Sentences with phrase «conserve momentum»

The equations conserve momentum, mass and energy across grid boundaries.

To conserve momentum there must be more going up than down, and in fact, all this excess momentum must eventually be carried by photons to outer space because otherwise the «trapping» molecules would end in the stratosphere.

Newton's law is wrong because it propagates changes instantaneously, and Newton's law with a light - speed delay is wrong because it doesn't conserve momentum.

However, the Exotic Perk on Merciless, Conserve Momentum, makes the weapon charge faster with each non-lethal hit.

Gearing is long and feels longer, because «triples» always sound as if they're revving less than they really are, so you tend to hang on to lower ratios and conserve momentum, finally reaching fifth for a relaxed motorway cruise.

To conserve momentum, both particles must have identical speeds.

The Sun and Moon (Digerati Distribution and Marketing): It's a platformer with a twist: You can dive into the ground, reversing your gravity while conserving your momentum.

Not exact matches

Campaigns in India have gained momentum against genetically engineered rice, including the Save our Rice network, the Folk Rice Movement and the Seed Mothers movement; all working to conserve and salvage thousands of traditional and indigenous seed varieties which would have otherwise been eroded by the onslaught of hybrid technology and conventional chemical inputs in the past decades.

We couldn't keep up the momentum without him in the second half but we conserved our energy for the big fight on Wednesday against Chelsea.

As the creation of giant reserves gains momentum, some fear such areas don't always conserve the habitats most in need.

For instance, if the winds that whip around the planet slow down, the Earth spins faster to conserve angular momentum.

Because momentum — created by the arm, absorbed by the rod, and passed into the thin fishing line — must be conserved, the tiny mass of the line achieves tremendous velocity, «especially at the end,» Kommers says.

For spirals, on the other hand, the gas infelt slowly conserving its angular momentum and stars formed steadily along a timescale comparable to the age of the Universe.

That's because the recipe exploits the fact that the black hole conserves angular momentum, so that its final spin is equal to its initial spin plus that of the electron.

At that time, a problem arose because it seemed that both energy and angular momentum were not conserved in beta - decay.

The spin of such cosmic objects is described by a conserved quantity called angular momentum, which accounts for both the speed of the rotating mass and its distance from the spin axis.

There are a variety of phonons, but to conserve the electron's momentum, these phonons have to be of a particular momentum and energy.

If you know of a mechanism whereby the Moon might be captured into a geocentric orbit whilst conserving angular momentum, please do let everyone know.

As always with physics, momentum is conserved so that the solar wind is correspondingly slowed down.»

Therefore, speed must decrease so that momentum is conserved.

The laws of physics state that momentum is always conserved in a system, in that it can neither be created nor destroyed, but rather can be transferred between colliding bodies.

Like in Valve's original games, momentum is conserved as you pass through a portal, allowing for all sorts of wacky, multiple portal chain reactions.

Momentum is conserved but gravity is reversed, letting you fling yourself high into the air or deep beneath the surface.

The complete quote is «Were angular momentum conserved this would lead to ridiculous spin rates, so it has long been known that angular momentum must be lost» -LRB-!)

We do know both mechanical energy and angular momentum are conserved quantities in any setup (with no dissipative processes, of course).

Also with angular momentum being conserved, it must fall.

They contain our best current understanding for how the physical processes interact (for instance, how evaporation depends on the wind and surface temperature, or how clouds depend on the humidity and vertical motion) while conserving basic quantities like energy, mass and momentum.

Like the dude who claims that momentum is not conserved.

4) I say that when air moves from a location with high rotational velocity (m / s following a circumference) to a location with a low angular velocity, the air will conserve angular momentum and hence be diverted at right angles to the the initial impetus, resulting (at the poles) in a vortex around the pole.

Basic physics tells us that as the diameter increases, the rate of rotation will slow in order to conserve angular momentum.

The requirement that both energy and angular momentum are conserved means that there's an unique connection between the rate of exchange of angular momentum and the rate of dissipation.

Since the 4 ms slowdown over 30 years was followed by a similar but slightly reduced speedup over the next 30 years, it is clear that a lot of the energy difference needed to conserve angular momentum had to have been stored elastically in the mantle rather than being dissipated to viscous heating of the mantle.

Otherwise, mass and energy will not be conserved and momentum balances get screwed up.

But as energy, momentum and mass must be conserved, the modeller must take an arbitrary decision what to do with this excess or deficit.

Indeed how do you want to validate something that just tries to conserve energy, mass and momentum on a grid with 100s km of size?

If a skater is spinning with out - stretched arms and they pull their arms closer into their body, the skater will begin to spin faster in order to conserve angular momentum.

The linear momentum, or just momentum must be conserved as you state.

Our planet as a whole conserves its angular momentum except for the known effects of external torque associated with the lunar - solar tide, which induces a gradual decelerating of the earth rotation velocity at a rate corresponding to the increase in the astronomic length of day (LOD) by about 1.4 millisecond per century (Munk and McDonald 1960).

It has definite momentum given by h * nu / c, and this has to be conserved.

Basically, I am aware that the model differencing schemes are specifically designed to conserve, mass, energy, linear and angular momentum, and vorticity.

I am pleased to hear that mass, momentum, and energy are conserved discretely.

In the so - called model numerics, a great deal of care is used in formulating the differential equation solution approach so as to explicitly conserve a number of quantities (mass, energy, water substance, angular momentum, linear momentum, vorticity) that are all important for the accurate representation of atmospheric dynamics.

Energy and momentum are conserved.

The density will continue to increase without limit, as the gravitational force increases due to the inverse square law of gravity, and the rotation will speed up, to conserve the angular momentum of the initial state, as the size decreases, so the moment of inertia continues to decline, and angular velocity increases to keep I. omega ^ 2 constant.

But the balls are compressible and momentum is conserved.

The Lagrangian of the molecule is an absolutely correct description of the state of the molecule; momentum and energy are absolutely conserved.

Scalar quantities have one continuity equation, conserved vector quantities like momentum have three.

And that dude Roger Peilke who thinks momentum is not conserved when friction heating occurs... sheesh!

I am concerned that in fact climate models do not discretely conserve mass, momentum, and energy.

In a vortex, turbulence is inhibited because when a particle of air moves inward, its tangential velocity increases to conserve angular momentum.