107 Sentences With "general theory of relativity"

How to use general theory of relativity in a sentence? Find typical usage patterns (collocations)/phrases/context for "general theory of relativity" and check conjugation/comparative form for "general theory of relativity". Mastering all the usages of "general theory of relativity" from sentence examples published by news publications.

Einstein presented his general theory of relativity more than 100 years ago.
The scientists tested Albert Einstein's general theory of relativity, and it held.
Einstein presented his general theory of relativity more than 22017 years ago.
These waves were first predicted by Einstein's general theory of relativity in 1916.
The redshift agreed precisely with the values predicted by Einstein's general theory of relativity.
That was the whole point: acquiring direct evidence to support Einstein's General Theory of Relativity.
One side of the contest, gravity, is described by Albert Einstein's general theory of relativity.
The EHT photo also seems to, yet again, validate Albert Einstein's general theory of relativity.
Einstein's general theory of relativity is now renowned as a pinnacle of modern-day physics.
It confirmed the existence of gravitational waves, a key prediction of Einstein's general theory of relativity.
Anyone trying to make sense of these discoveries owes a debt to the general theory of relativity.
But those anomalies were accounted for by Albert Einstein, with gravity and the general theory of relativity.
That reading could go a long way toward confirming a part of Albert Einstein's general theory of relativity.
Opinion A century ago, astronomers proved the general theory of relativity — and made him a global household name.
When Albert Einstein first proposed his general theory of relativity in 1916, he didn't know the universe was expanding.
The average American has little at stake riding on whether the general theory of relativity is right or not.
Didn't Albert Einstein's general theory of relativity say gravity is a property of space-time, rather than a force?
These ripples are the last holdout from Einstein's general theory of relativity to have evaded confirmation by direct evidence.
Truly original contributions, such as Einstein's general theory of relativity, published in 1915, are cited extensively by later papers.
That fulfills Einstein's general theory of relativity and means we now have ears, in addition to eyes, on the universe.
Though it's not been decided, McChrystal would like it to be titled, "Leaders: A general theory of relativity," he said.
His wife Elsa donated a manuscript of his general theory of relativity to the university when it opened in 1925.
When physicists bring the Standard Model of particle physics and Einstein's general theory of relativity together they get a clear prediction.
As early as 28, Einstein had suggested a way to verify his outlandish proposal, known as the general theory of relativity.
Measurements of the star S0-2 allowed scientists to carry out a unique test of Einstein&aposs general theory of relativity.
Einstein's general theory of relativity is now more than 100 years old, and scientists have yet to find cracks in it.
The discovery with the Hubble Space Telescope is the first direct detection of a key prediction of Einstein's general theory of relativity.
Einstein predicted this phenomenon based on his overall theories about the curvature of space, put forth in his general theory of relativity.
Einstein's general theory of relativity describes gravity as a property of spacetime, a four-dimensional scaffolding that is ubiquitous in the universe.
Just like that, all of Einstein's major predictions from his general theory of relativity have now been borne out by direct observational evidence.
This latest study takes a different approach, modeling the boarding process using Lorentzian geometry—the mathematical foundation of Einstein's general theory of relativity.
Gravitational waves are faint ripples in the fabric of spacetime, first predicted by Albert Einstein as a consequence of his general theory of relativity.
Scientists could describe the geometry of spacetime around a non-rotating black hole in 1915, when Albert Einstein introduced his general theory of relativity.
In Albert Einstein's general theory of relativity, gravity is defined as the fabric of space and time — or "space-time" — bending around massive objects.
Einstein predicted the existence of gravitational waves with his general theory of relativity in 23, and physicists uncovered indirect evidence in the 22s and 22s.
Einstein predicted their existence in his general theory of relativity back in 1915, but he thought it would never be possible to test that prediction.
In Einstein's general theory of relativity, space has a geometry that makes it curve around objects, and in turn influences how those objects move in space.
They were predicted by Albert Einstein in 22024 as part of his general theory of relativity (which, despite its name, is really a theory of gravity).
This field aims to understand interactions on the smallest scales of the universe, where physical laws do not cohere with Albert Einstein's general theory of relativity.
