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arXiv:1602.00089v2 [quant-ph] 12 Jun 2016

Casimir energy between two parallel plates
and projective representation of Poincaré group

Takamaru Akita 1 ** * E-mail: akita@q.phen.mie-u.ac.jp and   Mamoru Matsunaga 1,2 E-mail: matsuna@phen.mie-u.ac.jp; matsunaga@ars.mie-u.ac.jp

1Department of Physics Engineering, Mie University,
Tsu 514-8507, JAPAN
2College of Liberal Arts and Sciences, Mie University,
Tsu 514-8507, JAPAN

Abstract

The Casimir effect is a physical manifestation of zero point energy of quantum vacuum. In a relativistic quantum field theory, Poincaré symmetry of the theory seems, at first sight, to imply that non-zero vacuum energy is inconsistent with translational invariance of the vacuum. In the setting of two uniform boundary plates at rest, quantum fields outside the plates have (1+2)-dimensional Poincaré symmetry. Taking a massless scalar field as an example, we have examined the consistency between the Poincaré symmetry and the existence of the vacuum energy. We note that, in quantum theory, symmetries are represented projectively in general and show that the Casimir energy is connected to central charges appearing in the algebra of generators in the projective representations.

1 Introduction

Since the pioneering work of Casimir [1], vacuum energy of quantum fields has been the subject of intense investigations from both experimental and theoretical sides [2, 3, 4, 5]. Experimental measurements of the Casimir forces, by using an atomic force microscope or micro-electromechanical system, reach the high precision at the level within 1% and agreement with the theoretical prediction is also at the same level at least for zero temperature. Theoretical investigation of the Casimir effects extends a variety of fields of physics such as particle physics, atomic physics, astrophysics and cosmology, and condensed matter physics. In particle physics, for example, the Casimir energy of quark and gluon fields inside a hadron makes essential contributions to its mass. The Casimir force offers one of the effective mechanisms for spontaneous compactification of extra spatial dimensions in the Kaluza-Klein theories.

This paper discuss more theoretical issue, i.e. we examine the consistency between the existence of the Casimir energy and the Poincaré symmetry in the setting of two uniform perfectly-reflecting parallel boundary planes at rest. In this configuration, the quantum field theory is invariant under the time-translation, the translations and boosts along the plane, and under the rotation in the plane. As a result of these invariances of the theory, it seems that, if require the translational invariance of the vacuum (vanishing total momentum of the field), then the vacuum energy should vanish. This argument has a loophole as expected. We pay our attention to the representation of symmetries in quantum theory and to the fact that, in order to compare the zero point energies, we have to consider time-dependent Hamiltonian connecting the different static configurations.

The paper is organize as follows. In Sec. 2, we set up the problem in the example of a massless scalar field. Sec. 3 summarizes the projective representation and linear representations of symmetries in quantum theory. In Sec. 4, an adiabatic process connecting two static configuration is analyzed. The final section is devoted to the conclusion.

2 Setup

In this section,we set up the problem in the case of massless scalar field theory in Ox1x2x3O\mathchar 45x_{1}x_{2}x_{3} space with the Dirichlet boundary condition ϕ=0\phi=0 on the planes x3=L,Lx_{3}=-L,L.

This theory is invariant under the translations along the x1,x2x_{1}\mathchar 45,x_{2}\mathchar 45directions and the time direction, under the rotation in x1x2x_{1}x_{2}\mathchar 45plane, and under the boosts along the x1,x2x_{1}\mathchar 45,x_{2}\mathchar 45directions. These transformations and their compositions form the (1+2)-dimensional Poincaré group. Denoting the respective generator as P1,P2,H,J,K1,K2P_{1},P_{2},H,J,K_{1},K_{2}, we are given the Lie algebra of the Poincaré group

[Pi,Pj]\displaystyle[P_{i},P_{j}] =[Pi,H]=[J,H]=0,\displaystyle=[P_{i},H]=[J,H]=0, (1)
i[J,Pi]\displaystyle i[J,P_{i}] =ϵijPj,i[J,Ki]=ϵijKj,\displaystyle=-\epsilon_{ij}P^{j},\quad\quad i[J,K_{i}]=\epsilon_{ij}K^{j}, (2)
i[Ki,Kj]\displaystyle i[K_{i},K_{j}] =ϵijJ,i[Ki,H]=Pi,\displaystyle=\epsilon_{ij}J,\quad\quad\quad i[K_{i},H]=P_{i}, (3)
i[Ki,Pj]\displaystyle i[K_{i},P_{j}] =δijH,\displaystyle=\delta_{ij}H, (4)

with i,j=1,2i,j=1,2, the antisymmetric tensor ϵ12=1\epsilon_{12}=1 and summation for the repeated indices being implied.

