Cargando…

Simulations of Dark Energy Cosmologies

A major outstanding problem in physics is understanding the nature of the dark energy that is driving the accelerating expansion of the Universe. This thesis makes a significant contribution by demonstrating, for the first time, using state-of-the-art computer simulations, that the interpretation of...

Descripción completa

Detalles Bibliográficos
Clasificación:Libro Electrónico
Autor principal: Jennings, Elise (Autor)
Autor Corporativo: SpringerLink (Online service)
Formato: Electrónico eBook
Idioma:Inglés
Publicado: Berlin, Heidelberg : Springer Berlin Heidelberg : Imprint: Springer, 2012.
Edición:1st ed. 2012.
Colección:Springer Theses, Recognizing Outstanding Ph.D. Research,
Temas:
Acceso en línea:Texto Completo

MARC

LEADER 00000nam a22000005i 4500
001 978-3-642-29339-9
003 DE-He213
005 20220112172310.0
007 cr nn 008mamaa
008 120526s2012 gw | s |||| 0|eng d
020 |a 9783642293399  |9 978-3-642-29339-9 
024 7 |a 10.1007/978-3-642-29339-9  |2 doi 
050 4 |a QB980-991 
072 7 |a PGK  |2 bicssc 
072 7 |a SCI015000  |2 bisacsh 
072 7 |a PGK  |2 thema 
082 0 4 |a 523.1  |2 23 
100 1 |a Jennings, Elise.  |e author.  |4 aut  |4 http://id.loc.gov/vocabulary/relators/aut 
245 1 0 |a Simulations of Dark Energy Cosmologies  |h [electronic resource] /  |c by Elise Jennings. 
250 |a 1st ed. 2012. 
264 1 |a Berlin, Heidelberg :  |b Springer Berlin Heidelberg :  |b Imprint: Springer,  |c 2012. 
300 |a XII, 112 p.  |b online resource. 
336 |a text  |b txt  |2 rdacontent 
337 |a computer  |b c  |2 rdamedia 
338 |a online resource  |b cr  |2 rdacarrier 
347 |a text file  |b PDF  |2 rda 
490 1 |a Springer Theses, Recognizing Outstanding Ph.D. Research,  |x 2190-5061 
505 0 |a Introduction -- The Growth of Matter Perturbations in the Universe -- Simulations of Quintessential Cold Dark Matter -- Modelling Redshift Space Distortions in Hierarchical Cosmologies -- Testing Gravity Using the Growth of Large Scale Structure in the Universe -- Conclusions -- Appendices. 
520 |a A major outstanding problem in physics is understanding the nature of the dark energy that is driving the accelerating expansion of the Universe. This thesis makes a significant contribution by demonstrating, for the first time, using state-of-the-art computer simulations, that the interpretation of future galaxy survey measurements is far more subtle than is widely assumed, and that a major revision to our models of these effects is urgently needed. The work contained in the thesis was used by the WiggleZ dark energy survey to measure the growth rate of cosmic structure in 2011 and had a direct impact on the design of the surveys to be conducted by the European Space Agency's Euclid mission, a 650 million euro project to measure dark energy. 
650 0 |a Cosmology. 
650 0 |a Mathematical physics. 
650 0 |a Elementary particles (Physics). 
650 0 |a Quantum field theory. 
650 1 4 |a Cosmology. 
650 2 4 |a Theoretical, Mathematical and Computational Physics. 
650 2 4 |a Elementary Particles, Quantum Field Theory. 
710 2 |a SpringerLink (Online service) 
773 0 |t Springer Nature eBook 
776 0 8 |i Printed edition:  |z 9783642293405 
776 0 8 |i Printed edition:  |z 9783642436406 
776 0 8 |i Printed edition:  |z 9783642293382 
830 0 |a Springer Theses, Recognizing Outstanding Ph.D. Research,  |x 2190-5061 
856 4 0 |u https://doi.uam.elogim.com/10.1007/978-3-642-29339-9  |z Texto Completo 
912 |a ZDB-2-PHA 
912 |a ZDB-2-SXP 
950 |a Physics and Astronomy (SpringerNature-11651) 
950 |a Physics and Astronomy (R0) (SpringerNature-43715)