The dimensionless form of Newton’s Law of Gravity in terms of Planck scale units can be expressed as follows,
where,
, is the Planck Force. The expression above must be modified in cases when the magnitude of gravity is very large. However, the modification must be done such that the expression above will simply become a special case when gravity is relatively weak. One such particular case where modification is needed for a large magnitude of gravity is the case of a black hole. Another one is the case of the magnitude of gravity by a large number of objects that collectively generate a gravitational effect like in the case of a galaxy or a galaxy cluster. The modification of Equation (
4) for both cases mentioned above was attempted, historically, by General Relativity theory and by MOND theory respectively. Here, as mentioned in the previous section, the proposed modification will be similar to Verlinde’s theory of emergent gravity where he primarily used
that represents the number of bits of information within the volume enclosed by the holographic screen. However, it is argued here that
gives only the entropy of virtual particles generated out of empty space inside the black hole and even those outside the event horizon that enter into the black hole. One must also consider the information associated with the real particles within the black hole which are either free particles or bounded particles within the atoms of gravitating matters inside the black hole. It is posited here that this consideration must also be true for non-black hole settings. For example, the maximum density of information given by all real particles in a 2-body system can be represented by the quantity
, where
are the masses of the two gravitating objects that are composed of real particles while
, and
represent the maximum possible density of information that can be stored for each real particles inside each of the gravitating matter. Now, a purely information-theoretic approach to gravity would be that the magnitude of gravity is dependent solely on the amount of information that resides in space and matter within a gravitational system. If gravity is strong enough such that it can generate virtual particles in empty space within the vicinity of the objects, that must be included in the general description of entropy within the system. Hence, the magnitude of gravity
F should only be dependent on the value of
N and
. The former represents the amount of information that resides in a gravitating matter and the latter, by the Holographic Principle, represents the amount of information within a given volume of space represented by the amount of energy generated due to gravity within the system. Gravity, therefore, in essence, would only be proportional to the information density. To quantify this, consider the square of
such that the ratio of the magnitude of the gravity and Planck Force is proportional to it, that is,
, for some unitless constant of proportionality
. This will yield us,
where, it can be shown that,
which is the usual expression for the magnitude of gravity in Newtonian Gravity (NG) except for the addition of the unitless quantity
. Hence, it can be said that the quantity,
, must also be an expression that measures the magnitude of gravity that is expressed in terms of the density or amount of information that resides within a gravitational system. Meanwhile, the quantity,
, is a magnitude of an excess gravity i.e., a “Hidden Gravity” (HG), in addition to the magnitude of gravity that is already given by the Newtonian equation of gravity. In terms of masses,
M and
m, for a two-body system, we can rewrite Equation (
5) as follows,
which can be simplified further as follows,
where
. This result is similar in a black hole setting where the addition of mass does not necessarily imply the addition of individual entropy. The increase in mass
M in a black hole by introducing a test object with mass
m, i.e.,
, increases the entropy within the volume occupied by
M but with total entropy greater than the sum of the individual entropy
and
of the masses, respectively. Thus,
, since the total entropy would become,
This similarity in a black hole scenario should not be surprising since when a particle is added to a gravitational system it not only increases the entropy of the system, but the addition of its mass also increases the magnitude of the gravity generated by the whole system. However, since it is posited here that the magnitude of gravity is proportional to the entropy, thus, the excess entropy,
, would then correspond to an excess gravity that is usually unaccounted for in calculating the magnitude of gravity if one is to use the classical equation of gravity. In
Section 3 and
Section 4, this new approach to gravity that relates gravity with the entropy of the system will be applied to larger systems that involve a large number of gravitating objects. This approach is different from the most commonly used approach in introducing a new theory of gravity where one is to generalize the Einstein-Hilbert action,
, by imposing additional parameters into the action, such as scalar, vector, tensor, and spinor fields, and then making the action conformally invariant in order to produce a new field equation for gravity. One of the well-known examples of this approach is the Tensor-Vector-Scalar (TeVeS) gravity theory by Bekenstein [
8] as a relativistic generalization of MOND paradigm of Milgrom [
9]. This Lagrangian method will not be used here since the model presented here will focus more on the relation of gravity with the information density within a gravitational system rather than on its energy density. In addition, the main difference between the proposed theory here with MOND theories is that the so-called “interpolating function”,
, that is added to Newton’s laws in MOND theories [
10] was identified and derived here to be a product of the function
f and the unitless constant
. It has a specific physical interpretation and is not just added, arbitrarily. To show this, note that the correction term
is a function in terms of mass ratio. In Observational Astronomy, one can never calculate the mass ratio by getting the individual masses of the gravitating objects since the mass of one celestial object can never be known separately from the other mass of a celestial object that is gravitationally bound to it. However, one can express the function
f in other terms instead of mass ratio. One of which is in terms of the acceleration of the two gravitating objects toward each other. For simplicity, let
which gives as,
. Using Newton’s second and third law,
which then gives the familiar modification of MOND theories to Newton’s gravity equation,
where
. In MOND theories, it was originally suggested by Milgrom that
would be the optimal value based on his analysis to rotation curve data. Here, the quantity,
, is not arbitrarily added without any physical meaning or justification. It is not a new fundamental constant that marks the transition between the Newtonian and deep-MOND regimes. It is interpreted here as the acceleration of the gravitating matter towards the test object orbiting it. However, there are complications in knowing the exact value of
, especially if the gravitating matter is a collection of smaller bodies with spaces in between like in the case of galaxies where there are different distributions of stars or density distribution within the galaxy. Such variation leads to various shapes and configurations of galaxies making the corresponding range of the gravitational influence around a galaxy unique for every galaxy. The mathematical details of this will be further discussed in
Section 4. This scenario for a galaxy is very different in the case of a black hole in which the are no pockets of different density distribution within the black hole since all its mass is only concentrated at that center called the singularity. However, the magnitude of the gravitational effect should be relatively the same with galaxy, hence describing the magnitude of gravity must also be the same for both cases.