Probing Cosmic Dark Matter and Dark Energy with Weak Gravitational Lensing Statistics / Najlacnejšie knihy
Probing Cosmic Dark Matter and Dark Energy with Weak Gravitational Lensing Statistics

Kód: 09489423

Probing Cosmic Dark Matter and Dark Energy with Weak Gravitational Lensing Statistics

Autor Masato Shirasaki

In this book the applicability and the utility of two statistical approaches for understanding dark energy and dark matter with gravitational lensing measurement are introduced.§§For cosmological constraints on the nature of dark ... celý popis

113.79


Skladom u dodávateľa
Odosielame za 11 - 13 dní
Pridať medzi želanie

Mohlo by sa vám tiež páčiť

Darujte túto knihu ešte dnes
  1. Objednajte knihu a vyberte Zaslať ako darček.
  2. Obratom obdržíte darovací poukaz na knihu, ktorý môžete ihneď odovzdať obdarovanému.
  3. Knihu zašleme na adresu obdarovaného, o nič sa nestaráte.

Viac informácií

Viac informácií o knihe Probing Cosmic Dark Matter and Dark Energy with Weak Gravitational Lensing Statistics

Nákupom získate 281 bodov

Anotácia knihy

In this book the applicability and the utility of two statistical approaches for understanding dark energy and dark matter with gravitational lensing measurement are introduced.§§For cosmological constraints on the nature of dark energy, morphological statistics called Minkowski functionals (MFs) to extract the non-Gaussian information of gravitational lensing are studied. Measuring lensing MFs from the Canada-France-Hawaii Telescope Lensing survey (CFHTLenS), the author clearly shows that MFs can be powerful statistics beyond the conventional approach with the two-point correlation function. Combined with the two-point correlation function, MFs can constrain the equation of state of dark energy with a precision level of approximately 3-4 % in upcoming surveys with sky coverage of 20,000 square degrees.§§On the topic of dark matter, the author studied the cross-correlation of gravitational lensing and the extragalactic gamma-ray background (EGB). Dark matter annihilation is among the potential contributors to the EGB. The cross-correlation is a powerful probe of signatures of dark matter annihilation, because both cosmic shear and gamma-ray emission originate directly from the same dark matter distribution in the universe. The first measurement of the cross-correlation using a real data set obtained from CFHTLenS and the Fermi Large Area Telescope was performed. Comparing the result with theoretical predictions, an independent constraint was placed on dark matter annihilation. Future lensing surveys will be useful to constrain on the canonical value of annihilation cross section for a wide range of mass of dark matter.§§

Parametre knihy

Zaradenie knihy Książki po angielsku Mathematics & science Science: general issues Scientific standards

113.79

Obľúbené z iného súdka



Osobní odběr Bratislava a 2642 dalších

Copyright ©2008-24 najlacnejsie-knihy.sk Wszelkie prawa zastrzeżonePrywatnieCookies


Konto: Logowanie
Všetky knihy sveta na jednom mieste. Navyše za skvelé ceny.

Nákupní košík ( prázdný )

Nakupte za 59,99 € a
máte doručení zdarma.

Twoja lokalizacja: