Rare radioactive decay captured by dark matter detector

Scientists have found the first direct evidence of a rare radioactive decay reaction, known as the two neutrino double electron capture.

Scientists have found the first direct evidence of a rare radioactive decay reaction, known as the two neutrino double electron capture.

There are four fundamental forces in the Universe: gravitational force, electromagnetic force, strong forces and weak forces.
Among these, the weak forces act at the shortest distance and aid in the disintegration of atomic nuclei. This happens through a process known as beta decay.
One of the processes of beta decay is an electron capture — in which the nucleus captures an electron, in turn converting a proton in the nucleus into a neutron and emitting a neutrino.
The disintegration of some atomic nuclei happens through a double electron capture (two electrons are captured by the nucleus instead of one) which is very slow, and hence the longer half life.

Observations:-

The observation was made in the decay of xenon 124 nuclei, which were part of the XENON1T dark matter detector experiment, to tellurium 124.
This detection is an important step towards knowing the constituents of dark matter, which makes up 27 per cent of the Universe.
Researchers have theorised that dark matter could be made up of yet unfound particles known as Weakly Interacting Massive Particles (WIMP).
Such particles will display rare radioactive reactions such as neutrino-less double beta decay, one example of which is a neutrino-less double electron capture.
The current observation of a neutrino double electron capture is the first step towards the neutrino-less version of the reaction.

Dark Matter-

Everything else, on Earth or elsewhere that we can see and observe constitutes less than 5 per cent of the Universe. The rest of the Universe, around 68 per cent, is dark energy and remains unknown.
Scientists have come to this conclusion as the rate of expansion of the Universe cannot be explained with the existence of ordinary matter alone.
Only by taking dark matter and dark energy into account can this rate be explained. But apart from this, not much is known about these two mysterious entities.
The majority of dark matter is thought to be non-baryonic in nature, possibly being composed of some as-yet undiscovered subatomic particles.
Its presence is implied in a variety of astrophysicalobservations, including gravitational effects that cannot be explained by accepted theories of gravity unless more matter is present than can be seen.