Mediaspace scheduled maintenance: Aug 25, 2026 07:00 - 12:00 AM. During this time, videos will be temporarily unavailable. Check status updates.

Lecture

Untitled

Official source

https://switch-video-production.os.zhdk.cloud.switch.ch/1d33/3328/58141b48c40c91bb90d2/h264-1080p.mp4?X-Amz-Algorithm=AWS4-HMAC-SHA256&X-Amz-Credential=c70ce910fb73491f9933421af7a4fcee%2F20240725%2Fus-east-1%2Fs3%2Faws4_request&X-Amz-Date=20240725T142243Z&X-Amz-Expires=86400&X-Amz-SignedHeaders=host&X-Amz-Signature=e346b69888b660ca9cfb795e0df0f58bee9d890010a64e87f70b743756b44657

About this result

This page is automatically generated and may contain information that is not correct, complete, up-to-date, or relevant to your search query. The same applies to every other page on this website. Please make sure to verify the information with EPFL's official sources.

Related concepts (32)

Universe

The universe is all of space and time and their contents, including planets, stars, galaxies, and all other forms of matter and energy. The Big Bang theory is the prevailing cosmological description of the development of the universe. According to this theory, space and time emerged together 13.787billion years ago, and the universe has been expanding ever since the Big Bang. While the spatial size of the entire universe is unknown, it is possible to measure the size of the observable universe, which is approximately 93 billion light-years in diameter at the present day.

Shape of the universe

The shape of the universe, in physical cosmology, is the local and global geometry of the universe. The local features of the geometry of the universe are primarily described by its curvature, whereas the topology of the universe describes general global properties of its shape as a continuous object. The spatial curvature is described by general relativity, which describes how spacetime is curved due to the effect of gravity.

Ultimate fate of the universe

The ultimate fate of the universe is a topic in physical cosmology, whose theoretical restrictions allow possible scenarios for the evolution and ultimate fate of the universe to be described and evaluated. Based on available observational evidence, deciding the fate and evolution of the universe has become a valid cosmological question, being beyond the mostly untestable constraints of mythological or theological beliefs.

Static universe

In cosmology, a static universe (also referred to as stationary, infinite, static infinite or static eternal) is a cosmological model in which the universe is both spatially and temporally infinite, and space is neither expanding nor contracting. Such a universe does not have so-called spatial curvature; that is to say that it is 'flat' or Euclidean. A static infinite universe was first proposed by English astronomer Thomas Digges (1546–1595).

Neutrino detector

A neutrino detector is a physics apparatus which is designed to study neutrinos. Because neutrinos only weakly interact with other particles of matter, neutrino detectors must be very large to detect a significant number of neutrinos. Neutrino detectors are often built underground, to isolate the detector from cosmic rays and other background radiation. The field of neutrino astronomy is still very much in its infancy – the only confirmed extraterrestrial sources are the Sun and the supernova 1987A in the nearby Large Magellanic Cloud.

Related lectures (31)

Neutrino and gravitational wave telescopes MOOC: The Radio Sky II: Observational Radio Astronomy

Explains the operation of neutrino and gravitational wave telescopes, global astronomy events, and the solar neutrino problem.

Introduction to Astroparticle Physics: Cosmic Rays and Dark Matter

Covers astroparticle physics, focusing on cosmic rays, dark matter, and the universe's expansion.

Radio Interferometry: The Universe At Radio Wavelengths MOOC: The Radio Sky II: Observational Radio Astronomy

Explores radio interferometry, MeerKAT telescope, imaging vs. single measurement, and Fourier transform in radio astronomy.

Dark Matter Detection: WIMPs and Experimental Techniques

Covers the detection of dark matter, focusing on WIMPs and experimental techniques used in laboratories.

Data Inspection: Visibility Data and CASA Software MOOC: The Radio Sky II: Observational Radio Astronomy