Monday, 5 April 2021

Baikal GVD- telescope under water

Lake Baikal is deepest lake of the world. It is located in the region of Siberia in Russia. Russian scientists have developed world’s biggest underwater telescopes called Baikal- GVD (Gigaton Volume Detector). It is to be deployed in the waters of Lake Baikal. It is an international project in the field of neutrino astronomy. By this mission, it is possible to study about the most mysterious particle of our universe i.e. NEUTRINO. It will aid scientists to know about the origin of universe and even about the supernovas and nuclear reactions in the sun. Neutrinos are everywhere with no electric charge and no mass. They weakly interact or do not interact with the forces around them. So that’s why it is really challenging task to detect them.   

Just like Baikal- GVD, the other two largest neutrino detectors are deployed as ANTARES in Mediterranean Sea and other the IceCube at the South Pole.

Baikal- GVD: Its primary goal is to study the flux of high energy cosmic neutrinos and its sources. Telescope was submerged to 2500-4300 feet, about 4km from shore. Water is an effective medium to detect neutrinos. Lake Baikal is most suitable for this observation because of its depth.


What makes neutrino most interesting?

Neutrinos are second most abundant particle in our universe after photons. Trillions of neutrinos are passing through our body in every single second. Although their numbers are so huge, still it is so difficult to catch them. Why? This is because they do not posses any charge and does not interact with anything. Scientists also state that neutrinos might posses some unique properties which may helps us understanding that why this universe is made of matter rather than antimatter.

But why we are detecting neutrinos under water or in ice?

The answer is:  when one out of trillion neutrinos interacts, it may leave a flash of light or a line of bubbles which can be detected by large detectors like Baikal GVD. This telescope or we may say detector is designed to detect high energy neutrinos which may be coming from supernovas occurring somewhere in our universe, or may be from nuclear reactions in our sun, or may be from earth’s core.