# Time crystals from minimum time uncertainty

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## Abstract

Motivated by the Generalized Uncertainty Principle, covariance, and a minimum measurable time, we propose a deformation of the Heisenberg algebra and show that this leads to corrections to all quantum mechanical systems. We also demonstrate that such a deformation implies a discrete spectrum for time. In other words, time behaves like a crystal. As an application of our formalism, we analyze the effect of such a deformation on the rate of spontaneous emission in a hydrogen atom.

## 1 Introduction

The Heisenberg uncertainty principle predicts that the position of a particle can, in principle, be measured as accurately as one wants if its momentum is allowed to remain completely uncertain. However, most approaches to quantum gravity predict the existence of a minimum measurable length scale, usually the Planck length. There are also strong indications from black hole physics and other sources for the existence of a minimum measurable length [1, 2, 3]. This is because the energy needed to probe spacetime below the Planck length scale exceeds the energy needed to produce a black hole in that region of spacetime. Similarly, string theory also predicts a minimum length, as strings are the smallest probes [4, 5, 6, 7, 8]. Also in loop quantum gravity there exists a minimum measurable length scale, which turns the big bang into a big bounce [9].

The existence of a minimum measurable length scale in turn requires the modification of the Heisenberg uncertainty principle into a Generalized Uncertainty Principle (GUP) [4, 5, 6, 7]; there is a corresponding deformation of the Heisenberg algebra to include momentum-dependent terms and a modified coordinate representation of the momentum operators [8, 10, 11, 12, 13, 14, 15]. It may be noted that a different kind of deformation of the Heisenberg algebra occurs due to Doubly Special Relativity (DSR) theories, which postulate the existence of a universal energy scale (the Planck scale) [16, 17, 18]. These are also related to the idea of discrete spacetime [19], spontaneous symmetry breaking of Lorentz invariance in string field theory [20], spacetime foam models [21], spin-network in loop quantum gravity [22], non-commutative geometry [23, 24, 25], ghost condensation in perturbative quantum gravity [26], and Horava–Lifshitz gravity [27]. It may be noted that DSR has been generalized to curved spacetime and the resultant theory is called gravity’s rainbow [28, 29, 30, 31, 32, 33]. It is interesting to note that the deformation from DSR and the deformation from GUP can be combined into a single consistent deformation of the Heisenberg algebra [34].

A number of interesting quantum systems have been studied using this deformed algebra, such as the transition rate of ultra-cold neutrons in gravitational field [35], the Lamb shift and Landau levels [36]. There has been another interesting result derived from this deformed algebra, which shows that space needs to be a discrete lattice, and only multiples of a fundamental length scale (normally taken as the Planck length) can be measured [37]. Note that minimum length does not automatically imply discrete lengths, or vice versa. Motivated by this result, in this paper we analyze the deformation of the algebra and the subsequent Schrödinger equation consistent with the existence of a minimum time, and demonstrate that it leads to a discretization of time as well. It may be noted that discretization of time had also been predicted from a deformed version of the Wheeler–DeWitt equation [38]. The discretization of time, and the related breakdown of time reparametrization invariance of a system resembles a crystal lattice in time. Time crystals have been studied recently using a very different physical motivation, e.g. analyzing superconducting rings, and the spontaneous breakdown of time-translation symmetry in classical and quantum systems [39, 40, 41, 42, 43].

## 2 Observable time

In this section, we review the work done on viewing time as a quantum mechanical observable. It is well known that time cannot be represented as a self-adjoint operator [44]. This is because the Hamiltonian with a semi-bounded spectrum does not admit a group of shifts which can be generated from canonically conjugate self-adjoint operators. However, von Neumann had suggested that restricting quantum mechanics to self-adjoint operators could be quite limiting [45]. In fact, it was demonstrated by von Neumann that the momentum operator for a free particle bounded by a rigid wall at \(x = 0\) is not a self-adjoint operator but only a maximal Hermitian operator. This situation is similar to the time being defined as an observable.

*H*the map \(b \rightarrow e^{iHb}\) constitutes a unitary representation of the time translation group. Thus, the positive operator valued

*B*, with \(\theta \rightarrow B(\theta ) \), represents a time observation of the system, and it will satisfy \( e^{iHb} B(\theta ) e^{-iHb} = B(\theta - b)\). So for a time observable

*B*, it is possible to define a symmetric time operator \(t = \int t dB(t)\). This operator will not be self-adjoint. However, self-adjointness is not essential for calculating probabilities associated with the system. So, for any experiment the probability measure \(\theta \rightarrow p(\theta )\) can be associated with the states \(\rho \) by defining \(p(\theta ) = tr [\rho B(\theta )]\), where \(\theta \rightarrow B(\theta )\) is a positive operator valued measure [46]. Thus, it is possible to formally define time as an observable by using a maximal Hermitian (but non-self-adjoint) operator for time.

