Research Article | Open Access

Thiago PrudĂȘncio, "Kaluza-Klein State in Bekenstein-Hawking Entropy Cycles", *Advances in Mathematical Physics*, vol. 2019, Article ID 9051968, 7 pages, 2019. https://doi.org/10.1155/2019/9051968

# Kaluza-Klein State in Bekenstein-Hawking Entropy Cycles

**Academic Editor:**Antonio Scarfone

#### Abstract

A Kaluza-Klein state configuration in black-hole qubit correspondence (BHQC) is considered in cyclic cycles of its Bekenstein-Hawking entropy. After a sequence of Peccei-Quinn transformations on the Kaluza-Klein state in cyclic cycles alternating between large and small extremal black hole (EBH) configurations, we obtain the corresponding amount of variation in the initial Bekenstein-Hawking entropy in cyclic cycles. We consider different cases where the EBH state alternates between small and large states. We then demonstrate that the total Bekenstein-Hawking entropy increases in these processes.

#### 1. Introduction

An important class of extremal black holes (EBHs) is the special cases of black holes that cease evaporation due the presence of supersymmetric bounds [1â3]. The consequence of the bounds is to create a relation between the mass of the EBHs and their electric and magnetic charges [4, 5]. In the final state, the EBH can be described completely by their magnetic and electric charges and consequently is independent of the scalar fields that describe the nonstationary states [2]. A consequence is that a mapping with a Hilbert space can be done with the symmetries mapped on classes of entanglement, as a black hole qubit correspondence (BHQC) [6â9].

In recent years the BHQC of EBHs have been studied relating the entanglement classes with groups associated with string theories that lead to a description of the stationary states of EBHs, when the Hawking radiation is stopped and the state of the EBH is described completely in terms of their electric and magnetic charges [1].

Different configurations of EBH have been classified and the BHQC allows the classification of different configurations according to the entanglement class the EBH belongs. In particular, the association with qubits and the realization of quantum information protocols. An important advance in this field is the BHQC connection with quantum circuit protocols [10].

Recently these class of operations on a EBH state where investigated by means of Peccei-Quinn (PQ) transformations [11]. These classes of operations on an EBH state can be associated on a BHQC to operators that does not change the magnetic charges of an EBH state. These transformations produce changes in the Bekenstein-Hawking entropy [12, 13].

Here we investigate the class of Kaluza-Klein EBHs under the action of PQ operators in cycles alternating between large and small EBH configurations associated with their Bekenstein-Hawking entropy. The cases analyzed are transitions at fixed entropy and transitions at increasing or decreasing entropy. We consider different possible combinations where we finally compute the total amount of entropy exchange in the cycles. In the BHQC scenario this means it evolves as a set of gate operations applied in such a way to achieve cycles in EBH state configuration.

The paper is organized as follows: in Sections 2 and 3, some aspects of BHQC that will be applied in the next sections are revised; in Section 4, the relation between Bekenstein-Hawking entropy and the -invariant is discussed; in Section 5 the Kaluza-Klein (KK) state configurations in small and large configurations of EBH are discussed; in Section 6, operations on EBH charge states are discussed; in Section 7, the protocols of cyclic cycles of Bekenstein-Hawking entropy in KK EBH configurations are implemented; in Section 8, conclusions remarks are addressed.

#### 2. BHQC

BHQC has been established a bridge between certain solutions of black holes and quantum information theory (QIT). This correspondence allows the problem of classification of EBHs be associated with the classification of entanglement classes in QIT systems. The Bekenstein-Hawking entropy is in a class of black hole solutions in string theory and classes of multipartite entanglement measures associated in BHQC. The correspondence can also shed new light on the way EBHs evolve under certain QIT conditions [6, 10].

#### 3. BHQC States

In the BHQC realization, a general dyonic charge vector state is given by the superposition of typewhere a Fock basis is used as the symplectic basis of the Hilbert space associated with the electric and magnetic charges of the EBH. For convenience, the even states are associated with the magnetic charge configurations and the odd states to the electric charge configurations of the EBH. The dimension is associated with the number of vector multiplets .

A BHQC of Peccei-Quinn (PQ) symplectic transformation on the charge state is given by the action of the corresponding operator on the charge state being given by and has the following explicit expression:where the coefficients allows to a Peccei-Quinn group, [11], whose invariants are of the formwith the identity and the null matrices, where the submatrices with are defined as a real matrix (, ).

