Which Has A Stronger Gravitational Pull - A Black Hole or Neutron Star?

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The gravitational pull of a black hole is generally stronger than that of a neutron star, primarily due to the black hole's ability to curve spacetime so significantly that not even light can escape. Neutron stars, while incredibly dense and with gravity about 2 billion times that of Earth, cannot bend light to the same extent as black holes. The strength of gravitational fields is determined by mass and distance from the center, meaning that at a fixed distance, a black hole and neutron star of equal mass would exert the same gravitational force. However, black holes typically contain more mass than neutron stars, leading to a stronger gravitational pull overall. Ultimately, the gravitational effects observed depend on the mass and density of the object in question.
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Is this established or is it dependent on the size of the black hole?

http://www.space.com/22180-neutron-stars.html

Neutron stars pack their mass inside a 20-kilometer (12.4 miles) diameter. They are so dense that a single teaspoon would weigh a billion tons — assuming you somehow managed to snag a sample without being captured by the body's strong gravitational pull. On average, gravity on a neutron star is 2 billion times stronger than gravity on Earth. In fact, it's strong enough to significantly bend radiation from the star in a process known as gravitational lensing, allowing astronomers to see some of the back side of the star.


How does that compare to a black hole's gravity?
 
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Its certainly the g-force of black hole that the greatest. In the words of Relativity, black hole not only curve the space-time like other celestial bodies(like neutron star) but also curve it so enormously the not even light could escape from it.
 
aditya ver.2.0 said:
Its certainly the g-force of black hole that the greatest. In the words of Relativity, black hole not only curve the space-time like other celestial bodies(like neutron star) but also curve it so enormously the not even light could escape from it.

Further to that, if you would aim a ray of light accurately enough towards a black hole, it can bend the ray so severely that it circles around the hole and comes back to you. A neutron star cannot do that.
 
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The strength of a gravitational field is determined solely by mass and distance from the center of gravity of an object. Oddities like the bending of light are only noticeable for compact [dense] objects. In such cases a light beam can pass close enough to encounter a region of severely curved spacetime. This does not happen for a normal density object. A light beam runs into the surface before it enters a region of severe curvature. The density of a black hole is so high it has a diameter of virtually zero, whereas a neutron star diameter is a little over a dozen kilometers. The diameter of an ordinary star is many thousands of kilometers.
 
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Chronos said:
The strength of a gravitational field is determined solely by mass and distance from the center of gravity of an object.
Furthermore, at a fixed distance, the strength of the gravitational field is dependent ONLY on the mass.

i.e. if you had a black hole and a neutron star and a normal star that (somehow) all massed the same, the g-force at distance X from the centre of the mass would be identical in all three cases. If you were at a million clicks distance, and your spaceship had no windows, you would have a tough time telling which of the three you were orbiting.

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The exterior solution of the Einstein's field equations are isomorphic in the two cases. Whether its a star, or a black hole, the metric and hence the 'force' or deflection of light rays is the same.

The only difference is that in the case of a stellar black hole, the actual mass of the central object is slightly greater than that of a Neutron star (its something like 3 stellar masses for a Neutron star, and greater than 4 stellar masses for a black hole). Of course you could imagine an eternal black hole with the same mass.
 
https://en.wikipedia.org/wiki/Recombination_(cosmology) Was a matter density right after the decoupling low enough to consider the vacuum as the actual vacuum, and not the medium through which the light propagates with the speed lower than ##({\epsilon_0\mu_0})^{-1/2}##? I'm asking this in context of the calculation of the observable universe radius, where the time integral of the inverse of the scale factor is multiplied by the constant speed of light ##c##.
Why was the Hubble constant assumed to be decreasing and slowing down (decelerating) the expansion rate of the Universe, while at the same time Dark Energy is presumably accelerating the expansion? And to thicken the plot. recent news from NASA indicates that the Hubble constant is now increasing. Can you clarify this enigma? Also., if the Hubble constant eventually decreases, why is there a lower limit to its value?
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