Kontakt
Jak nakupovat
Doručení
Nákupní rádce
Simulations of Galaxy Formation and Large Scale Structure
PhD Thesis, Ludwig-Maximilians-Universität München (LMU)
Angličtina
182 b
Až 30 dní na vrácení zboží
Zákazníci také koupili
binding.
2 729
Kč
/
Pevná
1 446
Kč
/
Brožovaná
1 324
Kč
In this work we use the N-body resimulation technique to address aspects of structure formation. In the first chapter we study the influence of the local environment of DM haloes on their properties. In the second chapter we address the so-called substructure problem which is one of the major challenges of the CDM model of cosmology. We perform ultra-high resolution simulations of the assembly of a Milky Way type dark matter halo within its full cosmological context and propose a new analytical fitting formula (SWTS) which provides a better fit to the simulated Milky Way halo than the NFW or Moore profiles do. In the third chapter we use our ultra-high resolution simulations to study the possible -ray signal from dark matter annihilation. If such a signal was detected, the nature of the dark matter, the answer to one of the most important questions of modern cosmology, would be known. (urn:nbn:de:bvb:19-16446)
Informace o knize
Angličtina
Kategorie
Darujte tuto knihu ještě dnes
Je to snadné
1 Přidejte knihu do košíku a zvolte doručit jako dárek 2 Obratem vám zašleme poukaz 3 Kniha dorazí na adresu obdarovanéhoMohlo by vás také zajímat
/
Brožovaná
237
Kč
/
Brožovaná
4 820
Kč
/
Pevná
3 532
Kč
/
Brožovaná
1 207
Kč
/
Adobe ePub DRM
8 119
Kč
