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
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:
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:
The function χ(u) is so chosen as to ensure convergence of the heat kernel expansion of
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
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
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
and relate qB to the Dirac operator as
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:
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:
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
where we have denoted
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
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
There are three universal constants in the theory: Planck length LP and Planck time
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 ℒ is defined as
This so-called trace derivative is obtained by varying P with respect to 𝒪 and then cyclically permuting 𝒪 inside the trace, so that
The extra sign that appears in the commutator of fermionic matrices in (10) causes these matrices to follow different adjointness properties. If
So, two fermionic matrices χ1 and χ2 obey
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:
and an analogous equation for qF. Since the trace Lagrangian is independent of q, the conjugate momenta
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
where c1 and c2 are constant bosonic and fermionic matrices, respectively. These equations yield the following solutions for qB and qF:
This means that the velocities
Since
The trace Hamiltonian H can be constructed as
which becomes, after substituting for momenta and the Lagrangian
and in terms of the momenta
In trace dynamics, Hamilton’s equations of motion are
where εr = 1(−1) when qr is bosonic(fermionic). For our case, the Hamilton equations for bosonic variables are
The Hamilton equations for fermionic variables are
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
We note that it is a constant operator, and we can also express this as an eigenvalue equation
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
Thus, the Adler-Millard charge is conserved under the transformations, which obey
where U is a constant unitary matrix, which is written as
The above equation satisfies (31) if we choose
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]
Substituting the momenta in the above equation, we get
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
The terms
The terms
2.1 Adjointness Properties
The Hamiltonian is
It is very important to retain
From (40) and (41), to retain the
The Hamiltonian can be split into its self-adjoint and anti-self-adjoint parts as follows:
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
Assuming that qB is self adjoint, pB becomes self-adjoint when
which also means
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:
Using (47) and (46), (45) becomes
This is the condition for the adjointness of pB. Next, the self- and anti-self-adjoint parts of pF are given as
The self-adjoint and anti-self-adjoint parts of the fermionic anti-commutator in the Adler-Millard charge are
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.
In summary, we see that while it is reasonable to take
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
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:
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
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:
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:
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
Thus we can represent the inclusion of the anti-self-adjoint fluctuations in the above Schrödinger equation by a stochastic function
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
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:
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,
The spontaneous localisation of each STM atom to a specific eigenvalue reduces the first term of the trace Lagrangian to
If sufficiently many STM atoms undergo spontaneous localisation to occupy the various eigenvalues
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
Spontaneous localisation sends this term to
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
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
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:
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.
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
Let us return to our assumption
Let us return next to the modified Dirac equation that we wrote above:
Substituting LI as
and it is instructive to define a complex length scale Lcom by
where RS is the Schwarzschild radius associated with an STM atom of mass m having a Compton wavelength 1/L. If
For a black hole made of N nucleons, the amplified collapse rate is 10−17 N 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
Given a black hole solution ψBH (i.e.
The duality
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
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
It would be of great interest to explore the eigenvalues and eigenstates of the full Dirac operator
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
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.
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Articles in the same Issue
- Frontmatter
- Atomic, Molecular & Chemical Physics
- Numerical Investigation of the Cooling Temperature of the InGaP/InGaAs/Ge Subcells Under the Concentrated Illumination
- Dynamical Systems & Nonlinear Phenomena
- Ion-Acoustic Cnoidal Waves with the Density Effect of Spin-up and Spin-down Degenerate Electrons in a Dense Astrophysical Plasma
- Hydrodynamics
- Landau Quantised Modification of Rayleigh–Taylor Instability in Dense Plasmas
- Interaction of a Singular Surface with a Characteristic Shock in a Relaxing Gas with Dust Particles
- Quantum Theory
- Path Integrals, Spontaneous Localisation, and the Classical Limit
- Proposal for a New Quantum Theory of Gravity III: Equations for Quantum Gravity, and the Origin of Spontaneous Localisation
- Quantum-Phase-Field: From de Broglie–Bohm Double-Solution Program to Doublon Networks
- Solid State Physics & Materials Science
- Photovoltaic Generator Based on Laser-Induced Reversible Aggregation of Magnetic Nanoparticles
- Thermodynamics & Statistical Physics
- Investigation of the Finite Size Properties of the Ising Model Under Various Boundary Conditions