Falls Sie nur an einem bestimmten Exempar interessiert sind, können Sie aus der folgenden Liste jenes wählen, an dem Sie interessiert sind:
Nur diese Ausgabe anzeigen…
Nur diese Ausgabe anzeigen…
Nur diese Ausgabe anzeigen…
On the Topology and Future Stability of the Universe (Oxford Mathematical Monographs)
12 Angebote vergleichen
Bester Preis: € 31,15 (vom 03.09.2015)On the Topology and Future Stability of the Universe (Oxford Mathematical Monographs) (2013)
ISBN: 9780191669781 bzw. 0191669784, in Englisch, 768 Seiten, OUP Oxford, neu, Erstausgabe, E-Book, elektronischer Download.
The standard starting point in cosmology is the cosmological principle; the assumption that the universe is spatially homogeneous and isotropic. After imposing this assumption, the only freedom left, as far as the geometry is concerned, is the choice of one out of three permissible spatial geometries, and one scalar function of time. Combining the cosmological principle with an appropriate description of the matter leads to the standard models. It is worth notingthat these models yield quite a successful description of our universe. However, even though the universe may, or may not, be almost spatially homogeneous and isotropic, it is clear that the cosmological principle is not exactly satisfied. This leads to several questions. The most natural one concerns stability: given initial data corresponding to an expanding model of the standard type, do small perturbations give rise to solutions that are similar to the future? Another question concerns the shape of the universe: what are the restrictions if we only assume theuniverse to appear almost spatially homogeneous and isotropic to every observer? The main purpose of the book is to address these questions. However, to begin with, it is necessary to develop the general theory of the Cauchy problem for the Einstein-Vlasov equations. In order to to make the results accessible to researchers who are not mathematicians, but who are familiar with general relativity, the book contains an extensive prologue putting the results into a more general context. Kindle Edition, Ausgabe: 1, Format: Kindle eBook, Label: OUP Oxford, OUP Oxford, Produktgruppe: eBooks, Publiziert: 2013-05-23, Freigegeben: 2013-05-23, Studio: OUP Oxford.
On the Topology and Future Stability of the Universe
ISBN: 9780191669774 bzw. 0191669776, in Deutsch, Oxford University Press, Vereinigtes Königreich Großbritannien und Nordirland, neu, E-Book.
On the Topology and Future Stability of the Universe, The standard starting point in cosmology is the cosmological principle; the assumption that the universe is spatially homogeneous and isotropic. After imposing this assumption, the only freedom left, as far as the geometry is concerned, is the choice of one out of three permissible spatial geometries, and one scalar function of time. Combining the cosmological principle with an appropriate description of the matter leads to the standard models. It is worth notingthat these models yield quite a successful description of our universe. However, even though the universe may, or may not, be almost spatially homogeneous and isotropic, it is clear that the cosmological principle is not exactly satisfied. This leads to several questions. The most natural one concerns stability: given initial data corresponding to an expanding model of the standard type, do small perturbations give rise to solutions that are similar to the future? Another question concerns the shape of the universe: what are the restrictions if we only assume theuniverse to appear almost spatially homogeneous and isotropic to every observer? The main purpose of the book is to address these questions. However, to begin with, it is necessary to develop the general theory of the Cauchy problem for the Einstein-Vlasov equations. In order to to make the results accessible to researchers who are not mathematicians, but who are familiar with general relativity, the book contains an extensive prologue putting the results into a more general context.
On the Topology and Future Stability of the Universe
ISBN: 9780191669781 bzw. 0191669784, in Englisch, Oxford University Press, Vereinigtes Königreich Großbritannien und Nordirland, neu.
On the Topology and Future Stability of the Universe, The standard starting point in cosmology is the cosmological principle; the assumption that the universe is spatially homogeneous and isotropic. After imposing this assumption, the only freedom left, as far as the geometry is concerned, is the choice of one out of three permissible spatial geometries, and one scalar function of time. Combining the cosmological principle with an appropriate description of the matter leads to the standard models. It is worth notingthat these models yield quite a successful description of our universe. However, even though the universe may, or may not, be almost spatially homogeneous and isotropic, it is clear that the cosmological principle is not exactly satisfied. This leads to several questions. The most natural one concerns stability: given initial data corresponding to an expanding model of the standard type, do small perturbations give rise to solutions that are similar to the future? Another question concerns the shape of the universe: what are the restrictions if we only assume theuniverse to appear almost spatially homogeneous and isotropic to every observer? The main purpose of the book is to address these questions. However, to begin with, it is necessary to develop the general theory of the Cauchy problem for the Einstein-Vlasov equations. In order to to make the results accessible to researchers who are not mathematicians, but who are familiar with general relativity, the book contains an extensive prologue putting the results into a more general context.
On the Topology and Future Stability of the Universe
ISBN: 9780191669781 bzw. 0191669784, in Englisch, Oxford University Press, Vereinigtes Königreich Großbritannien und Nordirland, neu.
