Related Experiment Video
Updated: May 28, 2025

The Generation of Higher-order Laguerre-Gauss Optical Beams for High-precision Interferometry
Published on: August 12, 2013
Future directions in cosmology
1Lawrence Berkeley National Laboratory, 1 Cyclotron Road, Berkeley, CA 94720, USA.
Abstract:
Cosmology is entering a very exciting time in its history, when a wealth of cutting-edge experiments are all starting to collect data, or about to. These experiments aim at addressing some of the most intriguing questions in fundamental physics, such as what is the nature of dark matter, is dark energy a cosmological constant or a varying field, what are the masses of the neutrinos and more. While Λ-CDM has emerged as a simple model that is consistent with most of the current datasets, we are starting to see some interesting deviations that deserve further exploration. This contribution provides an overview of upcoming projects and the science opportunities they will allow. In particular, we recall and comment on the DESI year-1 BAO constraints and their implications for dark energy. We put some of the most recent results and outstanding questions into the perspective of the forthcoming observational programme.This article is part of the discussion meeting issue 'Challenging the standard cosmological model'.
Related Concept Videos
Space-Time Curvature and the General Theory of Relativity
This has been verified in many experiments. However, space and time are no longer absolute. Two observers moving relative to one another do not agree on the length of objects or the passage of time. The mechanics of objects based on Newton's laws of...
Schwarzschild Radius and Event Horizon
The minimum speed required to launch a projectile from the surface of an object to which it is gravitationally bound so that it eventually escapes the object’s gravitational field is called the escape velocity. The escape velocity is independent of the mass of the object. Merging the idea of escape...
Detection of Black Holes
Their closest cousins are neutron stars, which are composed almost entirely of neutrons packed against each other, making them extremely dense. A neutron star has the same mass as the Sun but its diameter is only a few kilometers. Therefore, the escape velocity from their surface is close to the speed of light.
Not until the 1960s, when the first neutron...
The Wave Nature of Light
The Principle of Superposition and the Gravitational Field
The Fossil Record

