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— journal of February 2015

physics pp. 309–316

Distribution of level spacing ratios using one- plus two-body random matrix ensembles

N D CHAVDA

Applied Physics Department, Faculty of Technology and Engineering, Maharaja Sayajirao University of Baroda, Vadodara 390 001, India E-mail: ndchavda-apphy@msubaroda.ac.in

DOI: 10.1007/s12043-015-0933-8; ePublication: 3 February 2015

Abstract. Probability distribution (P (r)) of the level spacing ratios has been introduced recently and is used to investigate many-body localization as well as to quantify the distance from inte- grability on finite size lattices. In this paper, we study the distribution of the ratio of consecutive level spacings using one-body plus two-body random matrix ensembles for finite interacting many- fermion and many-boson systems.P (r)for these ensembles move steadily from the Poisson to the Gaussian orthogonal ensemble (GOE) form as the two-body interaction strengthλis varied. Other related quantities are also used in the analysis to obtain critical strengthλcfor the transition. The λcvalues deduced using theP (r)analysis are in good agreement with the results obtained using the nearest neighbour spacing distribution (NNSD) analysis.

Keywords. Random matrix ensembles; embedded ensembles; EGOE(1+2); BEGOE(1+2);

Poisson–GOE transition; spacing distribution.

PACS Nos 05.45.Mt; 05.40.−a; 05.30.Fk; 05.30.Jp

1. Introduction

Random matrix theory (RMT) introduced to describe statistical properties of the energy levels of complex nuclei has seen tremendous growth recently [1]. It is now well rec- ognized that, the quantum system whose classical counterpart is chaotic, will follow one of the three classical random matrix ensembles, namely, the Gaussian orthogonal ensemble (GOE), Gaussian unitary ensemble (GUE) and Gaussian symplectic ensem- ble (GSE) ensemble, depending on the symmetries of the Hamiltonian [2]. In quantum domain, the NNSDP (S)dS giving a degree of level repulsion is one of the important measures in the study of level statistics. It is well known that if the system is in integrable domain, corresponding to the regular behaviour of the system, then the NNSD is Poisson (P (S)=exp(−S))in character [3], while in the chaotic domain it has the characteristic shape described by the Wigner surmiseP (S)=(π/2)Sexp(−π S2/4)[4]. It is interesting to note that the non-integrability (even in absence of chaos) is also a cause for level

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repulsion. For instance, in plane polygonal billiards, the spacing distribution shows level repulsion [5]. Furthermore, explicit forms for level spacing distribution functions are known for the universality class where parity and time reversal symmetries are broken.

These systems also exhibit level repulsion [6].

For a given set of energy levels, construction of NNSD requires unfolding of the energy spectrum to remove the variation in the density of eigenvalues [2,7]. Recently, Oganesyan and Huse [8] considered the probability distributionP (r)dr of the ratio of consecutive level spacings of the energy levels which does not require unfolding as it is independent of the shape of the eigenstate density. The statistics of ratios of successive spacings was used to quantify the distance from integrability on finite size lattices [9–11] and to numer- ically investigate many-body localization [8,12–14]. The expressions for the probability distribution of the ratio of two consecutive level spacings for the classical GOE, GUE and GSE ensembles of random matrices are derived in [15]. They are used in the study of spectral correlations in diffuse van der Waals clusters [16] and also to confirm, using embedded Gaussian orthogonal ensemble (EGOE) of one- plus random two-body matrix ensembles, that the finite many-particle quantum systems with strong enough interactions follow GOE [17].

The EGOE of one- plus random two-body matrix ensembles form generic models for finite isolated interacting many-fermion systems (denoted by EGOE(1+2)) (for boson systems, these are called BEGOE(1+2) with B for bosons) and they model what one may call quantum many-body chaos [1,18]. In the past, it is shown that as the strength of two-body interaction (λ) increases, both in EGOE(1+2) and in BEGOE(1+2), there is a transition from Poisson to GOE in the level fluctuations atλ =λc[18–20]. The NNSD shows Poisson character in general for very small values ofλdue to the presence of many good quantum numbers defined by the one-body part. As the strength of the two-body interaction increases, there is delocalization in the Fock space and hence one expects GOE behaviour for largeλvalues. Going beyond the work done in [17], the distribution of the consecutive level spacing ratios to demonstrate Poisson to GOE transition using these ensembles is studied.

