Studies in Loop Quantization of cosmological models (Record no. 48810)
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fixed length control field | 02033nam a2200241Ia 4500 |
008 - FIXED-LENGTH DATA ELEMENTS--GENERAL INFORMATION | |
fixed length control field | 160627s2009||||xx |||||||||||||| ||und|| |
080 ## - UNIVERSAL DECIMAL CLASSIFICATION NUMBER | |
Universal Decimal Classification number | HBNI Th-9 |
100 ## - MAIN ENTRY--AUTHOR NAME | |
Personal name | Kinjal Banerjee |
Relator term | author |
245 ## - TITLE STATEMENT | |
Title | Studies in Loop Quantization of cosmological models |
260 ## - PUBLICATION, DISTRIBUTION, ETC. (IMPRINT) | |
Year of publication | 2009 |
300 ## - PHYSICAL DESCRIPTION | |
Number of Pages | ix; 84p. |
502 ## - DISSERTATION NOTE | |
Dissertation note | 2009 |
502 ## - DISSERTATION NOTE | |
Degree Type | Ph.D |
502 ## - DISSERTATION NOTE | |
Name of granting institution | HBNI |
520 3# - SUMMARY, ETC. | |
Summary, etc | This thesis presents some studies on the Loop Quantization of cosmological models. The effect of loop quantization of FRW cosmology in the context of effective equations and WKB approximation are studied in the first part of the thesis. The initial steps undertaken in the second part, in construction of 'A Loop Quantized theory' of a midi-superspace model known as the Gowdy Model on T^3. One of the qualitatively distinct and robust implication of Loop Quantum Gravity - the underlying discrete structure is manifested by the Hamiltonian Constraint Equation, in the cosmological context elucidated by Loop Quantum Cosmology. An alternative derivation of the effective Hamiltonian is presented, by-passing the continuum approximation step. The Kinematical Hilbert Space is introduced on which the appropriate holonomies and fluxes are well represented. The quantization of the volume operator and the Gauss constraint is straightforward. Imposition of the Gauss constraint can be done on the Kinematical Hilbert Space to select subspace of gauge invariant states. The quantization of the Hamiltonian constraint is carried out, making specific choices. Alternative choices are briefly discussed. It appears that to get spatial correlations reflected in the Hamiltonian constraint, one may have to adopt the so called 'effective operator view point'. |
650 14 - SUBJECT ADDED ENTRY--TOPICAL TERM | |
Topical Term | Physics |
653 10 - INDEX TERM--UNCONTROLLED | |
Uncontrolled term | Loop Quantum Cosmology |
653 10 - INDEX TERM--UNCONTROLLED | |
Uncontrolled term | Loop Quantum Gravity |
720 1# - ADDED ENTRY--UNCONTROLLED NAME | |
Thesis Advisor | Ghanashyam Date |
Relator term | Thesis advisor [ths] |
856 ## - ELECTRONIC LOCATION AND ACCESS | |
Uniform Resource Identifier | http://www.imsc.res.in/xmlui/handle/123456789/122 |
942 ## - ADDED ENTRY ELEMENTS (KOHA) | |
Koha item type | THESIS & DISSERTATION |
Withdrawn status | Lost status | Damaged status | Not for loan | Current library | Full call number | Accession Number | Uniform Resource Identifier | Koha item type |
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IMSc Library | HBNI Th-9 | 61482 | http://www.imsc.res.in/xmlui/handle/123456789/122 | THESIS & DISSERTATION |