It is this definition of time that we will use when formally deforming the commutation relation. What we intend to do in this paper is to deform this formal definition of time to be consistent with the existence of a minimum measurable time interval. Mathematically this situation will be similar to the GUP deformation of the usual Heisenberg algebra. Physically observable time can be defined by defining an observable with reference to the evolution of some non-stationary quantity, if events are characterized by of a specific values of this quantity [46]. Such a non-stationary quantity could be the tunneling time for particles. Then the existence of a minimum measurable time interval will constitute a lower bound on such measurements. The existence of a lower bound on such measurements will effect the measurement of tunneling time for particles. In fact, such system have been analyzed by considering time as an observable [47, 48, 49, 50]. Even though such an analysis is important, we will concentrate on another problem in this paper. We will analyze the deformation of commutator between the Hamiltonian and time, and demonstrate that such a deformation can lead to the existence of a discrete spectrum for time.

## 3 Minimum time

*f*(

*H*) is a suitable function of the Hamiltonian of the system. Thus, the temporal part of Eq. (6) yields the modified Schrödinger equation

## 4 Time crystals

The spatially deformed Heisenberg algebra has been used for analyzing a free particle in a box [37]. The boundary conditions which were used for analyzing this system were \(\psi (0) =0\) and \(\psi (L) =0\), where *L* was the length of the box. It was demonstrated that the length of the box was quantized because of the spatial deformation of the Heisenberg algebra. As this particle was used as a test particle to measure the length of the box, this implied that space itself was quantized. The same argument can be now used for the temporal deformation. This can be done by taking the temporal analog of the particle in a box. The boundary conditions for this system can be written as \(\psi (0) =0\) and \(\psi (T) =0\), where *T* is a fixed interval of time. This is the temporal analog of a particle in a box, and the particle in this case is a test particle which measures the interval of time. Now we will demonstrate that in this case the interval of time has to be quantized. As this particle is a test particle used to measure this interval of time, we can argue that time itself is quantized.

## 5 Rate of spontaneous emission

It may be noted that we can also use the lifetime of particles to set bounds on \(\alpha _0\), for the modified Schrödinger equation. For example, the tau has a lifetime of \((290.3\pm 0.5)\times 10^{-15}\) s [55], and since the minimum time from Eq. (18) must be less than the uncertainty in measuring the tau’s life time, then \( 2\pi \hbar \alpha < 0.5 \times 10^{-15}\) s This means that \(\alpha _0<1.5\times 10^{27}\). However, the bound on \(\alpha _0\) from the hydrogen atom is more stringent than the bound on \(\alpha _0\) from the lifetime of particles. So, in the case that a minimum measurable time exists in nature, we are more likely to first observe its effects on the rate of spontaneous emission in hydrogen atoms.

## 6 Conclusions

We have shown here that the existence of a minimum measurable time scale in a quantum theory naturally leads to the discretization of time. This is similar to the existence of a minimum measurable length scale leading to a discretization of space. Thus, a crystal in time gets naturally formed by the existence of a minimum measurable time scale in the universe. Time crystals have been studied recently for systems in which time reparametrization is broken, just as spatial translation is broken in regular crystals. Time crystals have also been studied earlier for analyzing superconducting rings [39, 40, 41, 42, 43]. We also analyzed the effect of such a deformation on the rate of spontaneous emission in a hydrogen atom. It would be interesting to analyze a combination of minimum length and minimum time deformations of quantum mechanics to demonstrate a discretization of space and time in four dimensions. We expect to obtain non-local fractional derivative terms in that case, which may possibly be dealt with using a theory of harmonic extension of functions [56, 57], or via the Dirac equation approach [34]. It may be noted that it is conceptually useful to view the minimum measurable time as a component of a minimum Euclidean four volume with complex time, and then analytically continue the results to a Lorentz manifold. However, as we analyzed a system with Galilean symmetry, we did not to go through this procedure.

It is expected that the deformation of the Hamiltonian studied here will affect all physical systems. Thus for example, one can study the decay rates of particle and unstable nuclei using this deformed time evolution, which are expected to change as well. In fact, by fixing the value of this deformation parameter just below the experimentally measured limit, it might be possible to devise tests for detecting such deformation of time evolution of quantum mechanics. The deformed Hamiltonian should affect time-dependent perturbation theory as well. For example, the out-of-equilibrium Anderson model has been studied using the time-dependent density functional theory [58]. This has important applications for time-dependent processes in an open system where different scattering processes take place. This behavior will get modified due to this deformation of quantum mechanics. Similarly the quantum mechanical systems for which the strict adiabatic approximation fails, but which do not escape too far from the adiabatic limit, can be analyzed using a time-dependent adiabatic deformation of the theory [59]. It would be interesting to analyze the effect of having a minimum measurable time for such a time-dependent adiabatic deformation of the theory.

