Gravity's dark side
Description
Despite decades of searching, the 'dark matter' thought to hold galaxies together is still nowhere to be found. Matthew Chalmers describes how some physicists think it makes more sense to change our theory of gravity instead. Einstein's general theory of relativity is part of the bedrock of modern physics. It describes in elegant mathematical terms how matter causes space-time to curve, and therefore how objects move in a gravitational field. Since it was published in 1916, general relativity has passed every test asked of it with flying colours, and to many physicists the notion that it is wrong is sacrilege. But the motivation for developing an alternative theory of gravity is compelling. Over the last few years cosmologists have arrived at a simple yet extraordinarily successful model of universe. The trouble is that it requires most of the cosmos to be filled with mysterious stuff that we cannot see. In particular, general relativity - or rather its non-relativistic limit otherwise known as Newtonian gravity - can only correctly describe the dynamics of galaxies if we invoke huge quantities of 'dark matter'. Furthermore, an exotic entity called dark energy is necessary to account for the recent discovery that the expansion of the universe is accelerating. Indeed, in the standard model of cosmology, visible matter such as stars, planets and physics textbooks accounts for just 4% of the total universe. (U.K.)
Availability note (English)
Available online: http://www.physicsweb.org/Additional details
Additional titles
- Augmented title (English)
- Doing without dark matter
Identifiers
Publishing Information
- Journal Title
- Physics World
- Journal Volume
- 19
- Journal Issue
- 6
- Journal Page Range
- p. vp.
- ISSN
- 0953-8585
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 37082276
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Is Lead record
- Yes
- Descriptors DEI
- ACCELERATION; COSMOLOGICAL CONSTANT; COSMOLOGY; EINSTEIN FIELD EQUATIONS; GENERAL RELATIVITY THEORY; GRAVITATION; INFLATIONARY UNIVERSE; METRICS; NONLUMINOUS MATTER; SCALAR FIELDS; SPACE-TIME; TENSOR FIELDS; VECTOR FIELDS
- Descriptors DEC
- COSMOLOGICAL MODELS; EQUATIONS; FIELD EQUATIONS; FIELD THEORIES; MATHEMATICAL MODELS; MATTER; RELATIVITY THEORY