Just over 100 years after he published his general theory of relativity, scientists have found what Albert Einstein predicted as part of the theory: gravitational waves.
Their existence was predicted, just over a century ago, by the mathematics of Albert Einstein's general theory of relativity, which is actually a theory of gravity.
The idea of gravitational waves emerged from the general theory of relativity, Albert Einstein's fundamental exposition of gravity, unveiled almost exactly 100 years before GW150914's discovery.
In 0.00043, a pair of Austrian mathematicians named Josef Lense and Hans Thirring were thinking through the implications of Albert Einstein's recently published general theory of relativity.
The new photo also proves part of Einstein's general theory of relativity (again), showing that the structure of the black hole is what Einstein expected it to be.
It was a major milestone that now allows astrophysicists to "hear" cosmic events like the merger of two black holes, and basically proves Einstein's general theory of relativity.
As predicted by Albert Einstein in his 2100 general theory of relativity, these cosmic disruptions emit energy in waveforms that travel at the speed of light and warp spacetime.
Next, his general theory of relativity would show that space could be curved and textured, like a taut rubber sheet stretched and formed by the masses of planets and stars.
As you approach one of these super-dense objects, the fabric of space and time becomes increasingly curved—equivalent to strengthening gravity, according to Albert Einstein's general theory of relativity.
Cue: Einstein In the early 20th century, Einstein went further with his general theory of relativity and showed that mass and gravity are linked to time; yet another unification moment.
When a gravitational wave passes through Earth, the distance between those mirrors should change ever so slightly as space-time contracts and expands, if Einstein's general theory of relativity holds.
By better measuring pulsars, and more of them, the telescope could open up a new way to explore the long-elusive gravitational waves predicted by Einstein's general theory of relativity.
In 1915, Einstein published his general theory of relativity, showing that gravity was a property of space and time, and the University of Göttingen was all abuzz with the the discovery.
For the second time, a group of scientists has detected gravitational waves, bringing more physical proof of the phenomenon Albert Einstein anticipated in his general theory of relativity a century ago.
Scientists announced Wednesday that they had observed starlight as it was warped by the gravity of another, more distant star - one of the key predictions of Einstein's general theory of relativity.
By studying S2 while it made its pass, the astronomers were able to confirm a crucial prediction of Einstein's general theory of relativity by turning nature into a readymade gravitational laboratory.
Gravitational waves In 20173, scientists were able to confirm that Albert Einstein was right when he predicted gravitational waves, or ripples in space-time, in his 1915 general theory of relativity.
But perhaps most important, researchers hope that the work will open up a new way to unify quantum theory with Einstein's general theory of relativity, which describes the structure of space-time.
Since 1974, Hawking worked extensively on marrying the two cornerstones of modern physics - Einstein's General Theory of Relativity, which concerns gravity and large-scale phenomena, and quantum theory, which covers subatomic particles.
But it occurred to him that she might make use of another kind of hole consistent with Albert Einstein's general theory of relativity: a tunnel or "wormhole" connecting distant locations in space-time.
That means a chapter discussing the possible shapes of the universe consistent with the general theory of relativity ends without discussing what its actual shape might be in the light of such discoveries.
They were able to hear, and record, the sound of that massive collision: a chirp with a rising tone, which is exactly what Einstein predicted would happen in his general theory of relativity.
Astronomers confirmed a key of part of Einstein's general theory of relativity in 2016 when they announced that the LIGO array had detected gravitational waves released by the collision of two black holes.
While some astronomers seek to use gravitational waves to understand the structure of cosmic objects, others want to employ this new era of astronomy to test the limits of the general theory of relativity.
The jets are subject to some of the funky stuff from Albert Einstein's general theory of relativity—for instance, time slows down for these jets since they're moving at speeds comparable to light speed.
From the ancient Babylonian study of cosmology, through Kepler's laws of planetary motion, to Newton's theory of gravity and Einstein's general theory of relativity, Dr. Stewart continues the journey up to modern-day controversies.
Einstein's General Theory of Relativity, pronounced in 13, suggested that matter and energy would warp the geometry of space-time the way a heavy sleeper sags a mattress, producing the effect we call gravity.