## Notes

### Acknowledgments

The work of SD is supported by the Natural Sciences and Engineering Research Council of Canada.

### References

- 1.M. Maggiore, Phys. Lett. B
**304**, 65 (1993)ADSCrossRefGoogle Scholar - 2.M.I. Park, Phys. Lett. B
**659**, 698 (2008)ADSMathSciNetCrossRefGoogle Scholar - 3.S. Hossenfelder, Living Rev. Relativ.
**16**, 2 (2013)ADSCrossRefGoogle Scholar - 4.D. Amati, M. Ciafaloni, G. Veneziano, Phys. Lett. B
**216**, 41 (1989)ADSCrossRefGoogle Scholar - 5.A. Kempf, G. Mangano, R.B. Mann, Phys. Rev. D
**52**, 1108 (1995)ADSMathSciNetCrossRefGoogle Scholar - 6.L.N. Chang, D. Minic, N. Okamura, T. Takeuchi, Phys. Rev. D
**65**, 125027 (2002)ADSMathSciNetCrossRefGoogle Scholar - 7.L.N. Chang, D. Minic, N. Okamura, T. Takeuchi, Phys. Rev. D
**65**, 125028 (2002)ADSMathSciNetCrossRefGoogle Scholar - 8.S. Benczik, L.N. Chang, D. Minic, N. Okamura, S. Rayyan, T. Takeuchi, Phys. Rev. D
**66**, 026003 (2002)ADSCrossRefGoogle Scholar - 9.P. Dzierzak, J. Jezierski, P. Malkiewicz, W. Piechocki, Acta Phys. Polon. B
**41**, 717 (2010)MathSciNetGoogle Scholar - 10.L.J. Garay, Int. J. Mod. Phys. A
**10**, 145 (1995)ADSCrossRefGoogle Scholar - 11.C. Bambi, F.R. Urban, Class. Quantum Grav.
**25**, 095006 (2008)ADSMathSciNetCrossRefGoogle Scholar - 12.K. Nozari, Phys. Lett. B.
**629**, 41 (2005)ADSMathSciNetCrossRefGoogle Scholar - 13.A. Kempf, G. Mangano, R.B. Mann, Phys. Rev. D
**52**, 1108 (1995)ADSMathSciNetCrossRefGoogle Scholar - 14.A. Kempf, J. Phys. A
**30**, 2093 (1997)ADSMathSciNetCrossRefGoogle Scholar - 15.S. Das, E.C. Vagenas, Phys. Rev. Lett.
**101**, 221301 (2008)ADSCrossRefGoogle Scholar - 16.J. Magueijo, L. Smolin, Phys. Rev. Lett.
**88**, 190403 (2002)ADSCrossRefGoogle Scholar - 17.J. Magueijo, L. Smolin, Phys. Rev. D
**71**, 026010 (2005)ADSMathSciNetCrossRefGoogle Scholar - 18.J.L. Cortes, J. Gamboa, Phys. Rev. D
**71**, 065015 (2005)ADSMathSciNetCrossRefGoogle Scholar - 19.G. ’t Hooft, Class. Quantum Grav.
**13**, 1023 (1996)Google Scholar - 20.V.A. Kostelecky, S. Samuel, Phys. Rev. D
**39**, 683 (1989)ADSCrossRefGoogle Scholar - 21.G. Amelino-Camelia, J.R. Ellis, N.E. Mavromatos, D.V. Nanopoulos, S. Sarkar, Nature
**393**, 763 (1998)ADSCrossRefGoogle Scholar - 22.R. Gambini, J. Pullin, Phys. Rev. D
**59**, 124021 (1999)ADSMathSciNetCrossRefGoogle Scholar - 23.S.M. Carroll, J.A. Harvey, V.A. Kostelecky, C.D. Lane, T. Okamoto, Phys. Rev. Lett.
**87**, 141601 (2001)ADSMathSciNetCrossRefGoogle Scholar - 24.M. Faizal, Phys. Lett. B
**705**, 120 (2011)Google Scholar - 25.M. Faizal, Mod. Phys. Lett. A
**27**, 1250075 (2012)ADSMathSciNetCrossRefGoogle Scholar - 26.M. Faizal, J. Phys. A
**44**, 402001 (2011)CrossRefGoogle Scholar - 27.P. Horava, Phys. Rev. D
**79**, 084008 (2009)ADSMathSciNetCrossRefGoogle Scholar - 28.J. Magueijo, L. Smolin, Class. Quantum Grav.
**21**, 1725 (2004)ADSMathSciNetCrossRefGoogle Scholar - 29.J.J. Peng, S.Q. Wu, Gen. Relativ. Gravit.
