Neutrinos In Physics And Astrophysics

This book provides an up-to-date presentation of neutrino physics and astrophysics, covering topics such as neutrino interactions, detection techniques, neutrino masses, solar neutrinos, Earth's geoneutrinos, supernova explosions, cosmic rays, high-energy astrophysical neutrinos, cosmological neutrino background, and leptogenesis. It serves as a comprehensive resource for researchers and students in the field.

Format: Hardback
Length: 236 pages
Publication date: 19 October 2022
Publisher: World Scientific Publishing Co Pte Ltd

This comprehensive book delves into the realms of neutrino physics and astrophysics, offering a timely and detailed exploration of the cutting-edge research topics at the forefront of the field. It begins with a historical account, tracing the evolution of our understanding of neutrinos from their early discoveries to the present state. The core concepts of the Standard Model of electroweak interactions are introduced, along with a comprehensive presentation of the diverse neutrino interactions and detection techniques. The book explores various methods for imparting neutrinos with mass, shedding light on the phenomenon of neutrino oscillations, which serve as compelling evidence for non-vanishing neutrino masses.

The focus then shifts to the study of neutrinos originating from the Sun, including the insights gained from their observations and the potential applications in understanding our celestial neighbor. The geoneutrinos produced by radioactivity within the Earth are examined, along with the current status of their detection efforts. The book also surveys the neutrino production in the aftermath of supernova explosions, discussing the observations made in SN1987A and the insights that can be gained from future supernova events or the study of the diffuse supernova neutrino background.

In-depth descriptions are provided of the neutrino production by cosmic rays interacting with the atmosphere, highlighting the evidence for flavor oscillations and the oscillograms used to describe these flavor changes in terrestrial matter. The book explores the mechanisms behind the production of high-energy astrophysical neutrinos and presents the observations achieved with the IceCube detector, discussing their flavor content through the flavor triangle.

The cosmological neutrino background is explored, examining its impact on Big Bang nucleosynthesis and on cosmic microwave background (CMB) observations. The associated bound on neutrino masses and effective number is discussed, providing valuable insights into the nature of these enigmatic particles.

In conclusion, this book serves as a valuable resource for researchers and students in neutrino physics and astrophysics, providing a comprehensive and up-to-date account of the latest developments in the field. It offers a deep understanding of the fundamental principles, interactions, and observations related to neutrinos, paving the way for future advancements in our understanding of the universe.

Weight: 492g
Dimension: 159 x 237 x 21 (mm)
ISBN-13: 9789811260933