Gd4xg[R2Λ]+d4xgLmatter]

Here, SNMG on the left is the total action of all STM atoms in this non-commutative matter-gravity. The action on the right side of the arrow describes classical general relativity with a cosmological constant and point matter sources and is what emerges after spontaneous localisation. Our theory thus elegantly unifies, in a simple way, the disjoint matter-gravity descriptions on the right-hand side, by bringing them together as TrDi2. Note that, unlike the action on the left-hand side of the arrow, the right-hand side of the above equation is in no way the sum of the contributions of individual STM atoms: the matter part is a sum, but the gravity part is not. Undoubtedly then, the gravity part is an emergent condensate. It simply cannot be quantised. The right-hand is the (commutative) action at Level III covariant under general coordinate transformation of commuting coordinates, whereas the left-hand side action at Level I is covariant under general coordinate transformations of non-commuting coordinates. It is interesting that the transition from a non-commutative geometry to a commutative geometry is caused by spontaneous localisation and that statistical thermodynamics plays a central role in it.

Let us return to our assumption LI=L3/LP2, which, as we will now see, has profound consequences. If we consider the case of a nucleon, and substitute for L the Compton wavelength of a nucleon (∼10−13 cm), then LI comes out to be 1027 cm, which is close to the size of the observed universe (1028 cm). If this is not a coincidence, it suggests the possibility of a connection between spontaneous localisation and the scale of the universe. In particular, it might be possible to define the rate of spontaneous collapse as LI/c1017s1, which happens to be the same as the collapse rate assumed in standard models of localisation.

Let us return next to the modified Dirac equation that we wrote above:

(67)[DB+DF]ψ=λψ(λR+iλI)ψ(1L+i1LI)ψ.

Substituting LI as LI=L3/LP2, we can write this as

(68)[DB+DF]ψ=1L(1+iLP2L2)ψ

and it is instructive to define a complex length scale Lcom by

(69)LcomL2=1L(1+iLP2L2)1L(1+iRSL)Lcom=L+iRS,

where RS is the Schwarzschild radius associated with an STM atom of mass m having a Compton wavelength 1/L. If RSL (i.e. mmPl), the imaginary part of the complex length is ignorable compared to the real part, hence DF can be ignored compared to DB and we get the standard Dirac equation for a matter fermion. This is the microscopic quantum limit, where spontaneous localisation is insignificant. On the other hand, when RSL, (i.e. mmPl), the imaginary part of the length Lcom dominates over the real part, spontaneous localisation is significant, and we recover classical behaviour: in fact, a black hole solution of radius RS. Thus our matrix dynamics nicely interpolates between quantum theory and classical mechanics; we did not have to put in this behaviour by hand, rather it comes out quite naturally from the theory. Incidentally, the ratio L2/RS=2/Gm3, which is implicit in the above length scale, arises naturally as the decoherence length scale when one studies gravitationally induced decoherence using the Schrödinger-Newton equation. In our context, it implies that gravitational decoherence is significant when the Compton wavelength is larger than this decoherence length. As expected, for a nucleon this length is of the order of the size of the universe. The length Lcom cannot have a magnitude smaller than Planck length: this possibly is a way of avoiding the gravitational singularity of a black hole, because it will never shrink to a vanishing Lcom.

For a black hole made of N nucleons, the amplified collapse rate is 10−17N s−1, which for an astrophysical black hole with N ∼ 1057 gives an extremely rapid rate of 1040 collapses per second; obviously, then black holes behave classically. An object with a mass smaller than Planck mass cannot be a black hole: it is necessarily quantum in nature.

The Dirac equation (68) is one of great significance, as it admits solutions which have Dirac fermions and black holes as their special limiting cases. In that sense, this equation unifies the standard Dirac equation with Einstein equations. It answers the question: given a relativistic mass m, does it obey the Dirac equation or Einstein’s equations? It also helps in understanding why a Kerr-Newman black hole has the same gyromagnetic ratio as the electron: because they are both solutions of the same equation, i.e. (68).

Equation (68) admits a duality, between black hole and fermion solutions, after it is written as

(70)[DB+DF]ψ=LcomL2(L+iRS)ψ.

Given a black hole solution ψBH (i.e. RSL) with mass mBH, consider a Dirac fermion solution ψF (i.e. LRS) with a mass mF=mPl2/mBH. That is, the second solution is obtained by setting its Schwarzschild radius equal to Compton wavelength of first solution and setting its Compton wavelength equal to Schwarzschild radius of first one. This interchange means that the eigenvalue λF of the second solution is mPl2/mBH2 times the eigenvalue λBH of the first one, and the real and imaginary parts have been interchanged. Thus, given a solution ψBH with eigenvalue λBH, its dual solution ψF can be found by interchanging the real and imaginary parts of the eigenvalue and downscaling the magnitude of the eigenvalue, as just mentioned. This duality might be of some help in a computation of the entropy of the black hole, from a knowledge of the eigenvalues and eigenstates of the Dirac operator DB. This is plausible because the action function of the black hole, which in turn is related to its entropy, is after all constructed from the eigenvalues of DB.

The duality LLP2/L has been investigated earlier as well. The conclusion that space-time intervals have a minimum length LP has been derived in [11] by proposing that in the path integral for a spin-zero free particle, paths of length l have the same weightage as paths of length LP2/l. The subtle difference in our case is the i factor, which enables spontaneous localisation: thus the duality in our case is liLP2/l.

Thus far we have derived a reasonable understanding of the dynamics of STM atoms at Level 0, Level I, and Level III. Level 0 is the fundamental matrix dynamics, Level I is its statistical thermodynamics (equivalent of quantum general relativity), and Level III is its classical limit (caused by spontaneous localisation), i.e. the classical theory of general relativity. Level II is the hybrid level: quantum field theory on a curved space-time. Level II is concerned with those STM atoms that have not yet undergone spontaneous localisation. How to describe their dynamics from the point of view of the classical space-time which has already been created from the spontaneous localisation of many many other STM atoms? These uncollapsed atoms obviously live at Level 0, where we know how to understand their dynamics. Furthermore, we can also do the statistical thermodynamics for them and describe them at Level I, while neglecting their spontaneous localisation at Level I. To arrive at Level II, we first neglect their own gravitational degree of freedom qB, replace the Connes time evolution by time evolution provided by the emergent space-time of collapsed STM atoms, and replace their DB operator by the standard Dirac operator associated with the emergent space-time. We also neglect DF (no spontaneous localisation). Thus we have the standard Dirac equation for fermions, as well their standard quantum commutators. Since we have not yet introduced non-gravitational interactions in this matrix dynamics, there are no other bosonic fields yet in the theory.

It is very interesting to ask if we could have missed out some vital information in going from Level I to Level II in the above manner. Indeed we have. We recall from the discussion earlier in this section that space-time is emergent from the spontaneous localisation of qF. If we were to describe spontaneous localisation of the fermionic degrees of freedom at Level II, we must invoke the statistical fluctuations around equilibrium. And if we want to have a relativistic theory of collapse at Level II, we will need to bring Connes time back into the picture and describe spontaneous localisation at Level II precisely as we did above. We cannot appeal to the emergent space-time to provide a background for relativistic collapse [7]. This leads to a falsifiable prediction: spontaneous collapse of the operator coordinate time t^. Thus Connes time is crucial at Level II as well if we are to describe relativistic spontaneous localisation. Of course, one can take the non-relativistic limit of the relativistic theory of Level II and then describe collapse in absolute Newtonian time, as is done in conventional collapse models.

4 Concluding Remarks

We have presented a viable new quantum theory of gravity, which predicts spontaneous localisation and spontaneous collapse in time. The theory is hence falsifiable, and a vigorous experimental effort is currently under way in various laboratories to test models of spontaneous collapse [12], [13]. Our theory combines non-commutative geometry and trace dynamics to construct a matrix dynamics for our newly introduced concept of atoms of space-time matter. This is a quantum theory of gravity, from which quantum general relativity and classical general relativity emerge as approximations.

Among the outstanding open issues that still need to be resolved are understanding the exact relation between the q-operator and the space-time metric and the interpretation of the operator DF. Our guess is that qB somehow relates to the symmetric part of an asymmetric metric at Level 0, and qF relates to its complex anti-symmetric part, with DF being related to a complex torsion induced by the anti-symmetric part of the asymmetric metric. Also, right at the beginning we made the assumption χ(u) = u and restricted ourselves to the second order in the heat kernel expansion of the Dirac operator. Also we neglected the cosmological constant term, which arises at order LP4 in the heat kernel expansion. These assumptions will need to be relaxed so that one deals with the full theory without an expansion in LP2. Furthermore, DB is defined on a Euclidean space-time, so we have a Euclidean quantum gravity theory. This will have to be replaced by the Lorentzian theory. Another important aspect is to now include other interactions in this framework.

It would be of great interest to explore the eigenvalues and eigenstates of the full Dirac operator D=DB+DF on a non-commutative space. This could help predict the discrete masses of elementary particles. We have already seen above the relation LI=L3/LP2 between the real and imaginary parts of the eigenvalue of the D-operator. The fact that LI comes out to be the order of the size of the observed universe introduces an infra-red scale into the theory, which could help address the hierarchy problem. In fact, this relation allows us to ‘predict’ the mass mPr of a proton in terms of the Planck mass mP and the Hubble parameter (LIcH01), recalling that L is the Compton wavelength:

(71)mPrmP(LPcH01)1/3.

