Bolejko Krzysztof (15 results)

Condition: Very Good. Reviews developments in applications of inhomogeneous models to cosmology, for graduate students and academic researchers in astrophysics. Series: Cambridge Monographs on Mathematical Physics. Num Pages: 256 pages, 20 b/w illus. BIC Classification: PGK. Category: (P) Professional & Vocational; (UP) Postgraduate, Research & Scholarly. Dimension: 247 x 174 x 16. Weight in Grams: 62. Book in very good condition, front cover damaged. 2009. hardcover. . . . . Books ship from the US and Ireland.

Condition: As New. Reviews developments in applications of inhomogeneous models to cosmology, for graduate students and academic researchers in astrophysics. Series: Cambridge Monographs on Mathematical Physics. Num Pages: 256 pages, 20 b/w illus. BIC Classification: PGK. Category: (P) Professional & Vocational; (UP) Postgraduate, Research & Scholarly. Dimension: 247 x 174 x 16. Weight in Grams: 62. . 2009. hardcover. . . . . Books ship from the US and Ireland.

Condition: Very Good. Reviews developments in applications of inhomogeneous models to cosmology, for graduate students and academic researchers in astrophysics. Series: Cambridge Monographs on Mathematical Physics. Num Pages: 256 pages, 20 b/w illus. BIC Classification: PGK. Category: (P) Professional & Vocational; (UP) Postgraduate, Research & Scholarly. Dimension: 247 x 174 x 16. Weight in Grams: 62. Book in very good condition, front cover damaged. 2009. hardcover. . . . .

Condition: As New. Reviews developments in applications of inhomogeneous models to cosmology, for graduate students and academic researchers in astrophysics. Series: Cambridge Monographs on Mathematical Physics. Num Pages: 256 pages, 20 b/w illus. BIC Classification: PGK. Category: (P) Professional & Vocational; (UP) Postgraduate, Research & Scholarly. Dimension: 247 x 174 x 16. Weight in Grams: 62. . 2009. hardcover. . . . .

Condition: good. This is a pre-loved book that shows moderate signs of wear from previous reading. You may notice creases, edge wear, or a cracked spine, but it remains in solid, readable condition.Please note:-May include library or rental stickers, stamps, or markings.-Supplemental materials e.g., CDs, access codes, inserts are not guaranteed.-Box sets may not come with the original outer box. If it does, the box will not be in perfect condition. -Sourced from donation centers; authenticity not verified with publisher. Your satisfaction is our top priority! If you have any questions or concerns about your order, please don't hesitate to reach out. Thank you for shopping with us and supporting small businessâ"happy reading!

Cloth. Condition: Near Fine. 242 pp. Tightly bound. Corners not bumped. Text is free of markings. Minor, light ding to heal of spine.

Condition: Very Good.

Condition: New. In.

Hardback. Condition: New. As the structures in our Universe are mapped out on ever larger scales, and with increasing detail, the use of inhomogeneous models is becoming an essential tool for analyzing and understanding them. This book reviews a number of important developments in the application of inhomogeneous solutions of Einstein's field equations to cosmology. It shows how inhomogeneous models can be employed to study the evolution of structures such as galaxy clusters and galaxies with central black holes, and to account for cosmological observations like supernovae dimming, the cosmic microwave background, baryon acoustic oscillations or the dependence of the Hubble parameter on redshift within classical general relativity. Whatever `dark matter' and `dark energy' turn out to be, inhomogeneities exist on many scales and need to be investigated with all appropriate methods. This book is of great value to all astrophysicists and researchers working in cosmology, from graduate students to academic researchers.

Hardback. Condition: New. As the structures in our Universe are mapped out on ever larger scales, and with increasing detail, the use of inhomogeneous models is becoming an essential tool for analyzing and understanding them. This book reviews a number of important developments in the application of inhomogeneous solutions of Einstein's field equations to cosmology. It shows how inhomogeneous models can be employed to study the evolution of structures such as galaxy clusters and galaxies with central black holes, and to account for cosmological observations like supernovae dimming, the cosmic microwave background, baryon acoustic oscillations or the dependence of the Hubble parameter on redshift within classical general relativity. Whatever `dark matter' and `dark energy' turn out to be, inhomogeneities exist on many scales and need to be investigated with all appropriate methods. This book is of great value to all astrophysicists and researchers working in cosmology, from graduate students to academic researchers.

