Aggregate modulus

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Template:One source Holeums are hypothetical stable, quantized gravitational bound states of primordial or micro black holes.

Introduction

Holeums were proposed by L.K. Chavda and Abhijit Chavda in 2002.[1] They have all the properties associated with cold dark matter. Holeums are not black holes, even though they are made up of black holes.

Properties of Holeums

The binding energy En of a Holeum that consists of two identical micro black holes of mass m is given by[2]

En=mc2αg24n2

in which n is the principal quantum number, n=1,2,... and αg is the gravitational counterpart of the fine structure constant. The latter is given by

αg=m2Gc=m2mP2

where:

is the Planck constant divided by 2π;
c is the speed of light in vacuum;
G is the gravitational constant.

The nth excited state of a Holeum then has a mass that is given by

mH=2m+Enc2

The Holeum's atomic transitions cause it to emit gravitational radiation.

The radius of the nth excited state of a Holeum is given by

rn=(n2Rαg2)(π28)

where:

R=(2mGc2) is the Schwarzschild radius of the two identical micro black holes that constitute the Holeum.

The Holeum is a stable particle. It is the gravitational analogue of the hydrogen atom. It occupies space. Although it is made up of black holes, it itself is not a black hole. As the Holeum is a purely gravitational system, it emits only gravitational radiation and no electromagnetic radiation. The Holeum can therefore be considered to be a dark matter particle.[3]

Macro Holeums and their properties

A Macro Holeum is a quantized gravitational bound state of a large number of micro black holes. The energy eigenvalues of a Macro Holeum consisting of k identical micro black holes of mass m are given by[4]

Ek=p2mc22nk2(1p26n2)2

where p=kαg and k2. The system is simplified by assuming that all the micro black holes in the core are in the same quantum state described by n, and that the outermost, kth micro black hole is in an arbitrary quantum state described by the principal quantum number nk.

The physical radius of the bound state is given by

rk=π2kRnk216p2(1p26n2)

The mass of the Macro Holeum is given by

Mk=mk(1p26n2)

The Schwarzschild radius of the Macro Holeum is given by

Rk=kR(1p26n2)

The entropy of the system is given by

Sk=k2S(1p26n2)

where S is the entropy of the individual micro black holes that constitute the Macro Holeum.

The ground state of Macro Holeums

The ground state of Macro Holeums is characterized by n= and nk=1. The Holeum has maximum binding energy, minimum physical radius, maximum Schwarzschild radius, maximum mass, and maximum entropy in this state.

Such a system can be thought of as consisting of a gas of k1 free (n=) micro black holes that is bounded and therefore isolated from the outside world by a solitary outermost micro black hole whose principal quantum number is nk=1.

Stability of Holeums

It can be seen from the above equations that the condition for the stability of Holeums is given by

p26n2<1

Substituting the relations p=kαg and αg=m2mP2 into this inequality, the condition for the stability of Holeums can be expressed as

m<mP(6)14(nk)12

The ground state of Holeums is characterized by n=, which gives us m< as the condition for stability. Thus, the ground state of Holeums is guaranteed to be always stable.

Black Holeums

A Holeum is a black hole if its physical radius is less than or equal to its Schwarzschild radius, i.e. if

rkRk

Such Holeums are termed Black Holeums. Substituting the expressions for rk and Rk, and simplifying, we obtain the condition for a Holeum to be a Black Holeum to be

mmP2(πnkk)12

For the ground state, which is characterized by nk=1, this reduces to

mmP2(πk)12

Black Holeums are an example of black holes with internal structure. Black Holeums are quantum black holes whose internal structure can be fully predicted by means of the quantities k, m, n, and nk.

Holeums and cosmology

Holeums are speculated to be the progenitors of a class of short duration gamma ray bursts.[5][6] It is also speculated that Holeums give rise to cosmic rays of all energies, including ultra-high-energy cosmic rays.[7]

References

43 year old Petroleum Engineer Harry from Deep River, usually spends time with hobbies and interests like renting movies, property developers in singapore new condominium and vehicle racing. Constantly enjoys going to destinations like Camino Real de Tierra Adentro.

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