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Newtonian and mechanics
Cosmology as a science originated with the Copernican principle, which implies that celestial bodies obey identical physical laws to those on Earth, and Newtonian mechanics, which first allowed us to understand those laws.
* Dark star ( Newtonian mechanics ), a star that has a gravitational pull strong enough to trap light under Newtonian gravity
The concept of a dynamical system has its origins in Newtonian mechanics.
The evidence was compiled by W de Sitter ( 1927 ) who wrote " If we accept this hypothesis, then the ' astronomical time ', given by the earth's rotation, and used in all practical astronomical computations, differs from the ' uniform ' or ' Newtonian ' time, which is defined as the independent variable of the equations of celestial mechanics ".
As intriguing as geometric Newtonian gravity may be, its basis, classical mechanics, is merely a limiting case of ( special ) relativistic mechanics.
Matching the theory's prediction to observational results for planetary orbits ( or, equivalently, assuring that the weak-gravity, low-speed limit is Newtonian mechanics ), the proportionality constant can be fixed as κ = 8πG / c < sup > 4 </ sup >, with G the gravitational constant and c the speed of light.
As in Newtonian mechanics, no system consisting of more than two particles can be solved with an exact analytical mathematical approach ( see 3-body problem ) and helium is no exception.
A brief comparison of inertial frames in special relativity and in Newtonian mechanics, and the role of absolute space is next.
The inadequacy of the notion of " absolute space " in Newtonian mechanics is spelled out by Blagojević:
Within the realm of Newtonian mechanics, an inertial frame of reference, or inertial reference frame, is one in which Newton's first law of motion is valid.
Newtonian mechanics makes the additional assumptions of absolute space and absolute time.
Einstein's theory of special relativity, like Newtonian mechanics, assumes the equivalence of all inertial reference frames, but makes an additional assumption, foreign to Newtonian mechanics, namely, that in free space light always is propagated with the speed of light c < sub > 0 </ sub >, a defined value independent of its direction of propagation and its frequency, and also independent of the state of motion of the emitting body.
This phenomenon of geodesic deviation means that inertial frames of reference do not exist globally as they do in Newtonian mechanics and special relativity.
In angular mechanics, torque is analogous to the Newtonian mechanics parameter of force, moment of inertia to mass, and angle to distance.
In Newtonian mechanics, Newton's laws of motion,
Newton's 1687 Philosophiæ Naturalis Principia Mathematica provided a detailed mathematical account of mechanics, using the newly developed mathematics of calculus and providing the basis of Newtonian mechanics.
Within the domain of classical mechanics, relativistic momentum closely approximates Newtonian momentum: at low velocity, is approximately equal to, the Newtonian expression for momentum.