This paper is organized as follows: in §2, analytical results for Poisson and GOE for the probability distribution of the ratio of consecutive level spacings and related averages are briefly discussed. The EGOE(1+2) and BEGOE(1+2) used in the present analysis are described in §3. The numerical results of the probability distribution for the ratio of consecutive level spacings and the related averages showing Poisson to GOE transition by varying the two-body interaction strength, in EGOE(1+2) as well as in BEGOE(1+2), are presented in §4. Finally, concluding remarks are given in §5.

2. Probability distribution of the ratio of consecutive level spacings

Let us consider an ordered set of eigenvalues (energy levels)en, wheren = 1,2, ..., d.

The nearest-neighbour spacing is given bysn =en+1en. Then, the ratio of two con- secutive level spacings isrn=sn+1/sn. If a system is in the integrable domain, then the NNSD is Poisson andP (r)is (denoted byPP(r)),

PP(r)= 1

(1+r)2. (1)

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Similarly, for GOE, derived using a 3×3 real symmetric matrices,P (r)is given by Wigner-like surmise [15],

PW(r)= 27 8

r+r2

(1+r+r2)5/2. (2)

In addition torn, Oganesyan and Huse [8] considered the distribution of the ratiosr˜n

defined by

˜

rn= min(sn, sn−1)

max(sn, sn1) =min(rn,1/rn). (3)

For uncorrelated Poisson spectrum, the probability distribution ofr˜nis PP(r)˜ = 2

(1+ ˜r)2. (4)

As the ratiosrnandr˜nare independent of the local density of states, unfolding is not required for the probability distributions ofP (r)andP (r). As shown in [15], it is possible˜ to deriveP (r)˜ for a givenP (r). With the help of eq. (1), the average value ofrfor Poisson is given byrP= ∞, while for GOE using eq. (2) it isrGOE =1.75. However, average value ofr˜(denoted by˜r), is˜rGOE =0.536 for GOE and˜rP = 0.386 for Poisson.

In this study, we have usedP (r),P (r),˜ rand˜rin the analysis of the energy levels of embedded ensembles and the results are presented in §4.

3. Embedded ensembles for fermion and boson systems

Consider m spin-less fermions (bosons) occupying N single-particle states, with the Hamiltonian (H) matrix in two-particle spaces represented by GOE and then construct- ing the many-particle H matrix, with them-particle basis states being direct products of single-particle states, gives the EGOE of two-body interactions [EGOE(2)] in m- particle space [18]. Similarly, for interacting spin-less boson systems, they are denoted by BEGOE(2) [21]. Addition of the mean-field one-body part gives EGOE(1+2) and BEGOE(1+2) for fermion and boson systems, respectively [18,19] and the Hamiltonian H =h(1)+λ{V (2)}. Here,h(1)is the mean-field one-body part defined by the single- particle energiesi and{V (2)}represents EGOE(2) or BEGOE(2), i.e.,V (2)matrix in two-particle spaces is represented by GOE with matrix elements having zero mean and unit variance. Note that,{ }denotes the ensemble. The parameterλis the strength of the two-body interaction in units of average spacingof the single-particle states. The actual construction ofm-particle HamiltonianHis straightforward and is described completely in [18,19]. In this analysis, we have considered the following two examples:

(1) EGOE(1+2) form=6 fermions inN =14 single-particle states withHmatrix of dimension 3003 (see [18] for details).

(2) BEGOE(1+2) form=10 bosons inN =5 single-particle states withHmatrix of dimension 1001 (see [19,20] for details).