Since the field ϕ\phi satisfies the d’Alembert equation and the Dirichlet boundary condition, ϕ\phi can be expanded as

ϕ(t,x1,x2,x3)=n=1ϕ(n)(t,x1,x2)sinnπLx3,\phi(t,x_{1},x_{2},x_{3})=\sum_{n=1}^{\infty}\phi^{(n)}(t,x_{1},x_{2})\sin\frac{n\pi}{L}x_{3},

where the expansion coefficient ϕ(n)\phi^{(n)} satisfies the (1+2)-dimensional Klein-Gordon equation

(2+mn2)ϕ(n)(t,x1,x2)=0(n=1,2,).(\square_{2}+{m_{n}}^{2})\phi^{(n)}(t,x_{1},x_{2})=0\quad(n=1,2,\ldots).

with mn:=nπ/Lm_{n}:=n\pi/L. i.e. each mode ϕ(n)\phi^{(n)} forms (1+2)-dimensional scalar field with the mass mnm_{n}.

The Lagrangian density \mathcal{L} for the (1+3)-dimensional field ϕ\phi is written as the sum of the Lagrangian density (n)\mathcal{L}^{(n)} for the (1+2)-dimensional fields ϕ(n)\phi^{(n)}:

=n=1(n),\displaystyle\mathcal{L}=\sum_{n=1}^{\infty}\mathcal{L}^{(n)}, (5)
(n)=12(μϕ(n)μϕ(n)mn2ϕ(n) 2).\displaystyle\mathcal{L}^{(n)}=\frac{1}{2}(\partial^{\mu}\phi^{(n)}\partial_{\mu}\phi^{(n)}-{m_{n}}^{2}\phi^{(n)\,2}). (6)

As a result, the (1+3)-dimensional Poincaré algebra is decomposed to a direct sum of the (1+2)-dimensional ones generated by the generators Pi(n),H(n),J(n),Ki(n)P^{(n)}_{i},H^{(n)},J^{(n)},K^{(n)}_{i} for each nn-th mode. These generators have the same form of commutation relation as eqs. (1)–(4). In the following we take up the nn-th mode and drop the upperscript (n)(n).

We express the generators of the Poincaré algebra for the nn-th mode in terms of the canonical conjugate pairs ϕ(t,𝒙),π(t,𝒙)(𝒙:=(x1,x2))\phi(t,\bm{x}),\pi(t,\bm{x})\;(\bm{x}:=(x_{1},x_{2})), whose dynamics is derive from the Lagrangian (6) and whose commutation relations are given by

[ϕ(t,𝒙),ϕ(t,𝒙)]\displaystyle[\phi(t,\bm{x}),\phi(t,\bm{x}^{\prime})] =[π(t,𝒙),π(t,𝒙)]=0,\displaystyle=[\pi(t,\bm{x}),\pi(t,\bm{x}^{\prime})]=0, (7)
[ϕ(t,𝒙),π(t,𝒙)]\displaystyle[\phi(t,\bm{x}),\pi(t,\bm{x}^{\prime})] =iδ2(𝒙𝒙).\displaystyle=i\delta^{2}(\bm{x}-\bm{x}^{\prime}). (8)

Following Noether’s prescription, we obtain

H\displaystyle H =d2x,=12(π2+(ϕ)2+mn2ϕ2),\displaystyle=\int d^{2}x\,\mathcal{H},\quad\quad\mathcal{H}=\frac{1}{2}\left(\pi^{2}+(\nabla\phi)^{2}+{m_{n}}^{2}\phi^{2}\right), (9)
Pi\displaystyle P_{i} =d2xπiϕ,Ki=tPid2xxi,\displaystyle=\int d^{2}x\,\pi\,\partial_{i}\phi,\quad\quad K_{i}=tP_{i}-\int d^{2}x\,x_{i}\mathcal{H}, (10)
J\displaystyle J =d2xϵijxiπjϕ.\displaystyle=\int d^{2}x\,\epsilon_{ij}x^{i}\,\pi\,\partial^{j}\phi. (11)