As a consequence, PQ operators leave the EBH magnetic charges invariant,while changing the electric charges

#### 4. Bekenstein-Hawking Entropy and the -Invariant

A general EBH charge state configuration (1) is associated with a unique -invariant: where the cubic invariants are given by and the Poisson brackets are defined as

The Bekenstein-Hawking entropy formula for a general EBH state is given in terms of this invariant as [6]

#### 5. Large and Small Kaluza-Klein EBH Configurations

We say that the EBH configuration is large if and the EBH is small if instead An important type of EBH configuration particularly to BHQC due to the form correspondence with a qubit is a Kaluza-Klein EBH configuration.

A Kaluza-Klein (KK) EBH state configuration is given by the following state in BHQC: The KK invariant is given by where It follows that the Bekenstein-Hawking formula for a general EBH configuration of a Kaluza-Klein type is In the case with both and nonvanishing, one obtains a dyonic large EBH configuration, corresponding to the maximal rank element in the related Freudenthal Triple System [11].

If some of or vanish, one has a small EBH configuration, since in this case These cases are given by corresponding pure states and .

#### 6. Operations on EBH Charge States

After a PQ transformation, the Kaluza-Klein state dyonic EBH state acquires a superposition of change states This will alter the Bekenstein-Hawking EBH entropy. The state is written And the invariants are given by We can define the constant of the PQ transformation such that the quartic invariant is given by

Consequently, the Bekestein-Hawking entropy is written in the form A large EBH is achieved for , while the set of small EBHs after the transformation satisfy ; consequently In this case, two possible solutions are found

#### 7. Cyclic Cycles of Bekenstein-Hawking Entropy in Kaluza-Klein EBH Configurations

In order to consider a cyclic cycle of Kaluza-Klein EBH states, we consider a set of PQ operations as a BHQC quantum circuit in different protocols alternating small and large EBH configurations.

##### 7.1. Alternating Small and Large Kaluza-Klein EBH Configurations

We consider the interchange between large and small Kaluza-Klein EBH configurations obeying the following protocol (see Figure 1): We start with a Kaluza-Klein state where and , whose Bekenstein-Hawking entropy is given by The PQ symplectic transformation on this EBH configuration will lead toWe can consider the case where the transformation leaves the configuration in a Kaluza-Klein state but converts the EBH in a small configuration. This will occur under the condition Consequently, we will have which is small The second transformation will leave the state in the following charge configuration: where the simplest case is taken and again we put the state in a Kaluza-Klein configurationThis is then a large EBH with a Bekenstein-Hawking entropy given by Again, we apply a PQ symplectic transformation on this EBH configuration, and we are left in the following state: We now have that the small configuration implies And the state that is, a small EBH configuration Finally, the cyclic transformation is achieved by the transformation where we keep the Kaluza-Klein configuration with and The condition will lead to The whole cyclic transformation is then realized under the conditions In this case the Kaluza-Klein EBH states are alternating between large and small configurations.

The set of variations of Bekenstein-Hawking entropies in each step are given by It follows that the whole process has a total increasing entropy Considering a more general scenario where the final configuration is given by we have the total entropy in the process given by It follows that, after cycles, the entropy will suffer the total variation obeying the following relation: where is the proportionality of last cycle step in each cycle. The perfect case is ,

##### 7.2. Cycle with Sections of Small and Large EBH Configurations

We can also consider the following protocol (see Figure 2): where now the operation does not change the entropy. Starting again with the Kaluza-Klein state with and , whose Bekenstein-Hawking entropy is given by The PQ transformation will lead to Staying in a Kaluza-Klein configuration implies that which will lead to the following state In this case, the Bekenstein-Hawking entropy is given by Taking the case , we can write The PQ transformation on this state will now lead to the following: In this case, we have the relations such that the Kaluza-Klein state is reduced to and the EBH has a small configuration We then have the next transformation Since in this case we also have a small EBH configuration, This will lead to the EBH state This is finally after the transformation whocj will lead to and we have The Bekenstein-Hawking entropy in this case is The cyclic condition imposes the relation The variations of Bekenstein-Hawking entropy in each step are given by The total entropy variation is given by and consequently it has increased.

In a more general case This leads to In cycles, the total entropy variation is given by In particular, for , The Bekenstein-Hawking entropy after cycles is then an increasing quantity.

#### 8. Concluding Remarks

Within the black-hole/qubit correspondence (BHQC), we considered the Bekenstein-Hawking entropy variation in cyclic cycles, where PecceiâQuinn (PQ) symplectic transformations are used on the transitions between EBH state configurations. We considered the cases where the entropy is alternating between small and large configurations and the situation where the transitions occur in fixed small or large configurations. We showed applying BHQC that the total Bekenstein-Hawking entropy in each state increases. This is in complete agreement with area theorem [12, 14]. As a consequence, the cyclic transport of a qubit like state in BHQC leads to an increasing variation of the corresponding total Bekenstein-Hawking entropy.

