Skip to main content

Graphene and based bolometer

Graphene “the super material of the earth”.


Why this is super material? 

Because it conduct electricity better than ‘silver’, conduct heat better than ‘diamond’ and stronger than ‘steel’ and even with all these properties it also flexile.

What is Graphene?

Graphene is a simple material which forms of carbon atom. Graphite is the naturally occurring crystal of carbon and it is formed of large number of graphene shits which are placed over each other.

Or we can say that graphene is a semi-metal with a small overlap between the valence and the conduction bands. It is an allotrope of carbon consisting of a single layer of carbon atoms arranged in a hexagonal lattice.

Graphene was discovered by two Russian scientists “A Geim and K Novoselov" in 2004 with the help of two simple things i.e. “pencil and tape”.

They place pencil graphite over tape and make thin so that it will become a single layer i.e. Graphene.
And for this they get Noble prize in 2010.
Application
With all these properties it has so many applications like in future with this we will be able make buildings, mobiles phones, instant charging batteries and so many other things but in future.
But what’s now?
So now with graphene scientists have  made a graphene based “radiation detector”.
With a simple design and relative cost, the device classified as a bolometer. The new bolometer created by researcher at "Chalmers University of Technology" in Sweden is based on graphen's thermoelectric properties.
Radiation heats part of the device, inducing electron to move. The displaced electrons generate an electric field, which creates a voltage difference across the device.
Other devices rely on the generation of electric current or resistance change by incoming radiation.
However, measuring changes in current or resistent requires an external power source to generate initial current. Due to which these bolometers are slow.
But the piece of graphene in the new bolometer is small, so it is one of the fastest bolometer because it heats up and responds quickly.
  

Comments

Popular posts from this blog

What is Nebula. Images of some nebula by Hubble

A nebula is a giant cloud of dust and gas in space. Some nebulae (more than one nebula) come from the gas and dust thrown out by the explosion of a dying star, such as a supernova. Other nebulae are regions where new stars are beginning to form. For this reason, some nebulae are called "star nurseries." How do stars form in a nebula? Nebulae are made of dust and gases—mostly hydrogen and helium. The dust and gases in a nebula are very spread out, but gravity can slowly begin to pull together clumps of dust and gas. As these clumps get bigger and bigger, their gravity gets stronger and stronger. Eventually, the clump of dust and gas gets so big that it collapses from its own gravity. The collapse causes the material at the center of the cloud to heat up-and this hot core is the beginning of a star. Some of the most amazing nebula pictured by Hubble in Milky Way Galaxy The Eagle Nebula’s Pillars of Creation (M 16, Messier 16) The dust and gas in the pi...

WHAT IS A BLACK HOLE

In April, NASA created a big announcement that they captured first image of black hole.  BUT WHAT IS A BLACK HOLE It is a great amount of matter packed into a very small area - think of a star ten times more massive than the Sun squeezed into a sphere approximately the diameter of New York City. The result is a gravitational field so strong that nothing, not even light, can escape. Most famously, black holes were predicted by Einstein's theory of general relativity, which showed that when a massive star dies, it leaves behind a small, dense remnant core. If the core's mass is more than about three times the mass of the Sun, the equations showed, the force of gravity overwhelms all other forces and produces a black hole. HOW THEY ARE FORMED Most black holes form from the remnants of a large star that dies in a supernova explosion. (Smaller stars become dense neutron stars, which are not massive enough to trap light.) If the total mass of the star is large e...

Collision of galaxies, images taken by hubble

The interaction between galaxies is an on going process in universe. However the merging of big galaxies with each other on average once over the past 9 billion years. But Small galaxies were coalescing with large galaxies more frequently. In fact, our own Milky Way galaxy had several such mergers with small galaxies in its recent past. In the combination of galaxies there is no collision of stars with eath other, it is the dust and other material which collapse and billions of stars are born, mostly in groups and clusters of stars. Some of the images of colliding galaxies taken by hubble This is image of a pair of interacting galaxies called Arp 273. The distorted shape of the larger of the two galaxies shows signs of tidal interactions with the smaller of the two. It is thought that the smaller galaxy has actually passed through the larger one. This nearly 300 million light years away from earth. And a part of Constellation "Andromeda" Hubble has captured a...