Using the canonical commutation relations (7), (8), we see that eqs. (1)–(4) are satisfied. In particular, the vacuum expectation values of eq. (4)

i[Ki,Pi]=H(i=1,2)i[K_{i},P_{i}]=H\quad(i=1,2) (12)

gives

i0|[Ki,Pi]|0=0|H|0.i\left\langle 0\right|[K_{i},P_{i}]\left|0\right\rangle=\left\langle 0\right|H\left|0\right\rangle. (13)

If we require the translational invariance of the vacuum, P|0=0P\left|0\right\rangle=0, then eqs. (9) and (13) give

0|H|0=12d2x(0|π2|0+0|(ϕ)2|0+mn20|ϕ2|0)=0,\left\langle 0\right|H\left|0\right\rangle=\frac{1}{2}\int d^{2}x\left(\left\langle 0\right|\pi^{2}\left|0\right\rangle+\left\langle 0\right|(\nabla\phi)^{2}\left|0\right\rangle+{m_{n}}^{2}\left\langle 0\right|\phi^{2}\left|0\right\rangle\right)=0, (14)

which means

ϕ|0=ϕ|0=π|0=0\phi\left|0\right\rangle=\nabla\phi\left|0\right\rangle=\pi\left|0\right\rangle=0

in contradiction to eq. (8).

Usually, in field theories without boundaries, with the aid of the arbitrary additive constant inherent in the definition of the Hamiltonian, HH is redefined to satisfy H|0=0H\left|0\right\rangle=0, which, in turn, seems to mean the nonexistence of Casimir energy. This is nothing but the inconsistency sketched out in Sec. 1.

In the following sections, we show that this apparent inconsistency disappears if we note the following two points:

  • In quantum theory, symmetries are represented projectively in general, and represented linearly if certain condition is satisfied.

  • In the Casimir effect, comparison between the vacuum energies of two different configuration are made: in the setting we are considering, two configuration of the plates are e.g. L=L0L=L_{0} and L=L1L=L_{1}. Since the system should be described by a single Hamiltonian, we are to consider time-dependent Hamiltonian connecting L=L0L=L_{0} and L=L1L=L_{1}.

3 Projective representation of Poincaré group

In Sec. 2 we describe the Lie algebra of Poincaré group as eqs. (1)–(4). If the group is linearly represented, i.e. represented by a homomorphism from the group to linear operators, then the Lie algebra is nothing but the commutator algebra of the generators. However, as is well-known, in quantum theory, symmetry group GG is represented projectively in general [6]: Unitary operators U(g)(gG)U(g)\;(g\in G) form a linear representation up to phase factor, which means

U(g)U(g)=eiθ(g,g)U(gg)(g,gG).U(g)\,U(g^{\prime})=e^{i\theta(g,g^{\prime})}U(g\,g^{\prime})\quad(g,g^{\prime}\in G). (15)

Setting U(e)=IU(e)=I without loss of generality and expanding U(g)U(g) around g=eg=e, we get, from eq. (15), the algebra of the generators, wherein there appear central charges corresponding to the phase factor eiθe^{i\theta}. The associative law of the products of U(g)U(g)’s

U(g)(U(g)U(g′′))=(U(g)U(g))U(g′′)(g,g,g′′G)U(g)\,\left(U(g^{\prime})\,U(g^{\prime\prime})\right)=\left(U(g)\,U(g^{\prime})\right)\,U(g^{\prime\prime})\quad(g,g^{\prime},g^{\prime\prime}\in G) (16)

gives some constraints, called the cocycle condition, on the the phases θ(g,g)\theta(g,g^{\prime}). If we multiply U(g)U(g) by a phase factor eiα(g)e^{i\alpha(g)} and redefine eiα(g)U(g)e^{i\alpha(g)}\,U(g) as U(g)U(g),then the phase becomes θ(g,g)α(g)α(g)\theta(g,g^{\prime})-\alpha(g)-\alpha(g^{\prime}). In most cases, this redefinition of U(g)U(g) could makes the phase factor to disappear [7, 8].

