Kilonova: Colliding Neutron Stars

A little update on where I am with everything at the moment. Again I am incredibly apologetic for updating less frequently recently due to a lot going on. As you might already know, I entered the Breakthrough Junior Challenge, been notified as a semifinalist, and recently crowned Regional Champion of Europe – the popular vote process definitely was more time consuming than I had imagined, but now (I hope) I can share with you some of the exciting things I’ve been wanting to write about for a while.

wallpaper__somewhere__something_incredible_is_waiting_to_be_known__7

Firstly this post is on what I consider as THE BIGGEST DISCOVERY IN PHYSICS this year – the neutron star collision. You might already know that the 2017 Nobel Prize in Physics was awarded to the three leading physicists who were involved in a worldwide collaboration in the search for gravitational waves. The “kilonova” on August 17th was not only a detection of another gravity wave but it also unveiled so many more utterly amazing things about the cosmos we were yet to discover.

Neutron Stars

fb0f536c8c0bd7b2ccf429747dd36c12--neutron-star-about-space

To start off let’s jump straight into the science behind the event of colliding Neutron stars. Neutron stars can be thought of as the less extreme versions of black holes – which are a result of very massive stars collapsing under their own gravitational pull and forming a point of infinite space-time curvature. These stars are the remnants of the supernovae of stars that are roughly 10 to 29 solar masses, too big to form a white dwarf (like how our own Sun will after its death) and too small to form a black hole. When a star this size explodes, its gravity is so strong that it literally forces electrons and protons to combine into neutrons, and the neutron star is stopped from further collapse by neutron degeneracy pressure. Neutron stars are extremely small and dense, their diameters are the size of cities but a teaspoon can be the weight of Mount Everest. Thus, there is no wonder how they produce immensely strong gravitational fields and not only cause gravitational lensing but also gravitational waves.

Continue reading

Advertisements

Dark Matter #2: Gravitational Lensing

heic1506e.jpgA couple of months ago I talked about a piece of evidence supporting the existence of Dark Matter which is the fact that the stars in the outskirts of galaxies were seen to move at a similar pace as galaxies near the galactic core, defying the norm of the Keplerian Decline.

Recap: Dark Matter makes up roughly 25% of the Universe, so it is five times more prevalent than ordinary Baryonic Matter. Physicists gave it the name Dark Matter not because of it having some mysterious evil property or anything of that sort, but because it simply does not interact with Electromagnetic Radiation. I agree Physicists are a creative bunch.

Continue reading