The Morgan has a collection of Einstein-related ephemera that includes correspondence and manuscripts, including the draft of an article about the general theory of relativity which Einstein was writing for the journal Nature.
Earlier this year, gravitational waves created by the merging of two black holes were detected, proving a key part of Albert Einstein's general theory of relativity, just over 100 years after it was first published.
In 2017, the project is finally projected to produce its first snapshot of the black hole and its immediate environment, which will shed light on these exotic objects and test the general theory of relativity.
Advertise on Hyperallergic with Nectar Ads A century has passed since Albert Einstein published his general theory of relativity, which at its core demonstrates that space and time are connected, and both involved in gravity.
A few months earlier, on May 29, 1919, Albert Einstein's general theory of relativity, positing that gravity could bend light beams, had been proven true through the observation of a solar eclipse by British scientists.
Observing these collisions can also help us answer a range of outstanding questions, such as how black holes work as cosmic particle accelerators, or whether Einstein's General Theory of Relativity is the correct description of nature.
The gravitational waves had been predicted by Einstein in 1916, as an outgrowth of his groundbreaking general theory of relativity, which depicted gravity as a distortion of space and time triggered by the presence of matter.
Even lifting an atomic clock up can change how long a tick appears to take: according to the general theory of relativity, time moves ever so slightly more slowly closer to the Earth than further away.
The seven lessons are about Einstein's general theory of relativity, quantum mechanics, the architecture of the cosmos, elementary particles, quantum gravity, probability and the heat of black holes and, finally, how humans fit into this picture.
Einstein in 1916 proposed the existence of gravitational waves as an outgrowth of his ground-breaking general theory of relativity, which depicted gravity as a distortion of space and time triggered by the presence of matter.
You may have heard of this guy named Albert Einstein who, among other things, fundamentally changed the way we thought about space and time when he published his general theory of relativity about a century ago.
Not only will such a discovery support a prediction that's essential to Albert Einstein's general theory of relativity, but it will also add to our understanding of the universe, said Szabolcs Marka, a physics professor at Columbia University.
Go deeper: When Einstein was developing the general theory of relativity 100 years ago, he predicted that gravity would act like a magnifying lens when a distant star passed by a closer object, brightening and bending the starlight.
Half a century before Einstein described gravity as "curved space" in his general theory of relativity, the equations describing curved space had appeared on the blackboards of mathematicians like Georg Friedrich Bernhard Riemann of Gottingen University in Germany.
Ultimately, physicists want to combine observations from these detectors with those from optical telescopes to both "see" and "hear" events like neutron stars colliding, which could explain the origins of heavy elements, and test Einstein's general theory of relativity.
Yes, the theoretical physicist made one of the most influential contributions to science of all time — the general theory of relativity, MC-something-or-other — but he was also a surprisingly funny dude who didn't take himself too seriously.
On May 29, 1919, the British astronomer Arthur Eddington photographed a solar eclipse, and in the process confirmed that starlight was bent by the sun's gravitational field in precisely the manner predicted by Albert Einstein's general theory of relativity.
Out There A team of scientists announced on Thursday that they had heard and recorded the sound of two black holes colliding a billion light-years away, a fleeting chirp that fulfilled the last prediction of Einstein's general theory of relativity.
They made the announcement on February 11, 2016: they'd been able to prove Einstein's 100-year-old general theory of relativity, about incredible disturbances in the cosmos causing a ripple (or a gravitational wave) in the fabric of space-time.
The bending of light was a key test for Einstein's general theory of relativity, which was published more than 100 years ago, and proven in 1919 when scientists measured the curving of starlight around the sun during a total solar eclipse.
"In this year of exceptional anniversaries -- 50 years after Apollo 11 and 100 years after the solar eclipse that proved Einstein's General Theory of Relativity -- we should not lose sight of one more," said Paul Hertz, Director of Astrophysics at NASA.
Einstein's 100-year-old general theory of relativity predicted that light from stars would be stretched to longer wavelengths by the extreme gravitational field of a black hole, and the star would appear redder, an effect known as gravitational red shift.
There's still a lot we don't know about gravity The thing is, there's still a lot we don't know about gravity, which, while successfully integrated with Einstein's general theory of relativity, still has issues in incorporating laws of quantum physics.