We can say that the proton mass is much much smaller than the Planck scale, because the universe is much much bigger than the Planck scale.

Our theory probably also has interesting implications for black hole evaporation. Black holes for us arise as a spontaneous localisation of a collection of STM atoms having a total mass M, for which the Schwarzschild radius exceeds the Compton wavelength. Thus black hole formation is a far-from-equilibrium, non-unitary (caused by a statistical fluctuation) process. Thus even though a black hole has enormous entropy, it is nonetheless a far-from-equilibrium state of relatively low entropy (compared to what it would be at thermodynamic equilibrium). Hawking evaporation is a process (opposite to spontaneous localisation) whereby a black hole returns to thermodynamic equilibrium with the ‘sea of STM atoms’ in the Hilbert space. Recall that the equilibrium is described by quantum general relativity/quantum field theory. In the long run, all matter in the universe will condense into black holes, and then evaporate as radiation and go back to quantum gravitational equilibrium: this will amount to loss of classical space-time and a return to evolution in Connes time. There is no question of an information loss paradox, because in the first place the formation of a black hole is itself a non-unitary process [14].

Lastly, we note that we were compelled to introduce two constant matrices β1 and β2, and work with qB+β1qF and qB+β2qF, as if to suggest that our STM atom is a two-dimensional entity (‘space time is two-dimensional at the Planck scale?’). Could it be that the object that we have called the STM atom is after all the closed string of classical string theory? Or, could it be related to the loop in loop quantum gravity?

Acknowledgements

For valuable discussions and ongoing collaboration, we would like to thank B. J. Arav, Shivnag Sista, Diya Kamnani, Guru Kalyan, Shubham Kadian, Siddhant Kumar, Ankur, Abhinav Varma, Ish Mohan Gupta, Krishnanand K Nair, and Shounak De. TPS would like to thank Thanu Padmanabhan for insightful conversations on this work.

References

[1] T. P. Singh, Z. Naturforsch. A 74, 617 (2019).10.1515/zna-2019-0079Search in Google Scholar

[2] T. P. Singh, Z. Naturforsch. A 74, (2019).10.1515/zna-2019-0041Search in Google Scholar

[3] A. Connes, in: Visions in Mathematics – GAFA 2000 Special Volume, Part II (Eds. N. Alon, J. Bourgain, A. Connes, M. Gromov, and V. Milman), Springer, Birkhauser Basel 2000, p. 481, arXiv:math/0011193.10.1007/978-3-0346-0425-3_3Search in Google Scholar

[4] G. Landi, Lect. Notes Phys. 596, 299 (2002).10.1007/3-540-46082-9_16Search in Google Scholar

[5] S. L. Adler, Quantum Theory as an Emergent Phenomenon, Cambridge University Press, Cambridge 2004.10.1017/CBO9780511535277Search in Google Scholar

[6] L. P. Horwitz, Relativistic Quantum Mechanics, Springer, Netherlands 2015.10.1007/978-94-017-7261-7Search in Google Scholar

[7] T. P. Singh, Z. Naturforsch. A 74, 147 (2019).10.1515/zna-2018-0477Search in Google Scholar

[8] S. L. Adler, Quantum Non-locality and Reality (Eds. M. Bell and S. Gao), Cambridge University Press, Cambridge 2016.Search in Google Scholar

[9] S. L. Adler, Found. Phys. 48, 1557 (2018).10.1007/s10701-018-0215-7Search in Google Scholar

[10] G. Landi and C. Rovelli, Phys. Rev. Lett. 78, 3051 (1997).10.1103/PhysRevLett.78.3051Search in Google Scholar

[11] T. Padmanabhan, Phys. Rev. Lett. 78, 1854 (1997).10.1103/PhysRevLett.78.1854Search in Google Scholar

[12] A. Bassi, K. Lochan, S. Satin, T. P. Singh, and H. Ulbricht, Rev. Mod. Phys. 85, 471 (2013).10.1103/RevModPhys.85.471Search in Google Scholar

[13] M. Carlesso and M. Paternostro, Do Wave Functions Jump? Perspectives on the Work of GianCarlo Ghirardi (Eds. V. Allori, A. Bassi, D. Dürr, and N. Zanghì), SpringerNature, Berlin, Germany (forthcoming in 2019).Search in Google Scholar

[14] S. De, T. P. Singh, and A. Varma, Int. J. Mod. Phys. D 28, (2019). DOI: 10.1142/S0218271819440036, arXiv:1903.11066.10.1142/S0218271819440036Search in Google Scholar

Received: 2019-08-18
Accepted: 2019-09-09
Published Online: 2019-10-05
Published in Print: 2020-02-25

©2020 Walter de Gruyter GmbH, Berlin/Boston

Downloaded on 23.9.2025 from https://www.degruyterbrill.com/document/doi/10.1515/zna-2019-0267/html
Scroll to top button