On the Topology and Future Stability of the Universe, The standard starting point in cosmology is the cosmological principle; the assumption that the universe is spatially homogeneous and isotropic. After imposing this assumption, the only freedom left, as far as the geometry is concerned, is the choice of one out of three permissible spatial geometries, and one scalar function of time. Combining the cosmological principle with an appropriate description of the matter leads to the standard models. It is worth notingthat these models yield quite a successful description of our universe. However, even though the universe may, or may not, be almost spatially homogeneous and isotropic, it is clear that the cosmological principle is not exactly satisfied. This leads to several questions. The most natural one concerns stability: given initial data corresponding to an expanding model of the standard type, do small perturbations give rise to solutions that are similar to the future? Another question concerns the shape of the universe: what are the restrictions if we only assume theuniverse to appear almost spatially homogeneous and isotropic to every observer? The main purpose of the book is to address these questions. However, to begin with, it is necessary to develop the general theory of the Cauchy problem for the Einstein-Vlasov equations. In order to to make the results accessible to researchers who are not mathematicians, but who are familiar with general relativity, the book contains an extensive prologue putting the results into a more general context.
On the Topology and Future Stability of the Universe (Oxford Mathematical Monographs) (2013)
ISBN: 9780199680290 bzw. 0199680299, in Englisch, 768 Seiten, Oxford University Press, gebundenes Buch, neu, Erstausgabe.
Von Händler/Antiquariat, upandawaybooks.
The standard starting point in cosmology is the cosmological principle; the assumption that the universe is spatially homogeneous and isotropic. After imposing this assumption, the only freedom left, as far as the geometry is concerned, is the choice of one out of three permissible spatial geometries, and one scalar function of time. Combining the cosmological principle with an appropriate description of the matter leads to the standard models. It is worth noting that these models yield quite a successful description of our universe. However, even though the universe may, or may not, be almost spatially homogeneous and isotropic, it is clear that the cosmological principle is not exactly satisfied. This leads to several questions. The most natural one concerns stability: given initial data corresponding to an expanding model of the standard type, do small perturbations give rise to solutions that are similar to the future? Another question concerns the shape of the universe: what are the restrictions if we only assume the universe to appear almost spatially homogeneous and isotropic to every observer? The main purpose of the book is to address these questions. However, to begin with, it is necessary to develop the general theory of the Cauchy problem for the Einstein-Vlasov equations. In order to to make the results accessible to researchers who are not mathematicians, but who are familiar with general relativity, the book contains an extensive prologue putting the results into a more general context. Hardcover, Ausgabe: 1, Label: Oxford University Press, Oxford University Press, Produktgruppe: Book, Publiziert: 2013-07-18, Studio: Oxford University Press, Verkaufsrang: 2417367.
On the Topology and Future Stability of the Universe (Oxford Mathematical Monographs) (2013)
ISBN: 9780199680290 bzw. 0199680299, in Englisch, 768 Seiten, Oxford University Press, gebundenes Buch, gebraucht, Erstausgabe.
Von Händler/Antiquariat, LABYRINTH BOOKS.
The standard starting point in cosmology is the cosmological principle; the assumption that the universe is spatially homogeneous and isotropic. After imposing this assumption, the only freedom left, as far as the geometry is concerned, is the choice of one out of three permissible spatial geometries, and one scalar function of time. Combining the cosmological principle with an appropriate description of the matter leads to the standard models. It is worth noting that these models yield quite a successful description of our universe. However, even though the universe may, or may not, be almost spatially homogeneous and isotropic, it is clear that the cosmological principle is not exactly satisfied. This leads to several questions. The most natural one concerns stability: given initial data corresponding to an expanding model of the standard type, do small perturbations give rise to solutions that are similar to the future? Another question concerns the shape of the universe: what are the restrictions if we only assume the universe to appear almost spatially homogeneous and isotropic to every observer? The main purpose of the book is to address these questions. However, to begin with, it is necessary to develop the general theory of the Cauchy problem for the Einstein-Vlasov equations. In order to to make the results accessible to researchers who are not mathematicians, but who are familiar with general relativity, the book contains an extensive prologue putting the results into a more general context. Hardcover, Ausgabe: 1, Label: Oxford University Press, Oxford University Press, Produktgruppe: Book, Publiziert: 2013-07-18, Studio: Oxford University Press, Verkaufsrang: 2417367.
On the Topology and Future Stability of the Universe
ISBN: 9780199680290 bzw. 0199680299, in Englisch, Oxford University Press, gebundenes Buch, neu.
On the Topology and Future Stability of the Universe, 9780199680290, Book, Textbook, No Synopsis Available.
On the Topology and Future Stability of the Universe (Oxford Mathematical Monographs) (2013)
ISBN: 9780199680290 bzw. 0199680299, in Englisch, Oxford University Press, gebraucht.
Gently used. Expect delivery in 2-3 weeks.
On the Topology and Future Stability of the Universe
ISBN: 9780191669781 bzw. 0191669784, in Englisch, OUP Oxford, neu, E-Book.
Die Beschreibung dieses Angebotes ist von geringer Qualität oder in einer Fremdsprache. Trotzdem anzeigen