**40**, 2619 (2008)ADSMathSciNetCrossRefGoogle Scholar - 30.A.F. Ali, M. Faizal, M.M. Khalil, Nucl. Phys. B
**894**, 341 (2015)ADSCrossRefGoogle Scholar - 31.A.F. Ali, M. Faizal, M.M. Khalil, Phys. Lett. B
**743**, 295 (2015)ADSMathSciNetCrossRefGoogle Scholar - 32.A.F. Ali, M. Faizal, M.M. Khalil, JHEP
**1412**, 159 (2014)Google Scholar - 33.A.F. Ali, Phys. Rev. D
**89**, 104040 (2014)Google Scholar - 34.S. Das, E.C. Vagenas, A.F. Ali, Phys. Lett. B
**690**, 407 (2010)ADSCrossRefGoogle Scholar - 35.P. Pedram, K. Nozari, S.H. Taheri, JHEP.
**1103**, 093 (2011)ADSCrossRefGoogle Scholar - 36.A.F. Ali, S. Das, E.C. Vagenas, Phys. Rev. D
**84**, 044013 (2011)ADSCrossRefGoogle Scholar - 37.A.F. Ali, S. Das, E.C. Vagenas, Phys. Lett. B
**678**, 497 (2009)ADSMathSciNetCrossRefGoogle Scholar - 38.M. Faizal, A. F. Ali. S. Das, arXiv:1411.5675 (2014)
- 39.P. Bruno, Phys. Rev. Lett.
**111**, 070402 (2013)ADSCrossRefGoogle Scholar - 40.F. Wilczek, Phys. Rev. Lett.
**109**, 160401 (2012)ADSCrossRefGoogle Scholar - 41.A. Shapere, F. Wilczek, Phys. Rev. Lett.
**109**, 160402 (2012)ADSCrossRefGoogle Scholar - 42.E. Castillo, B. Koch, G. Palma, arXiv:1410.2261 (2014)
- 43.H. Watanabe, M. Oshikawa, Phys. Rev. Lett.
**114**, 251603 (2015)ADSCrossRefGoogle Scholar - 44.W. Paili,
*General Principle of Quantum Theory*(Springer, Berlin, 1980)CrossRefGoogle Scholar - 45.J. von Neumann,
*Mathematische Grundlagen der Quantenmechanik*(Springer, Berlin, 1932)MATHGoogle Scholar - 46.P. Buscha, M. Grabowskib, P.J. Lahtic, Phys. Lett. A
**191**, 357 (1994)ADSCrossRefGoogle Scholar - 47.V.S. Olkhovsky, Adv. Math. Phys.
**2009**, 859710 (2009)MathSciNetCrossRefGoogle Scholar - 48.V.S. Olkhovsky, Int. J. Mod. Phys. A
**22**, 5063 (2007)ADSMathSciNetCrossRefGoogle Scholar - 49.V.S. Olkhovsky, E. Recami, Int. J. Mod. Phys. B
**22**, 1877 (2008)ADSMathSciNetCrossRefGoogle Scholar - 50.R. Brunetti, K. Fredenhagen, M. Hoge, Found. Phys.
**40**, 1368 (2010)ADSMathSciNetCrossRefGoogle Scholar - 51.G. Ludwig,
*Foundations of Quantum Mechanics*, vol. 1 (Springer, Berlin, 1983)MATHGoogle Scholar - 52.A.S. Holevo,
*Probabilistic and Statistical Aspects of Quantum Theory*(North-Holland, Amsterdam, 1982)MATHGoogle Scholar - 53.D.J. Griffiths,
*Introduction to Quantum Mechanics*, 2nd edn. (Prentice Hall, NJ, 2004)Google Scholar - 54.W. Wiese, J. Phys. Chem. Ref. Data
**38**, 565 (2009)ADSCrossRefGoogle Scholar - 55.K.A. Olive et al. (Particle Data Group), Chin. Phys. C
**38**, 090001 (2014)Google Scholar - 56.M. Faizal, arXiv:1406.2653 (2014)
- 57.M. Faizal, Int. J. Geom. Methods Mod. Phys.
**12**, 1550022 (2015)MathSciNetCrossRefGoogle Scholar - 58.A.M. Uimonen, E. Khosravi, A. Stan, G. Stefanucci, S. Kurth, R. van Leeuwen, E.K.U. Gross, Phys. Rev. B
**84**, 115103 (2011)ADSCrossRefGoogle Scholar - 59.D. Viennot, J. Phys. A
**47**, 065302 (2014)ADSMathSciNetCrossRefGoogle Scholar

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