Buch. Condition: Neu. Druck auf Anfrage Neuware - Printed after ordering - As the structures in our Universe are mapped out on ever larger scales, and with increasing detail, the use of inhomogeneous models is becoming an essential tool for analyzing and understanding them. This book reviews a number of important developments in the application of inhomogeneous solutions of Einstein's field equations to cosmology. It shows how inhomogeneous models can be employed to study the evolution of structures such as galaxy clusters and galaxies with central black holes, and to account for cosmological observations like supernovae dimming, the cosmic microwave background, baryon acoustic oscillations or the dependence of the Hubble parameter on redshift within classical general relativity. Whatever `dark matter' and `dark energy' turn out to be, inhomogeneities exist on many scales and need to be investigated with all appropriate methods. This book is of great value to all astrophysicists and researchers working in cosmology, from graduate students to academic researchers.

Hardcover. Condition: new. Hardcover. As the structures in our Universe are mapped out on ever larger scales, and with increasing detail, the use of inhomogeneous models is becoming an essential tool for analyzing and understanding them. This book reviews a number of important developments in the application of inhomogeneous solutions of Einstein's field equations to cosmology. It shows how inhomogeneous models can be employed to study the evolution of structures such as galaxy clusters and galaxies with central black holes, and to account for cosmological observations like supernovae dimming, the cosmic microwave background, baryon acoustic oscillations or the dependence of the Hubble parameter on redshift within classical general relativity. Whatever `dark matter' and `dark energy' turn out to be, inhomogeneities exist on many scales and need to be investigated with all appropriate methods. This book is of great value to all astrophysicists and researchers working in cosmology, from graduate students to academic researchers. Inhomogeneous models are becoming an essential tool in analyzing and understanding the structures in our Universe. This book reviews important developments in the application of inhomogeneous solutions of Einstein's field equations to cosmology. The text is of great value to astrophysicists working in cosmology, from graduate students to academic researchers. This item is printed on demand. Shipping may be from multiple locations in the US or from the UK, depending on stock availability.

Hardcover. Condition: new. Hardcover. As the structures in our Universe are mapped out on ever larger scales, and with increasing detail, the use of inhomogeneous models is becoming an essential tool for analyzing and understanding them. This book reviews a number of important developments in the application of inhomogeneous solutions of Einstein's field equations to cosmology. It shows how inhomogeneous models can be employed to study the evolution of structures such as galaxy clusters and galaxies with central black holes, and to account for cosmological observations like supernovae dimming, the cosmic microwave background, baryon acoustic oscillations or the dependence of the Hubble parameter on redshift within classical general relativity. Whatever `dark matter' and `dark energy' turn out to be, inhomogeneities exist on many scales and need to be investigated with all appropriate methods. This book is of great value to all astrophysicists and researchers working in cosmology, from graduate students to academic researchers. Inhomogeneous models are becoming an essential tool in analyzing and understanding the structures in our Universe. This book reviews important developments in the application of inhomogeneous solutions of Einstein's field equations to cosmology. The text is of great value to astrophysicists working in cosmology, from graduate students to academic researchers. This item is printed on demand. Shipping may be from our UK warehouse or from our Australian or US warehouses, depending on stock availability.

Condition: New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. Inhomogeneous models are becoming an essential tool in analyzing and understanding the structures in our Universe. This book reviews important developments in the application of inhomogeneous solutions of Einstein s field equations to cosmology. The text is.

Hardcover. Condition: new. Hardcover. As the structures in our Universe are mapped out on ever larger scales, and with increasing detail, the use of inhomogeneous models is becoming an essential tool for analyzing and understanding them. This book reviews a number of important developments in the application of inhomogeneous solutions of Einstein's field equations to cosmology. It shows how inhomogeneous models can be employed to study the evolution of structures such as galaxy clusters and galaxies with central black holes, and to account for cosmological observations like supernovae dimming, the cosmic microwave background, baryon acoustic oscillations or the dependence of the Hubble parameter on redshift within classical general relativity. Whatever `dark matter' and `dark energy' turn out to be, inhomogeneities exist on many scales and need to be investigated with all appropriate methods. This book is of great value to all astrophysicists and researchers working in cosmology, from graduate students to academic researchers. Inhomogeneous models are becoming an essential tool in analyzing and understanding the structures in our Universe. This book reviews important developments in the application of inhomogeneous solutions of Einstein's field equations to cosmology. The text is of great value to astrophysicists working in cosmology, from graduate students to academic researchers. This item is printed on demand. Shipping may be from our Sydney, NSW warehouse or from our UK or US warehouse, depending on stock availability.