FP7Индивидуална стипендия2012–2015

QUANTUM COSMOLOGY · Quantum Gravity and the Early Universe

7РП — „Хора“ (Действия „Мария Кюри“)

Период
2012-11-16 → 2015-04-21
Финансиране от ЕС
191 675 €
Участници
1
Схема
MC-IIF

Линиите свързват координатора с партньорите.

Накратко на български

Квантовата гравитация изследва ранната Вселена чрез моделиране на малките неравномерности в пространството. Това помага да се разберат законите на физиката в началото на времето чрез сравнение на теоретичните изчисления с реални наблюдателни данни.

Този кратък обзор е генериран от изкуствен интелект

Кратко обяснение, генерирано от езиков модел по текста на CORDIS. Оригиналът е по-долу.

Резултати накратко

Quantum Gravity and the Early Universe

The major goals of this project were: 1. Develop and extend the Loop Quantisation approach to cosmological systems with perturbative inhomogeneities. 2. Derive the expected cosmological power spectra for such systems and hence confront these Loop Quantum Gravity cosmological models with precision observational data. 3. Use these inhomogeneous cosmological models to shed light on the challenges facing the development of the full, non-linear theory, in particular use the Hamiltonian and dynamics of the inhomogeneous cosmological models as a guide to understanding the dynamical sector of the full theory. 4. Begin a program of 'Loop Quantising' cosmological models of higher derivative gravity in order to go beyond the phase space of general relativity. Despite the fact that this project was terminated after seven months, due to a change in personal circumstances, the first two of these goals was achieved and the results published (see the Major Accomplishments section above). Together with two other publications in the same series, this work has been extremely well received by the quantum gravity community and has already been cited more the fifty times. The specific goals and milestones reached are detailed in the following ‘Goals and Milestones’ section. At the end of the seven month period, the project was approximately four months ahead of schedule. Several outreach goals were specified in the original proposal, the first two to be completed at four and eight months into the project (see ‘Goals and Milestones’ section below). The first of these was to give a series of talks to Philosophy and other non-physics undergraduates, and was partially completed. As an invited speaker at a philosophy and physics workshop at Penn State (see Major Accomplishments section above), I had an opportunity to present this work to philosophy students, in addition to other workshop attendees. This was very successful, however it was not the initially envisioned series of talks and hence can only be considered to have been partially successful. The second outreach goal, ‘Give a series of talks/ presentations to local secondary schools’ was to be completed at month eight, however the project was suspended prior to this stage. In addition to the outreach activities outlined in the original proposal, the work completed in this project was documented by the international popular science magazine ‘New Scientist’ (see Major Accomplishments section above).

Текст от CORDIS, на английски · Данни: CORDIS, © Европейски съюз

Цел на проекта

Quantum Gravity will be studied in the context of early universe cosmology. Specifically, inhomogeneous perturbations, and their evolution, within Loop Quantum Cosmology will be developed so as to allow direct observational testing of the theory. A phase of the early universe that is dominated by Quantum Gravity may produce effects observable in the detailed structure of the Cosmic Microwave Background or large scale galaxy distributions. In order to understand and quantify such effects the power spectra and non-gaussianities of scalar and tensor perturbations, will be calculated within Loop Quantum Cosmology. This will then allow the theory to be directly tested against a wide range of observational data, such that from the WMAP and Plank satellites and various deep field galaxy surveys. This would provide us with a unique window into the deep Quantum Gravity regime and an unprecedented probe of ultra high energy physics.This project will require a significant extension of the Loop Quantum Cosmological model which should follow as closely as possible the full underlying Loop Quantum Gravity theory. Thus this project will simultaneously strengthen the link between Loop Quantum Cosmology and the full theory whilst also producing (potentially) observable predictions. Since quantum field theory in curved space-times is a key part of cosmological perturbation theory, this project will also draw links between full Loop Quantum Gravity, quantum fields on a semi-classical space-time and classical cosmology.Although the main thrust of this project will be aimed towards Loop Quantum Cosmology, the methods developed will be applicable to other approaches to Quantum Gravity. This project will provide a toolbox with which many theories of Quantum Gravity can, for the first time, be tested and constrained against observations. This if particularly timely due to the flood of precision cosmological data that will come from the next generation of observatories.

Оригинален текст от CORDIS (на английски).

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Данни: CORDIS, © Европейски съюз