Menu

Blog

Archive for the ‘cosmology’ category: Page 301

Aug 29, 2019

Black hole warning: Astronomer’s dire prediction over Earth’s future revealed

Posted by in categories: cosmology, futurism

A black hole is a region of spacetime exhibiting gravitational acceleration so strong that nothing can escape, not even light. These cosmic phenomena are said to form when massive stars collapse at the end of their life cycle. Then, they can continue to grow by absorbing mass from their surroundings, engulfing stars in their path and merging with other black holes.

Aug 29, 2019

Watch the expansion of the Cas A supernova remnant with your own eyes!

Posted by in category: cosmology

Wow. The Chandra X-ray Observatory just celebrated its 20th anniversary of being launched into space! It roared into orbit on board the Space Shuttle Columbia on July 23, 1999.

Continue reading “Watch the expansion of the Cas A supernova remnant with your own eyes!” »

Aug 27, 2019

You might actually be immortal according to quantum mechanics

Posted by in categories: cosmology, quantum physics

Then again, maybe not.

In a previous post, I explained why quantum mechanics predicts that there are countless versions of you running around in what could be an infinite number of parallel universes.

This time, I’m going to introduce a controversial proposal by MIT physicist Max Tegmark, that uses these parallel universes to argue that you might actually be immortal.

Aug 27, 2019

Physicists Just Released Step-by-Step Instructions for Building a Wormhole

Posted by in categories: cosmology, physics, space travel

I am going home :3.


Everybody wants a wormhole. I mean, who wants to bother traveling the long-and-slow routes throughout the universe, taking tens of thousands of years just to reach yet another boring star? Not when you can pop into the nearest wormhole opening, take a short stroll, and end up in some exotic far-flung corner of the universe.

There’s a small technical difficulty, though: Wormholes, which are bends in space-time so extreme that a shortcut tunnel forms, are catastrophically unstable. As in, as soon as you send a single photon down the hole, it collapses faster than the speed of light.

Aug 27, 2019

Experiments with a single atom rule out the ‘fifth force’ theory of dark energy

Posted by in categories: cosmology, particle physics

We still don’t know what dark energy is, but we have a better idea of what it isn’t.

Aug 26, 2019

Simulation of eight million ‘mock universes’ sheds light on galaxy evolution

Posted by in categories: cosmology, evolution, physics

Physics World represents a key part of IOP Publishing’s mission to communicate world-class research and innovation to the widest possible audience. The website forms part of the Physics World portfolio, a collection of online, digital and print information services for the global scientific community.

Aug 26, 2019

New theory draws connections between Planckian metals and black holes

Posted by in categories: cosmology, information science, particle physics, quantum physics

Two researchers at Harvard University, Aavishkar A. Patel and Subir Sachdev, have recently presented a new theory of a Planckian metal that could shed light on previously unknown aspects of quantum physics. Their paper, published in Physical Review Letters, introduces a lattice model of fermions that describes a Planckian metal at low temperatures (Tà 0).

Metals contain numerous , which carry . When physicists consider the electrical resistance of metals, they generally perceive it as arising when the flow of current-carrying electrons is interrupted or degraded due to electrons scattering off impurities or off the crystal lattice in the metal.

“This picture, put forth by Drude in 1900, gives an equation for the electrical resistance in terms of how much time electrons spend moving freely between successive collisions,” Patel told Phys.org. “The length of this time interval between collisions, called the ‘,’ or ‘electron liftetime,’ is typically long enough in most common metals for the electrons to be defined as distinct, mobile objects to a microscopic observer, and the Drude picture works remarkably well.”

Aug 23, 2019

Do Doors to Interdimensional Travel Exist?

Posted by in category: cosmology

Idk how I found this o.o


Last year we looked at multiverse theory and the highly speculative — but very real — science behind what has become a pop culture phenomenon. It isn’t just “Stranger Things” anymore. Interdimensional travel, and the portals that might allow it, are everywhere these days.

So, how to open a portal to another dimension?

Continue reading “Do Doors to Interdimensional Travel Exist?” »

Aug 23, 2019

How We Recreated The Early Universe In The Laboratory

Posted by in categories: cosmology, particle physics

One of the all-time great mysteries in physics is why our universe contains more matter than antimatter, which is the equivalent of matter but with the opposite charge. To tackle this question, our international team of researchers have managed to create a plasma of equal amounts of matter and antimatter – a condition we think made up the early universe.

Matter as we know it appears in four different states: solid, liquid, gas, and plasma, which is a really hot gas where the atoms have been stripped of their electrons. However, there is also a fifth, exotic state: a matter-antimatter plasma, in which there is complete symmetry between negative particles (electrons) and positive particles (positrons).

This peculiar state of matter is believed to be present in the atmosphere of extreme astrophysical objects, such as black holes and pulsars. It is also thought to have been the fundamental constituent of the universe in its infancy, in particular during the Leptonic era, starting approximately one second after the Big Bang.

Aug 23, 2019

Star crust is 10 billion times stronger than steel

Posted by in categories: cosmology, physics

By Rachel Courtland

The crust of neutron stars is 10 billion times stronger than steel, according to new simulations. That makes the surface of these ultra-dense stars tough enough to support long-lived bulges that could produce gravitational waves detectable by experiments on Earth.

Neutron stars are the cores left behind when relatively massive stars explode in supernovae. They are incredibly dense, packing about as much mass as the sun into a sphere just 20 kilometres or so across, and some rotate hundreds of times per second.