As a consequence, a sequence of gate operations in a KK state in a cyclic cycle with the initial state as a target state implies increasing of the total Bekenstein-Hawking entropy, in agreement with the expected in the thermodynamics of black holes, implying that such a scenario can be implemented physically under a cost of increasing entropy.

#### Data Availability

The data used to support the findings of this study are included within the article.

#### Conflicts of Interest

The author declares there are no conflicts of interest in this paper.

#### Acknowledgments

This work is supported by the projects APCINTER-00273/14-FAPEMA (Brazil), FundaĂ§ĂŁo de Amparo Ă Pesquisa e Desenvolvimento CientĂfico e TecnolĂłgico do MaranhĂŁo (FAPEMA), Grant UNIVERSAL-01401/16-FAPEMA (Brazil), and Conselho Nacional de Desenvolvimento CientĂfico e TecnolĂłgico (CNPq), Grant UNIVERSAL-432929/2016-9-CNPq (Brazil).

#### References

- R. Kallosh, A. Linde, T. OrtĂn, A. Peet, and A. Van Proeyen, âSupersymmetry as a cosmic censor,â
*Physical Review D: Particles, Fields, Gravitation and Cosmology*, vol. 46, no. 12, pp. 5278â5302, 1992. View at: Publisher Site | Google Scholar | MathSciNet - S. Ferrara, R. Kallosh, and A. Strominger, âN=2 extremal black holes,â
*Physical Review D: Particles, Fields, Gravitation and Cosmology*, vol. 52, no. 10, pp. R5412âR5416, 1995. View at: Publisher Site | Google Scholar - A. Strominger, âMacroscopic entropy of extremal black holes,â
*Physics Letters. B. Particle Physics, Nuclear Physics and Cosmology*, vol. 383, no. 1, pp. 39â43, 1996. View at: Publisher Site | Google Scholar | MathSciNet - S. Ferrara and R. Kallosh, âSupersymmetry and attractors,â
*Physical Review D: Particles, Fields, Gravitation and Cosmology*, vol. 54, no. 2, pp. 1514â1524, 1996. View at: Publisher Site | Google Scholar - S. Ferrara and R. Kallosh, âUniversity of supersymmetric attractors,â
*Physical Review D: Particles, Fields, Gravitation and Cosmology*, vol. 54, no. 2, pp. 1525â1534, 1996. View at: Publisher Site | Google Scholar - L. Borsten, M. J. Duff, and P. Levay, âThe black-hole/qubit correspondence: an up-to-date review,â
*Classical and Quantum Gravity*, vol. 29, no. 22, 224008, 80 pages, 2012. View at: Publisher Site | Google Scholar | MathSciNet - R. Kallosh and A. Linde, âStrings, black holes, and quantum information,â
*Physical Review D: Particles, Fields, Gravitation and Cosmology*, vol. 73, no. 10, Article ID 104033, 2006. View at: Publisher Site | Google Scholar - L. Borsten, D. Dahanayake, M. J. Duff, A. Marrani, and W. Rubens, âFour-Qubit Entanglement Classification from String Theory,â
*Physical Review Letters*, vol. 105, no. 10, Article ID 100507, 2010. View at: Publisher Site | Google Scholar - P. LĂ©vay, âQubits from extra dimensions,â
*Physical Review D: Particles, Fields, Gravitation and Cosmology*, vol. 84, no. 12, Article ID 125020, 2011. View at: Publisher Site | Google Scholar - T. PrudĂȘncio, D. J. Cirilo-Lombardo, E. O. Silva, and H. Belich, âBlack hole qubit correspondence from quantum circuits,â
*Modern Physics Letters A*, vol. 30, no. 23, p. 1550104, 2015. View at: Publisher Site | Google Scholar - T. PrudĂȘncio, A. Marrani, and D. Cirilo-Lombardo, âPecceiâQuinn Transformations and Black Holes: Orbit Transmutations and Entanglement Generation,â
*Universe*, vol. 3, no. 1, p. 12, 2017. View at: Publisher Site | Google Scholar - S. W. Hawking, âGravitational radiation from colliding black holes,â
*Physical Review Letters*, vol. 26, no. 21, pp. 1344â1346, 1971. View at: Publisher Site | Google Scholar - J. D. Bekenstein, âBlack holes and entropy,â
*Physical Review D: Particles, Fields, Gravitation and Cosmology*, vol. 7, pp. 2333â2346, 1973. View at: Publisher Site | Google Scholar | MathSciNet - D. N. Page, âHawking radiation and black hole thermodynamics,â
*New Journal of Physics*, vol. 7, pp. 203.1â203.32, 2005. View at: Publisher Site | Google Scholar | MathSciNet

#### Copyright

Copyright © 2019 Thiago Prudêncio. This is an open access article distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.