“event horizon”可以造什么句，event horizon造句

The event horizon temperature of black holewith magnetic dipole moment

They have not only an outer event horizon but also an inner horizon, called a "Cauchy" horizon.

Using coordinate transformation, we study the event horizon of accelerating non-stationary black holes, the equation of event horizon surface is calculated out.

The trailing edge of the second pulse, therefore, also ACTS as an event horizon.

Hawking radiation:Radiation theoretically emitted from just outside the event horizon of a Black hole.

If, however, the pair appears on the edge of an event horizon, either particle or hole may wander across the horizon, never to return.

In effect, an event horizon has formed in the river, preventing waves from making their way out.

Essentially, the leading edge of the chasing pulse sucks it in, acting like the event horizon of a black hole.

It is pointed out that a coordinate or essential singularity near an event horizon will strongly influence the temperature of the horizon. It is a universal effect in 2-dimensional Riemann Space-time.

In his paper, Dokuchaev studies hypothetical orbits in the area between the event horizon and the singularity to understand their dynamics.

However, in1974, Hawking applied quantum field theory to the curved spacetime around the event horizon and discovered that black holes can emit thermal radiation, known as Hawking radiation.

So, a thermodynamic representation of the cosmic censor conjecture is proposed by us, as that it is forbidden that the temperature of an event horizon approaches zero or goes infinity.

As an example of non-stationary black holes,the relationship between the compression factor of time scale near the event horizon and the temperature as well as the change rate of entropy of the Vaidya black hole is researched.

Black holes are dense, but their event horizons preclude observations.

Therefore, you can never escape from inside the event horizon.

Thus, anything inside the event horizon, including a photon, is prevented from escaping across the event horizon by the extremely strong gravitational field.

The general event horizon formula of black hole is given from null hypersurface equation.

Using the method proposed by Zhao and Dai, the temperature of a black hole and event horizon are obtained.

When the event horizon of the black hole does not depend upon the advanced-time, the results can return to the well-known static case.

The "surface" of a black hole is the so-called event horizon, an imaginary surface surrounding the mass of the black hole.

"Stephen W. Hawking proposed in 1974 that subatomic particle pairs (photons, neutrinos, and some massive particles) arising naturally near the event horizon may result in one particle's escaping the vicinity of the black hole while the other particle, of negative energy, disappears into it."

Radii stop converging as they approach the event horizon, are parallel at the horizon, and begin diverging in the interior.

If you tell me what m is, I will tell you what the radius of the event horizon is.

一旦有物体穿过环绕该区域的所谓视界(event horizon)，它就注定有去无回。

The event horizon equation is given.

To the distant observer, the object, falling slower and slower, approaches but never reaches the event horizon.

At the event horizon, the escape velocity is equal to the speed of light.

From the object's frame of reference, it will cross the event horizon and reach the singularity, or center of the black hole, all within a finite amount of time.