Newtonian and which
These are fluids which one would expect to be less viscoelastic or more Newtonian because of their lower molecular weight.
In aerodynamics, air is normally assumed to be a Newtonian fluid, which posits a linear relationship between the shear stress ( the internal friction forces ) and the rate of strain of the fluid.
The effect of gravity on light was then explored by Johann Georg von Soldner ( 1801 ), who calculated the amount of deflection of a light ray by the sun, arriving at the Newtonian answer which is half the value predicted by general relativity.
For fluids which are sufficiently dense to be a continuum, do not contain ionized species, and have velocities small in relation to the speed of light, the momentum equations for Newtonian fluids are the Navier-Stokes equations, which is a non-linear set of differential equations that describes the flow of a fluid whose stress depends linearly on velocity gradients and pressure.
The result is a geometric formulation of Newtonian gravity using only covariant concepts, i. e. a description which is valid in any desired coordinate system.
Drawing further upon the analogy with geometric Newtonian gravity, it is natural to assume that the field equation for gravity relates this tensor and the Ricci tensor, which describes a particular class of tidal effects: the change in volume for a small cloud of test particles that are initially at rest, and then fall freely.
The model mimics the Newtonian law of gravity which also considers distance and physical size between two objects.
The Lorentz transformation supersedes the Galilean transformation of Newtonian physics, which assumes an absolute space and time ( see Galilean relativity ).
In addition, Maxwell's equations required that all electromagnetic waves in vacuum propagate at a fixed speed, c. As this can only occur in one reference frame in Newtonian physics ( see Galilean-Newtonian relativity ), the aether was hypothesized as the absolute and unique frame of reference in which Maxwell's equations hold.
This effect is basic to all Newtonian dynamics, which says that everything from sound to the trajectory of a thrown baseball should all remain the same in the aircraft as sitting still on the Earth.
Forces such as Newtonian gravity, which depend only on the scalar distance between objects, satisfy this criterion.
In Newtonian mechanics, the law of conservation of momentum can be derived from the law of action and reaction, which states that the forces between two particles are equal and opposite.
In relativity theory, orbits follow geodesic trajectories which approximate very well to the Newtonian predictions.
Note that that while bound orbits around a point mass or around a spherical body with an Newtonian gravitational field are closed ellipses, which repeat the same path exactly and indefinitely, any non-spherical or non-Newtonian effects ( as caused, for example, by the slight oblateness of the Earth, or by relativistic effects, changing the gravitational field's behavior with distance ) will cause the orbit's shape to depart from the closed ellipses characteristic of Newtonian two-body motion.
Note that the following is a classical ( Newtonian ) analysis of orbital mechanics, which assumes that the more subtle effects of general relativity, such as frame dragging and gravitational time dilation are negligible.
" Five years later, Albert Einstein published his paper on special relativity, which challenged the very simple set of rules laid down by Newtonian mechanics, which had been used to describe force and motion for over two hundred years.

Newtonian and can
Neither G nor M < sub >☉</ sub > can be measured to high accuracy in SI units, but the value of their product is known very precisely from observing the relative positions of planets ( Kepler's Third Law expressed in terms of Newtonian gravitation ).
In the Newtonian limit, i. e. when is sufficiently large compared to the Schwarzschild radius, the redshift can be approximated by a binomial expansion to become
As can be shown using simple thought experiments following the free-fall trajectories of different test particles, the result of transporting spacetime vectors that can denote a particle's velocity ( time-like vectors ) will vary with the particle's trajectory ; mathematically speaking, the Newtonian connection is not integrable.
Measurements in one inertial frame can be converted to measurements in another by a simple transformation ( the Galilean transformation in Newtonian physics and the Lorentz transformation in special relativity ).
The principle of simplicity can be used within Newtonian physics as well as in special relativity ; see Nagel and also Blagojević.
Essentially all experimental evidence that can distinguish between the theories agrees with relativity theory to within experimental measuremental accuracy, but the differences from Newtonian mechanics are usually very small ( except where there are very strong gravity fields and very high speeds ).
To this Newtonian approximation, for a system of two point masses or spherical bodies, only influenced by their mutual gravitation ( the two-body problem ), the orbits can be exactly calculated.
Newtonian fluids can be characterized by a single coefficient of viscosity for a specific temperature.
In Newtonian physics, however, no such acceleration can occur unless at least one of the objects is being operated on by a force.
In astronomy, the Arago spot can be also easily observed in the strongly defocussed image of a star in a Newtonian telescope.
The equations of Newtonian mechanics can exhibit sensitive dependence on initial conditions.
Strikingly, this mathematics can generate patterns of amazing complexity, but it also has the power to generate seemingly natural or organic shapes that defeat Newtonian geometry.
Some simple applications of Newtonian mechanics and / or materials sciences can supply correct approximations to the mechanics of many biological systems.
In this approach, the state of the system can be described by any type of generalized coordinates q ; the laws of motion need not be expressed in a Cartesian coordinate system, as was customary in Newtonian mechanics.
For instance, in Newtonian mechanics, an observed acceleration can be explained by reference to an applied force.
While not seriously advocated after Einstein's development of relativity, Newtonian gravity can be used to model the universe and non-rigorously derive the Friedmann equations that are used in the big bang universe.
A comparison can be made between Newtonian relativity and special relativity.
This can greatly reduce the sizes of such approximate frames, in comparison to Newtonian frames.
The translational part can be decoupled from the rotational part in standard Newtonian kinematics by considering the motion of the center of mass, and rotations of the rigid body about the center of mass.

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