A team of scientists announced in February that they had heard and recorded the sound of two black holes colliding a billion light-years away, a fleeting chirp that fulfilled the last prediction of _________'s general theory of relativity. 8493.
Physicists who study LQG lack a clear understanding of how to zoom out from their network of space-time chunks and arrive at a large-scale description of space-time that dovetails with Einstein's general theory of relativity—our best theory of gravity.
While Einstein predicted them in his general theory of relativity in 1916, and their existence was indirectly demonstrated in the 1980s, it wasn't until the LIGO detector came online in 2002 that the hunt for elusive spacetime ripples started to get serious.
Observations from other eclipses through the centuries have provided important findings like the first descriptions of the sun's outer atmosphere, called the corona, measurements of the corona's intense heat, the discovery of helium and even verification of Einstein's General Theory of Relativity.
When Einstein formulated his general theory of relativity, the universe seemingly consisted of a single galaxy; today, we know not only that the universe has at least 100 billion galaxies, but that it is expanding, ballooning at a faster rate every second.
Based on the mathematics in Einstein's general theory of relativity of 2100, you would fall through the event horizon unscathed, then the force of gravity would pull you into a noodle and ultimately cram you into singularity, the black hole's infinitely dense core.
One of the big questions in physics is why the observed force of gravity around a galaxy is so much stronger than Einstein's general theory of relativity would predict, even at distances that are up to a hundred times the radius of the galaxy.
But other theories have become the foundation of modern science, such as the theory of evolution, the general theory of relativity, the theory of plate tectonics, the theory that the sun is at the center of the solar system, and the germ theory of disease.
He compares Einstein's general theory of relativity — which explains that the force of gravity, as we perceive it, actually arises from the curvature of space and time — to Mozart's "Requiem," Homer's "Odyssey," the Sistine Chapel and "King Lear" in terms of its soul-expanding qualities.
Today, what is known as the Hughes-Drever experiment is considered one of the most precise tests of the equivalence principle, which states that all masses in a gravitational field fall with the same acceleration — a key notion in Einstein's general theory of relativity.
The discovery stands to open up a whole new frontier of research in astronomy and astrophysics — one that may even take scientists beyond Einstein's general theory of relativity, Dave Reitze, a professor of physics at the University of Florida, and the executive director of LIGO, told CNBC.
Where else but on the Yiddish stage would a comic relish the opportunity to expound on Albert Einstein's general theory of relativity to a friend on a park bench: "If you're in a room with a woman, kissing her, an hour is like a minute," he explains.
To scientists, however, he will be forever known for finding a relation between gravity — in the form of Einstein's general theory of relativity — that bends the cosmos and determines its destiny and the atomic randomness that lives inside it, swept helplessly along in the river of time.
Although Einstein himself never really accepted it, his general theory of relativity predicted that if enough mass or energy were concentrated at one point, space would sag like mattress and eventually close itself off, creating a black hole from which nothing, not even light, could ever escape.
During a lecture at Caltech in the 1960s, the esteemed Richard Feynman first pointed out that the center of the Earth would be younger than the surface, owing to a fascinating outcome of Einstein's general theory of relativity: clocks run more slowly when positioned closer to a large gravitational mass.
When it was rebooted in the fall of 2015 for an engineering test a few days before the official search was to begin, and while the world was celebrating the 100th year anniversary of Albert Einstein's general theory of relativity, this upgraded LIGO, called Advanced LIGO, found a gravitational wave.
To help tease out the puny wiggle of a passing gravitational wave from a noisy background, LIGO's algorithms constantly compare the lengths of the twin detectors' arms, which oscillate when agitated by a passing gravitational wave or background noise, to "template waveforms" — possible gravitational-wave signals calculated from Einstein's general theory of relativity.
One hundred years ago, Albert Einstein used his newly discovered general theory of relativity (which implies that space itself responds to the presence of matter by curving, expanding or contracting) to demonstrate that each time we wave our hands around or move any matter, disturbances in the fabric of space propagate out at the speed of light, as waves travel outward when a rock is thrown into a lake.

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