In our case of (1+2)-dimensional Poincaré group, the algebra of the generators P1,P2,H,J,K1,K2P_{1},P_{2},H,J,K_{1},K_{2} has the central charges in the righthand side of eq. (1)–(4): for example,

i[Ki,H]\displaystyle i[K_{i},H] =Pi+C0,0i,\displaystyle=P_{i}+C_{0,0i}, (17)
i[Ki,Pj]\displaystyle i[K_{i},P_{j}] =δijH+Cj,0i,\displaystyle=\delta_{ij}H+C_{j,0i}, (18)
i[J,Pi]\displaystyle i[J,P_{i}] =ϵijPj+Ci,12.\displaystyle=-\epsilon_{ij}P^{j}+C_{i,12}. (19)

The cocycle condition for the central charges is

Cμ,λν=gμνCλgμλCν,\displaystyle C_{\mu,\lambda\nu}=g_{\mu\nu}\,C_{\lambda}-g_{\mu\lambda}\,C_{\nu}, (20)
Cλ:=12gμνCμ,λν.\displaystyle C_{\lambda}:=\frac{1}{2}g^{\mu\nu}C_{\mu,\lambda\nu}. (21)

From these equations, we get

C0,0i=Ci,\displaystyle C_{0,0i}=-C_{i}, (22)
Cj,0i=δijC0,\displaystyle C_{j,0i}=-\delta_{ij}C_{0}, (23)
Ci,12=ϵijCj.\displaystyle C_{i,12}=-\epsilon_{ij}C^{j}. (24)

Thus, we can eliminate CiC_{i} and C0C_{0} by redefining Pi+CiP_{i}+C_{i} and H+C0H+C_{0} as PiP_{i} and HH, respectively. Other central charges disappear by similar redefinitions of JJ and KiK_{i}.

The choice of arbitrary additive constant in the definition of the Hamiltonian, mentioned in Sec. 2, corresponds to the elimination of the central charge C0C_{0}.

As for the setting of two parallel plates discussed in this paper, even if we eliminate the central charge in one configuration, there remains non-zero central charge in the other configuration.

4 Adiabatic process and projective representation

The Casimir energy is the difference between the vacuum energies of two different configurations, in our case L=L0L=L_{0} and L=L1L=L_{1}. The Hamiltonian of the nn-th mode scalar field given by

H(L)=d2x(L)=12d2x(π2+(ϕ)2+mn2(L)ϕ2)H(L)=\int d^{2}x\,\mathcal{H}(L)=\frac{1}{2}\int d^{2}x\left(\pi^{2}+(\nabla\phi)^{2}+{m^{2}_{n}(L)}\phi^{2}\right) (25)

has the mass parameter mn(L)=nπ/Lm_{n}(L)=n\pi/L and hence become time-dependent when connecting these two configurations.

We set the time-dependence of LL as, for example,

sT(t)=tanh(tanπt2T),\displaystyle s_{T}(t)=\tanh(\tan\frac{\pi t}{2T}), (26)
L(t)={L0(tT)1sT(t)2L0+1+sT(t)2L1(TtT)L1(Tt).\displaystyle L(t)=\begin{cases}L_{0}&(t\leq-T)\\ \displaystyle{\frac{1-s_{T}(t)}{2}}L_{0}+\displaystyle{\frac{1+s_{T}(t)}{2}}L_{1}&(-T\leq t\leq T)\\ L_{1}&(T\leq t)\end{cases}. (27)

as shown in Fig. 1.

Refer to caption
Fig. 1: Adiabatic change of the distance L(t)L(t)

In the regions tTt\leq-T and tTt\geq T, the Hamiltonian, denoted as H(L0)H(L_{0}) and H(L1)H(L_{1}) respectively, is time-independent, and hence the system is invariant under the infinitesimal Poincaré transformations.

