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Quantum Cosmology [A Fundam...
The universe, ultimately, is to be described by quantum theory. Quantum aspects of all there is, including space and time, may not be significant for many purposes, but are crucial for some time. And so a quantum description of cosmology is required for a complete and consistent worldview. Consequences of quantum gravity on grander scales are expected to be enormous. In Quantum Cosmology, A Fundamental Description of the Universe, Martin Bojowald discusses his theory to see how black holes behave and where our universe came from. Applications like loop quantum gravity and cosmology have by now shed much light on cosmic evolution of a universe in a fundamental, microscopic description. Modern techniques demonstrate how the universe may have come from a non-singular phase before the Big Bang, how equations for the evolution of structure can be derived, how observations could be used to test these claims, but also what fundamental limitations remain to our knowledge of the universe before the Big Bang
Monografía
monografia Rebiun03603806 https://catalogo.rebiun.org/rebiun/record/Rebiun03603806 |acr nuu---uuuuu 130607s2011 xxu| s |||| 0|eng d 9781441982766 10.1007/978-1-4419-8276-6 doi UPM 991005528296704212 UCAR 991007917913304213 UPVA 996894117003706 UAM 991007719757104211 UR0338903 BUS PHDV bicssc PHR bicssc SCI033000 bisacsh 530.1 23 Bojowald, Martin Quantum Cosmology Recurso electrónico] A Fundamental Description of the Universe by Martin Bojowald Servicio en línea New York, NY Springer New York Imprint: Springer 2011 New York, NY New York, NY Springer New York Imprint: Springer IX, 308 p. digital IX, 308 p. Lecture Notes in Physics 0075-8450 835 Libros electrónicos descargables Introduction -- Cosmology and Quantum Theory -- Kinematics: Spatial Atoms -- Dynamics: Changing Atoms of Space-Time -- Effective Equations -- Harmonic Cosmology: The Universe Before the Big Bang and How Much We Can Know About It -- What Does It Mean for a Singularity to be Resolved? -- Anisotropy -- Midisuperspace Models: Black Hole Collapse -- Perturbative Inhomogenities -- Difference Equations -- Physical Hilbert Spaces -- General Aspects of Effective Descriptions The universe, ultimately, is to be described by quantum theory. Quantum aspects of all there is, including space and time, may not be significant for many purposes, but are crucial for some time. And so a quantum description of cosmology is required for a complete and consistent worldview. Consequences of quantum gravity on grander scales are expected to be enormous. In Quantum Cosmology, A Fundamental Description of the Universe, Martin Bojowald discusses his theory to see how black holes behave and where our universe came from. Applications like loop quantum gravity and cosmology have by now shed much light on cosmic evolution of a universe in a fundamental, microscopic description. Modern techniques demonstrate how the universe may have come from a non-singular phase before the Big Bang, how equations for the evolution of structure can be derived, how observations could be used to test these claims, but also what fundamental limitations remain to our knowledge of the universe before the Big Bang SpringerLink eBooks (Servicio en línea) Lecture Notes in Physics (Servicio en línea) Lecture Notes in Physics 0075-8450 835