Skip to main content

Can energy be sucked out of a black hole?

Can energy be sucked out of a black hole?
 Can energy be sucked out of a black hole?

 A rotating region is such an extreme force of nature that it drags surrounding time and space around with it. So it's only natural to ask whether black holes might be used as some kind of energy source. In 1969, mathematical physicist Roger Penrose proposed a way to try to to just this, now referred to as the "Penrose Process."



The method might be employed by sophisticated civilizations (aliens or future humans) to reap energy by making "black hole bombs." a number of the physics required to try to to so, however, had never been experimentally verified — so far . Our study confirming the underlying physics has just been published in Nature Physics.

Around its event horizon (the boundary around a region beyond which nothing, not even light, can escape), a rotating region creates a neighborhood called the "ergosphere." If an object falls into the ergosphere in such how that it splits — with one part falling into the region and therefore the other escaping — the part that flees effectively gains energy at the expense of the region . So by sending objects or light toward a rotating region , we could get energy back.

But does this theory hold up? In 1971, the Russian physicist Yakov Zel'dovich translated it to other rotating systems that would be tested back on Earth. The region became a rotating cylinder made up of a cloth which will absorb energy.

Advertisement
Zel'dovich imagined that light waves could extract energy from the cylinder and become amplified. For the amplification effect to figure , however, these waves got to have something called "angular momentum," which twists them into spirals.

When twisted light waves hit such a cylinder, their frequency should change due to something called the "Doppler shift." you've got presumably experienced this when taking note of an ambulance siren. When it moves toward you it's a better pitch than when it moves faraway from you — the direction of travel changes the pitch of the sound. during a similar way, changes in rotational speed alter the perceived frequency of a light-weight wave.

If the cylinder rotates fast enough, the altered wave frequency should drop so low that it'll become negative (which simply means the wave spins within the opposite direction).

Positive frequency waves should be partly absorbed by the cylinder, losing energy. But the negative frequency waves would transform this loss into gain and instead become amplified by the cylinder. they might extract energy from the rotation, a bit like the thing escaping from Penrose's region .



Testing Zeldovich's theory may appear simple. But the rotating object must spin at an equivalent or higher frequency because the waves. To amplify light waves, which oscillate at a frequency of many trillions of times a second, you'd got to rotate an absorbing object billions of times faster than anything that's mechanically possible today.

Breakthrough eventually
Light travels at about 300 million meters per second. So to form the idea easier to check , we opted to use sound waves, which travel roughly 1,000,000 times slower, meaning we didn't need the absorber to rotate so quickly.

Advertisement
To create a twisted acoustic wave , we used a hoop of speakers all emitting an equivalent frequency but starting at slightly different times, therefore the sound follows a spiral. For our rotating absorber we used a bit of sound-absorbing foam attached to a motor. Microphones placed inside the froth allowed us to record the sound after it had interacted with the rotating absorber.

We found that when the froth span slowly (at a coffee frequency), the sound we recorded was quieter because it had been absorbed by the froth . But once we spun the froth fast enough for it to Doppler effect the frequency of the sound waves enough to form them negative, the sound became louder.

This can only mean that the acoustic wave had taken energy from our rotating absorber, finally proving the 50-year-old

Comments

Popular posts from this blog

What is space time?

What is space time? The fabric of space-time may be a conceptual model combining the three dimensions of space with the time of your time . consistent with the simplest of current physical theories, space-time explains the weird relativistic effects that arise from traveling near the speed of sunshine also because the motion of massive objects within the universe. Who discovered space-time?  The famous physicist Einstein helped develop the thought of space-time as a part of his theory of relativity. before his pioneering work, scientists had two separate theories to elucidate physical phenomena: Isaac Newton's laws of physics described the motion of massive objects, while James Clerk Maxwell's electromagnetic models explained the properties of sunshine , consistent with NASA. But experiments conducted at the top of the 19th century suggested that there was something special about light. Measurements showed that light always traveled at an equivalent speed, regardle

What is cosmic dust?

 What is cosmic dust? The Universe may be a very dusty place. cloud consists of small particles of solid material floating around within the space between the celebs . it's not an equivalent because the dust you discover in your house but more like smoke with small particles varying from collections of just a couple of molecules to grains of 0.1 mm in size. Dust is vital because we discover many it around young stars. actually it helps them to make , and it's also the staple from which planets just like the Earth are formed. The diagram below illustrates the cloud cycle. Dust is made in stars and is then blown off during a slow wind or a huge star explosion. The dust is then ‘recycled’ within the clouds of gas between stars and a few of it's consumed when subsequent generation of stars begins to make . Astronomers wont to consider dust as a nuisance because it absorbs the light from objects, keeping them hidden from our optical telescopes making the Universe app

How NASA Will Protect Astronauts From Space Radiation at the Moon

How NASA Will Protect Astronauts From Space Radiation at the Moon August 1972, as NASA scientist Ian Richardson remembers it, was hot. In Surrey, England, where he grew up, the fields were brown and dry, and other people tried to remain indoors — out of the Sun, televisions on. except for several days that month, his TV picture kept ending . “Do not adjust your set,” he recalls the BBC announcing. “Heat isn’t causing the interference. It’s sunspots.” The same sunspots that disrupted the tv signals led to enormous solar flares — powerful bursts of energy from the Sun — Aug. 4-7 that year. Between the Apollo 16 and 17 missions, the solar eruptions were a mishap for lunar explorers. Had they been in orbit or on the Moon’s surface, they might have experienced high levels of radiation sparked by the eruptions. Today, the Apollo-era flares function a reminder of the threat of radiation exposure to technology and astronauts in space. Understanding and predicting solar eruptions is cru