Примери за използване на Hole would на Английски и техните преводи на Български
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Black hole would result.
Even a stable microscopic black hole would be harmless.
The hole would be way too big.
A completely isolated black hole would not be visible.
The hole would need to be large and if it was rotating it might have a passage to another universe.
I told you one day his hole would be filled with greatness.
The total entropy of matter outside the black hole would go down.
But a bullet hole wouldn't make those markings.
Fold this over the middle of the floor,otherwise a hole would remain.
The hole would need to be large, and if it was rotating, it might have a passage to another universe.
After a long, long period of time the Black Hole would simply disappear.
A 100-solar-mass black hole would be roughly twice as massive as the theoretical limit.
Even an HH-60 helicopter with a top speed of 195 knots wouldn't get here for another 86 minutes, andthat's four minutes after the hole would be full of water.
But they also said that anyone who went through the hole would groove straight into a singularity, a black hole. .
The sending black hole would increase in mass, and the receiving black hole would decrease in mass, with each message sent.
To create a luminosity of 10(40) watts(the typical brightness of a quasar),a super-massive black hole would have to consume the material equivalent of 10 stars per year.
A giant black hole would have a gravitational pull so overwhelming it would hurl gas and stars around it at almost the speed of light.
The existence of alternative histories with black holes suggests this might be possible, the hole would need to be large, and if it was rotating, it might have a passage to another universe.
The hole was narrow, not inflamed, the pain was a little aching and tolerable, now it is not there at all(does the medicine relieve pain in the hole, or is everything so good and shouldn't hurt?)I was surprised that they said that the hole would heal itself(???) push the gauze with medicine.
With the first message, the receiving black hole would lose about 30% of its mass, and over subsequent messages, the black hole would disappear.
The existence of alternative histories with black holes suggests this might be possible,” reports from the Stockholm University suggested that,Hawking stated,“The hole would need to be large and if it was rotating it might have a passage to another universe.
This growth rate is so small that the tiny,black hole would only have absorbed a few milligrams of Earth's matter by the time the end of the universe arrived.
Whereas in ordinary three-dimensional space it takes a two-dimensional object(a surface) to create a boundary inside a black hole, in the bulk universe the event horizon of a 4D black hole would be a 3D object- a shape called a hypersphere.
At this temperature,a planet around a sufficiently cool black hole would receive 130 gigawatts of power, around a millionth of what the sun provides Earth.
He said:"A mountain-sized black hole would give off X-rays and gamma rays, at a rate of about 10 million megawatts, enough to power the world's electricity supply.
Suddenly I realised that if two black holes collided and merged,the area of the horizon of the final black hole would be greater than the sum of the areas of the original black holes. .
Mallary also discovered a feature that was not fully appreciated before:the fact that the effects of the singularity in the context of a rotating black hole would result in rapidly increasing cycles of stretching and squeezing on the spacecraft.
Or if two black holes collided and merged together to form a single black hole, the area of the event horizon of the final black hole would be greater than or equal to the sum of the areas of the event horizons of the original black holesFig.
Both the big bang and black holes would contain singularities, places where space and time come to an end, and the laws of physics break down.
These black holes would be smaller than stellar black holes formed from collapsing massive stars, said James Unwin, a physicist at the University of Chicago and co-author of the paper.