The general theory of relativity, published by Albert Einstein in 1915, is one of the cornerstones of modern physics. It is a theory that describes the gravitational interactions, generalising and overcoming the previous theory of Isaac Newton, developed almost three centuries earlier.
General relativity has revolutionised the concept of gravity, which after Einstein is no longer a force able to propagate instantaneously, like Newton thought. Instead, it is the effect of the curvature of spacetime, which is transformed from a simple stage to a lead actor.
Einstein’s revolution does not, however, cancel Newton, but completes him. In “weak” regimes, in which gravitational interaction is not very intense, Newton’s gravity actually continues to be an excellent approximation of Einstein’s.
Over the last century, general relativity has received many experimental confirmations, completing an evolution shared by many revolutionary theories. First considered a bizarre mathematical model without practical purposes, it quickly became crucial for explaining many astrophysical phenomena, until becoming, today, fundamental for daily applications as well (just think of satellite navigators, which would be unusable if relativistic effects were not taken into account).
Einstein’s most spectacular predictions include often counter-intuitive phenomena. One example is the dilation of time near an intense gravitational field, or the effect known as “gravitational lensing”, which predicts the curvature of starlight around massive objects (with the consequent deformation or multiplication of the source in the eyes of the observer). But the solutions to the equations of general relativity also predicted black holes (similarly considered merely mathematical curiosities up to a certain point, but whose existence in nature is almost certain today) and gravitational waves. The first historic observation of the latter, in 2015, represented the final confirmation of perhaps the most iconic theory o fphysics of the last century.
The standard model of cosmology, also called the Lambda-CDM model, is the simplest theoretical framework able to provide a good description of all the observed cosmological phenomena with just 6 free parameters.
The Big Bang theory is currently the most reliable scientific theory about the origins of the cosmos. It postulates that our universe started approximately 13.8 billion years ago from an extremely hot and dense state and, since then, has expanded basically continuously.
The universe is continuously traversed by elementary and subatomic particles, which travel through space at very high speeds. Many of these reach Earth, bringing very precious information about astrophysical phenomena that produced them.
Gravitational waves are ripples in spacetime produced by large masses in accelerated motion during violent astrophysical phenomena, such as, for example, the merging of pairs of black holes or neutron stars.
On 17 August 2017, a coalescence of neutron stars that occurred in the NGC 4993 galaxy (at approximately 130 million light years from us) was observed at the same time by LIGO and Virgo gravitational wave observers and by numerous electromagnetic telescopes (from radio waves to energetic gamma rays) throughout the world.
Black holes are one of the most fascinating and mysterious astronomical objects. They were hypothesised for the first time in 1916, a year after Albert Einstein’s publication of his general theory of relativity, when the German astronomer Karl Schwarzschild presented the first exact solution of the theory’s equations, known as “Einstein equations”.
Dark matter is a kind of matter that is invisible to telescopes, which does not emit electromagnetic radiation and whose (presumed) existence can only be indirectly detected today through its gravitational effects.
Observations of the speeds of galaxies collected by Edwin Hubble in the 1920s showed that our universe is not static but expanding, providing one of the first solid proofs in favour of the Big Bang theory.