In all the calculations, single-particle energies are drawn from the centre of a GOE. Both the ensembles considered in this analysis have 100 members and the numerical results are presented in the following section.

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4. Results and discussions

Figure 1a shows theP (r)distribution histograms obtained for EGOE(1+2) for various values ofλ. Each histogram is superimposed by Poisson and Wigner predictions given in eqs (1) and (2), respectively. Here bin size 0.1 is used to construct P (r)histograms.

Figure 1. Histograms represent (a)P (r)distribution and (b)P (r)˜ distribution for a 100-member EGOE(1+2) ensemble withm=6 fermions inN =14 single-particle states for various values of two-body interaction strengthλ. Ensemble-averaged values ofr(r) andr˜(˜r) are also given in the figure. Bin sizes of 0.1 and 0.05 are used for P (r)andP (˜r), respectively. The chaos markerλc=0.018 corresponds to˜r =0.5.

The last histogram in both (a) and (b) is for EGOE(2). EGOE results are compared with Poisson (blue dash curve) and GOE (red dash curve) predictions.

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Ensemble-averaged values of r (r) are also given in the figure. In the absence of interaction, one-body part of the Hamiltonian is integrable and level distribution is therefore Poissonian giving ensemble-averaged ratio of consecutive level spacings r = ∞. When the two-body interaction strengthλincreases, the eigenstates spread over all the basis states leading to complete mixing of the basis states. Hence, one expects

Figure 2. Histograms represent (a)P (r)distribution and (b)P (r)˜ distribution for a 100-member BEGOE(1+2) ensemble withm=10 bosons inN =5 single-particle states for various values of two-body interaction strengthλ. Ensemble-averaged values ofr(r) andr˜(˜r) are also given in the figure. Bin sizes of 0.1 and 0.05 are used for P (r)andP (˜r), respectively. The chaos markerλc=0.024 corresponds to˜r =0.5.

The last histogram in both (a) and (b) is for BEGOE(2). BEGOE results are compared with Poisson (blue dash curve) and GOE (red dash curve) predictions.

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Figure 3. Ensemble-averaged values ofr, denoted asr(a) andr, denoted as˜ ˜r (b), as a function of two-body interaction strengthλ, calculated using 100-member ensemble for EGOE(1+2) ensemble with(m, N )= (6,14). The vertical dash-line represents the position ofλc. Hereλc∼0.018.

level repulsion givingrclose to GOE for largeλvalues. Figure 1a clearly displays the transition ofP (r)from the Poisson character for low values ofλto the GOE character as the strength of the two-body interaction is slowly increased by increasingλ. Simi- larly, figure 1b represents results forP (r)˜ distribution. Each histogram is superimposed by Poisson prediction given by eq. (4). The GOE probability distribution shown in each histogram of figure 1b is obtained using a 500-member 1000×1000 GOE random matrix.

For constructingP (r)˜ histograms, bin size=0.05 is used. Ensemble-averaged values of

˜

rr) are also given in the figure. The results in figure 1b are consistent with that of figure 1a and it clearly shows the transition from Poisson to GOE inP (r)˜ as the strength of the two-body interactionλincreases. The last histogram in figures 1a and 1b is for EGOE(2). Figure 2 representsP (r)andP (r)˜ results for BEGOE(1+2). The results are consistent with that of EGOE(1+2) results.

Figure 4. Ensemble-averaged values ofr, denoted asr(a) andr, denoted as˜ ˜r (b), as a function of two-body interaction strengthλ, calculated using 100-member ensemble for BEGOE(1+2) ensemble with(m, N )=(10,5). The vertical dash-line represents the position ofλc. Hereλc∼0.024.

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Further, figures 3 and 4 show values ofrand˜r, as a function of two-body interaction strengthλ, for EGOE(1+2) and BEGOE(1+2), respectively. The horizontal lines in the figures represent Poisson and GOE estimates. The results in figures 3 and 4 clearly display the transition from Poisson to GOE in terms ofrand˜ras the strength of the two-body interaction slowly increases. Similar results are obtained using lattice models in [13,14].

