Thermodynamics and excitations of Coulomb glass Vikas Malik and Deepak Kumar School of Physical Sciences, Jawaharlal Nehru University, New Delhi 110 067, India Received 13 March 2007; revised manuscript received 7 June 2007; published 24 September 2007 We have calculated the phase diagram and density of states of single-particle excitations of a lattice model of the Coulomb glass. We employ the replica method to average over disorder and then use linked-cluster expansion to obtain the free energy in the random phase approximation. We find that the system has a transition to an antiferromagnetic phase below a critical disorder. Above the critical disorder, the system has a glassy “independent spin phase” at zero temperature which crosses over to paramagnetic phase as the temperature is increased. In the antiferromagnetic phase, the single-particle excitation density density of states DOS has a feature including the gap at the Fermi level due to long-range order. To obtain DOS in the glassy phase, we analyze cavity-field equations for local magnetization occupation. We obtain DOS at nonzero temperatures and find that with temperature the DOS at the Fermi level increases quadratically and the Coulomb gap decreases linearly. DOI: 10.1103/PhysRevB.76.125207 PACS numbers: 71.23.An, 73.20.Qt, 72.80.Ng I. INTRODUCTION The Coulomb glass has been a problem of long standing interest as it involves a very interesting interplay of disorder and Coulomb interactions. The initial interest in the problem lies in describing the hopping transport in bands where the electronic states are localized around Fermi level as is ob- tained in doped, compensated semiconductors 1 at sufficiently low temperatures. It was recognized early by Pollak 2,3 and Srinivasan 4 that in such systems, Coulomb interactions play a crucial role: they cause a depletion in the single-particle density of states around the Fermi level. Efros and Shk- lovskii ESmade these arguments more precise by invoking stability considerations of the ground state to show that this depletion is actually a soft gap, now known as Coulomb gap, with a density of states having the form g- d-1 , where is the chemical potential and d is the dimension of the system. 5,6 They also pointed out its very significant effect on conduction in the variable range hopping VRHregime. The concept of VRH was introduced earlier by Mott, 7,8 who argued that when the temperatures become too low to permit nearest neighbor hopping, the electrons optimize between the hop distance and the activation energy, which results in the temperature dependence of conductivity of the form exp-T M / T 1/4 . Efros and Shklovskii 5 showed that interac- tions between electrons would cause a qualitative change in the temperature dependence of conductance to the form exp-T ES / T 1/2 due to the presence of the soft Coulomb gap. A large number of experimental studies of conduction have been made in the VRH regime examining the above temperature dependences and the crossover between them. 1,9 Recently, experimental studies have focused on other as- pects of the dynamical behavior of Coulomb glasses. 1014 In studies by Ovadyahu and co-workers, 1012 the relaxation of conductivity is measured after carrier concentration of the sample has been changed by field effect or photoexcitation. The decay of excess conductivity is found to be logarithmi- cally slow and shows aging effects typical of glasses at low temperatures. Another set of experiments which point toward strong correlation effects in these system is due to Massey and Lee, 13 who by combining tunneling conduction studies with bulk conduction behavior argue that the Coulomb gap is significantly lower than Efros-Shklovskii prediction, imply- ing a role for multielectron excitations. Tunneling studies of Sandow et al. 14 suggest strong correlation effects by showing large departures from ES form of density of states. In the last three decades or so, there have been numerous numerical and analytical studies to explore various transport and thermodynamic properties of Coulomb glasses. 1530 Par- ticular attention has been focused on the numerical compu- tation of the density of states DOSfor the single-particle excitation. While all the studies find the gap, there are dif- ferences regarding the form of the gap in various numerical studies. 16,3134 Many studies agree with the ES prediction, but other studies find results which are either lower or higher than these values. A main problem of the numerical calcula- tions is that the system has a complex energy landscape with innumerable metastable states, which makes it difficult to reach the ground state. To relax from a metastable state to another one typically needs multielectron excitations, for which the phase space is too large to tackle numerically. The metastable states also exhibit the Coulomb gap features, 33 but a clear power law over the full energy range is not seen in these studies. The finite-size effects are particularly strong for low energies. 33 Most of the theoretical studies have been done on a lattice model, first discussed by Efros. 6 In this model, the electron states are assumed to be localized around centers placed on a regular lattice of N s sites. When the number of electrons N is N s /2, the Hamiltonian of the system is taken to be H = i i n i + 1 2 ij e 2 |r i - r j | n i - 1/2n j - 1/2, 1 where n i and i denote the electron occupation number and the energy of the localized state at site i, respectively. The variable n i takes values 0 and 1, as the typical on-site Cou- lomb energy is too large to permit more than one electron per site. The site energies are taken to be independent random variables with a site-independent probability distribution PHYSICAL REVIEW B 76, 125207 2007 1098-0121/2007/7612/1252079©2007 The American Physical Society 125207-1