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dc.contributor.advisorPandit, Rahul
dc.contributor.advisorPai, Ramesh V
dc.contributor.authorKurdestany, Jamshid Moradi
dc.date.accessioned2016-09-12T07:40:50Z
dc.date.accessioned2018-07-31T06:18:38Z
dc.date.available2016-09-12T07:40:50Z
dc.date.available2018-07-31T06:18:38Z
dc.date.issued2016-09-12
dc.date.submitted2013
dc.identifier.urihttps://etd.iisc.ac.in/handle/2005/2563
dc.identifier.abstracthttp://etd.iisc.ac.in/static/etd/abstracts/3330/G25751-Abs.pdfen_US
dc.description.abstractThis thesis covers most of my work in the field of ultracold atoms loaded in optical lattices. This thesis can be divided into five different parts. In Chapter 1, after a brief introduction to the field of optical lattices I review the fundamental aspects pertaining to the physics of systems in periodic potentials and a short overview of the experiments on ultracold atoms in an optical lattice. In Chapter 2 we develop an inhomogeneous mean-field theory for the extended Bose-Hubbard model with a quadratic, confining potential. In the absence of this poten¬tial, our mean-field theory yields the phase diagram of the homogeneous extended Bose-Hubbard model. This phase diagram shows a superfluid (SF) phase and lobes of Mott-insulator(MI), density-wave(DW), and supersolid (SS) phases in the plane of the chemical potential and on-site repulsion ; we present phase diagrams for representative values of , the repulsive energy for bosons on nearest-neighbor sites. We demonstrate that, when the confining potential is present, superfluid and density-wave order parameters are nonuniform; in particular, we obtain, for a few representative values of parameters, spherical shells of SF, MI ,DW ,and SSphases. We explore the implications of our study for experiments on cold-atom dipolar con¬densates in optical lattices in a confining potential. In Chapter3 we present an extensive study of Mottinsulator( MI) and superfluid (SF) shells in Bose-Hubbard (BH) models for bosons in optical lattices with har¬monic traps. For this we develop an inhomogeneous mean-field theory. Our results for the BH model with one type of spinless bosons agrees quantitatively with quan¬tum Monte Carlo(QMC) simulations. Our approach is numerically less intensive than such simulations, so we are able to perform calculations on experimentally realistic, large three-dimensional(3D) systems, explore a wide range of parameter values, and make direct contact with a variety of experimental measurements. We also generalize our inhomogeneous mean-field theory to study BH models with har¬monic traps and(a) two species of bosons or(b) spin-1bosons. With two species of bosons we obtain rich phase diagrams with a variety of SF and MI phases and as¬sociated shells, when we include a quadratic confining potential. For the spin-1BH model we show, in a representative case, that the system can display alternating shells of polar SF and MI phases; and we make interesting predictions for experi¬ments in such systems. . In Chapter 4 we carry out an extensive study of the phase diagrams of the ex-tended Bose Hubbard model, with a mean filling of one boson per site, in one dimension by using the density matrix renormalization group and show that it contains Superfluid (SF), Mott-insulator (MI), density-wave (DW) and Haldane ¬insulator(HI) phases. We show that the critical exponents and central charge for the HI-DW,MI-HI and SF-MI transitions are consistent with those for models in the two-dimensional Ising, Gaussian, and Berezinskii-Kosterlitz-Thouless (BKT) uni¬versality classes, respectively; and we suggest that the SF-HI transition may be more exotic than a simple BKT transition. We show explicitly that different bound¬ary conditions lead to different phase diagrams.. In Chapter 5 we obtain the excitation spectra of the following three generalized of Bose-Hubbard(BH) models:(1) a two-species generalization of the spinless BH model, (2) a single-species, spin-1 BH model, and (3) the extended Bose-Hubbard model (EBH) for spinless interacting bosons of one species. In all the phases of these models we show how to obtain excitation spectra by using the random phase approximation (RPA). We compare the results of our work with earlier studies of related models and discuss implications for experiments.en_US
dc.language.isoen_USen_US
dc.relation.ispartofseriesG25751en_US
dc.subjectUltracold Atomsen_US
dc.subjectOptical Latticesen_US
dc.subjectSuperfluid Phasesen_US
dc.subjectBose-Hubbard Modelen_US
dc.subjectMean-Field Theoryen_US
dc.subjectSupersolid Phasesen_US
dc.subjectMott-Insulator Phasesen_US
dc.subjectBosonsen_US
dc.subjectBose-Einstein Condensationen_US
dc.subjectDensity-Wave Phasesen_US
dc.subjectPhase Diagramsen_US
dc.subjectRandom-Phase-Approximation (RPA)en_US
dc.subjectSuperfluid-Haldane Insulator Transitionen_US
dc.subjectQuantum Phase Transitionen_US
dc.subjectRandom Phase Approximationen_US
dc.subjectPhase Transitionsen_US
dc.subjectSuperfluid-Mott-Insulator Transitionen_US
dc.subjectBose-Hubbard Modelsen_US
dc.subject.classificationCondensed Matter Physicsen_US
dc.titlePhases, Transitions, Patterns, And Excitations In Generalized Bose-Hubbard Modelsen_US
dc.typeThesisen_US
dc.degree.namePhDen_US
dc.degree.levelDoctoralen_US
dc.degree.disciplineFaculty of Scienceen_US


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