Examples of using Equivalence principle in English and their translations into Indonesian
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This argument is called the Equivalence principle.
The Strong Equivalence Principle says that this binding energy still will react gravitationally as if it were mass.
This connection between gravity and acceleration became known as the equivalence principle.
The equivalence principle is so important to modern physics that its depth and reach are still being debated and tested even today.
The scientists believe that this unique stellar laboratory will provide the best opportunityyet to discover a violation of a concept called the Equivalence Principle.
According to the equivalence principle of general relativity, the ratio of inertial mass to gravitational mass of all elementary particles is unity.
All evidence seems to indicate that the gravitational and inertial masses of a body are equal,as demanded by Einstein's equivalence principle of relativity;
In the strong equivalence principle, the gravitational result of the external white dwarf would be equal for both the internal white dwarf and the neutron star.
In 1968, the United Bible Societies(UBS) and the Vaticanentered into a joint agreement to undertake hundreds of new interconfessional Bible translation projects around the world, using functional equivalence principles.
Under the Strong Equivalence Principle, the gravitational effect of the outer white dwarf would be identical for both the inner white dwarf and the neutron star.
The principle that one can always find an inertial frame at every point of space and time in which physics follows thelaws in the absence of gravitation is called the Equivalence Principle.
The equivalence principle, which Albert Einstein used as a starting point for general relativity, proves to be a consequence of these principles. .
The reason for the appearance of a gravitational offset is Einstein's equivalence principle, which states that the effects of gravity on an object are indistinguishable from acceleration.
The equivalence principle, which Albert Einstein used as a starting point for general relativity, proves to be a consequence of these principles. .
The demanding demonstration of the technology also allowed them tolay the technical foundations for examining Einstein's equivalence principle using potassium and rubidium atomic interferometers under the MAIUS project.
This follows from Einstein's equivalence principle, which implies that in your immediate surrounding you cannot tell the difference between acceleration in flat space and curved space that gives rise to gravity.
Taking things a step further, the new way to measure gravity might prove useful for scientists trying to understand the nature of dark matter andto test other physics ideas, such as the equivalence principle.
This firewall, however, is incompatible with the equivalence principle that underlies general relativity, which holds that observers can't tell whether they have crossed the horizon.
Someone crossing the event horizon shouldn't actually feel any great hardship because an object would be in free fall and,based on the equivalence principle, that object- or person- would not feel the extreme effects of gravity.
To put it another way, at any point in spacetime the equivalence principle guarantees the existence of a local inertial frame, and an accelerometer measures the acceleration relative to that frame.
If our quasar observations are correct, then the accelerations of different materials differ by about one part in 1014--too small to see in the laboratory by a factor of about 100 but large enough to show up inplanned missions such as STEP(space-based test of the equivalence principle).
We now call this Einstein's equivalence principle, and it tells us that any accelerated reference frame cannot have its cause of acceleration determined by an object that's a part of the internal system.
All evidence seems to indicate that the gravitational and inertial masses of a body are equal,as demanded by Einstein's equivalence principle of relativity; so that at the same location equal(inertial) masses have equal weights.
The development of general relativity began with the equivalence principle, which the states of accelerated motion and being at rest in a gravitational field(for example when standing on the surface of Earth) are physically identical.
A good place free of air resistance to test this equivalence principle is Earth's Moon, and so in 1971, Apollo 15 astronaut David Scott dropped both a hammer and a feather together toward the surface of the Moon.
In this paper, Einstein outlined his"equivalence principle," which stated that observing an experiment on the Earth(with gravitational acceleration g) would be identical to observing an experiment in a rocket ship that moved at a speed of g.
This reasonable extrapolationbecame what is now known as the Einstein Equivalence Principle, or EEP:"In small enough regions of spacetime, the laws of physics reduce to those of special relativity; it is impossible to detect the existence of a gravitational field.".
The most famous experiments illustrating the equivalence principle are Galileo's reputed dropping of two balls of different weights from the Leaning Tower of Pisa and Apollo 15 astronaut Dave Scott's dropping of a hammer and a feather while standing on the airless surface of the Moon in 1971.