How strong gravity is when the neutrons are not together in the neutron star, and how gravity acts when they are separated?Neutron stars:The Neutrons stars have an intense field that can impact the orbits and other planets if they come close...
motion or spinning and there is not a visible reason for this motion and the invisible reason has an effect that appears to be caused by an object with a mass greater than three solar masses (too big to be a neutron star), then it is possible that a black hole is causing the motion...
Reflected light - Reflected light, usually in the form of glare (see explanation above), is light that has bounced off a reflective object to enter your eyes. Just like direct light, strong reflected light can make it difficult to perceive the details or directly view an object. Snow, water...
In order to investigate such systems, model approaches that include hadrons and quarks in a unified approach, will be discussed. Special attention will be given to high-density matter as it occurs in neutron stars. Given the current observational limits for neutron star masses, the properties of...
Alpha decay: A nucleus ejects two protons and two neutrons bound together, known as an alpha particle. Beta decay: A neutron becomes a proton, an electron and an antineutrino. The ejected electron is abeta particle. Spontaneous fission: A nucleus splits into two pieces. In the process, it...
That enormous explosion sends the outer bits of the star into space. All that is left is the collapsing center. If the center has enough matter, the strong gravity in the center squeezes it so much as it collapses that it turns into a black hole. Scientists think there may be as many...
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if a visible star or disk of gas has a "wobbling" motion or spinning and there is not a visible reason for this motion and the invisible reason has an effect that appears to be caused by an object with a mass greater than three solar masses (too big to be a neutron star), then it...
In the initial stage of the life of WDs, their evolution is governed by neutrino cooling via plasmon decay into neutrinos exiting the WD core [48, 49]. The cooling through plasmon decay could in principle be enhanced by strong magnetic fields or through the addition of new fields that could...
Shape of the Universe | Flat, Open & Closed from Chapter 28 / Lesson 10 55K Learn whether the universe is open, closed, or flat by examining cosmological models. Understand the different cosmological models and why a flat universe has strong evidence. Related...