Recently, the Poisson-to-GOE transition was studied in terms of the distribution of ratio of consecutive level spacings by constructing 3×3 random matrix model [11]. This model involves a transition parameter. The critical value ofc ∼0.3 gives the onset of GOE fluctuations. Withc ∼ 0.3, we haver ∼ 2 and ˜r ∼ 0.5. The critical value of two-body interaction strength isλc = 0.018 for EGOE(1+2) andλc = 0.024 for BEGOE(1+2). This is shown by vertical lines in figures 3 and 4. Theλc values obtained for the examples considered in this study are consistent with the previous results [19,20,22].

5. Conclusions

In this work, using EGOE(1+2) and BEGOE(1+2), we have demonstrated that the prob- ability distributionP (r)of the ratio of consecutive level spacings for embedded random matrix ensembles moves steadily from Poisson-type to the GOE-type, asλ, the strength of the two-body interaction, is increased. Furthermore, we have defined the value of the critical strength parameterλcusing the criterion given in [11]. Theλc values deduced usingP (r)and that obtained in the past using the NNSD analysis are found to be in good agreement.

Acknowledgements

The author thanks V K B Kota and V Potbhare for useful discussions and also acknowl- edges support from the University Grants Commission, New Delhi (India) (Grant No.

F.40-425/2011(SR)).

References

[1] V K B Kota, Embedded random matrix ensembles in quantum physics, Lecture Notes in Physics (Springer, Heidelberg, 2014) Vol. 884

[2] F Haake, Quantum signatures of chaos, 3rd Edn (Springer-Verlag, Heidelberg, 2010) [3] M V Berry and M Tabor, Proc. R. Soc. (London) A 356, 375 (1977)

[4] O Bohigas, M-J Giannoni and C Schmit, Phys. Rev. Lett. 52, 1 (1984) [5] B Gremaud and S R Jain, J. Phys. A 31, L637 (1998)

[6] Z Ahmed and S R Jain, Phys. Rev. E 67, 045106 (2003); J. Phys. A 36, 3349 (2003) [7] T A Brody, J Flores, J B French, P A Mello, A Pandey and S S M Wong, Rev. Mod. Phys. 53,

385 (1981)

[8] V Oganesyan and D A Huse, Phys. Rev. B 75, 155111 (2007)

[9] C Kollath, G Roux, G Biroli and A M Läuchli, J. Stat. Mech. P08011 (2010) [10] M Collura, H Aufderheide, G Roux and D Karevski, Phys. Rev. A 86, 013615 (2012)

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[11] N D Chavda, H N Deota and V K B Kota, Phys. Lett. A 378, 3012 (2014) [12] V Oganesyan, A Pal and D A Huse, Phys. Rev. B 80, 115104 (2009) [13] A Pal and D A Huse, Phys. Rev. B 82, 174411 (2010)

[14] S Iyer, V Oganesyan, G Refael and D A Huse, Phys. Rev. B 87, 134202 (2013) [15] Y Y Atas, E Bogomolny, O Giraud and G Roux, Phys. Rev. Lett. 110, 084101 (2013) [16] S K Haldar, B Chakrabarti, N D Chavda, T K Das, S Canuto and V K B Kota, Phys. Rev. A

89, 043607 (2014)

[17] N D Chavda and V K B Kota, Phys. Lett. A 377, 3009 (2013) [18] V K B Kota, Phys. Rep. 347, 223 (2001)

[19] N D Chavda, V Potbhare and V K B Kota, Phys. Lett. A 311, 331 (2003) [20] N D Chavda, V K B Kota and V Potbhare, Phys. Lett. A 376, 2972 (2012)

[21] T Asaga, L Benet, T Rupp and H A Weidenmüller, Ann. Phys. (N.Y.) 298, 229 (2002) [22] V K B Kota, A Relaño, J Retamosa and M Vyas, J. Stat. Mech. P10028, 1 (2011)

References

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