We denote the vacuum state of H(L0)H(L_{0}) as |0L0\left|0\right\rangle_{L_{0}} and the energy eigenvalue as E0E_{0}:

H(L0)|0L0=E0|0L0.H(L_{0})\left|0\right\rangle_{L_{0}}=E_{0}\left|0\right\rangle_{L_{0}}. (28)

In the region TtT-T\leq t\leq T, the state |0L0\left|0\right\rangle_{L_{0}} is not necessarily an eigenstate of the Hamiltonian H(L)H(L). However, because the excited states of H(L)H(L) given by Eq. (25) consist of quanta with the mass mn(L)m_{n}(L), excitation energy above the ground state is greater than mn(L)>0m_{n}(L)>0. Hence we can invoke the adiabatic theorem: If we take TT large enough, then the state |0L0\left|0\right\rangle_{L_{0}} remains the ground state of H(L)H(L), which means in particular

H(L1)|0L0=E1|0L0.H(L_{1})\left|0\right\rangle_{L_{0}}=E_{1}\left|0\right\rangle_{L_{0}}. (29)

Now, we consider, in the regions tTt\leq-T and tTt\geq T, the consistency of invariance under the infinitesimal Poincaré transformations and the existence of the Casimir energy. We take the generators for the translations and the boosts as

Pi=d2x:πiϕ:\displaystyle P_{i}=\int d^{2}x\,:\pi\,\partial_{i}\phi: (30)
Ki(L)=tPid2xxi(L).\displaystyle K_{i}(L)=tP_{i}-\int d^{2}x\,x_{i}\mathcal{H}(L). (31)

The generators PiP_{i} are independent of LL and are defined by normal ordered product, while the generators H(L)H(L) given by Eq. (25) and Ki(L)K_{i}(L) are dependent on LL and hence are not normal-ordered. Straightforward calculation of the left-hand side of eq. (18) for i=ji=j shows that

i[Ki(L),Pi]=H(L)E(L),i[K_{i}(L),P_{i}]=H(L)-E(L), (32)

where E(L)E(L) is an LL-dependent constant. From eqs. (28), (29), (32), we see that, if we choose E0=E(L0)E_{0}=E(L_{0}) and E1=E(L1)E_{1}=E(L_{1}), then the translational invariance of the vacuum |0L0\left|0\right\rangle_{L_{0}}

Pi|0L0=Pi|0L1=0P_{i}\left|0\right\rangle_{L_{0}}=P_{i}\left|0\right\rangle_{L_{1}}=0

and the commutator algebra with the central charges of Poincaré generators

i[Ki(L0),Pi]=H(L0)E0\displaystyle i[K_{i}(L_{0}),P_{i}]=H(L_{0})-E_{0} (33)
i[Ki(L1),Pi]=H(L1)E1\displaystyle i[K_{i}(L_{1}),P_{i}]=H(L_{1})-E_{1} (34)

are compatible, in contrast to eq. (13).

By adding constant E0E_{0} to H(L)H(L), we could redefine H(L)H(L) so as to eliminate central charge in eq. (33), i.e. we could reproduce eq. (12) in the region tTt\leq-T. Then, in the region tTt\geq T, there remains central charge E0E1E_{0}-E_{1} in eq. (34).

5 Summary

In this paper, we have confirmed the consistency between the existence of the Casimir energy and translational invariance of the vacuum of the Poincaré invariant massless scalar field in the configuration of two parallel boundary plates. The points are:

  • Since, in the Casimir effect, comparison between the vacuum energies of two different static configuration are made, we are to consider time-dependent Hamiltonian connecting these static configurations.

  • Even if we could choose the additive constant of the Hamiltonian so as to make the representation of the Poincaré group linear (no central charge in the algebra) in the one configuration, the representation of the group become projective (nonzero central charge in the algebra) in the other.

A few comments are order. First, the additive constants such as E(L)E(L) in Eq. (32) are divergent and the discussion in this paper is formal: We should investigate the energy density (L)\mathcal{E}(L) (the eigenvalue of the Hamiltonian density (L)\mathcal{H}(L)) instead of the total energy E(L)E(L) (the eigenvalue of the Hamiltonian H(L){H}(L)). In particular, we are to consider, instead of Eq. (32), the commutator between PiP_{i} and the boost operator denisity 𝒦i(L)\mathcal{K}_{i}(L), which may suffer from the singular Schwinger terms appearing in the commutator among the components of stress tensor [9]. Second, we have focused on the nn-th mode ϕ(n)\phi^{(n)} in most of the present paper. We should sum up all of the modes and treat the resulting divergence using some regularization. Detailed study of these two points will be a subject of further research.

Acknowledgement

We thank the anonymous referee for noticing the importance of the expectation values and commutators of stress tensor and the related references. One of the authors (M. M.) thanks C. Hattori, M. Matsuda, and T. Matsuoka for discussion.

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