Ground state energy of a two particle gravitational atom

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SUMMARY

The ground state energy of a two-particle gravitational atom, consisting of two neutral spinless particles of mass m, can be derived using the Hamiltonian approach. The total Hamiltonian is expressed as Htotal = H1 + H2, leading to the equation Htotalψ12 = (E1 + E21ψ2. The Hamiltonian for a single particle is given by the equation (p2/2m) - (Gm2/x2), resulting in a second-order ordinary differential equation (ODE) that describes the system. The discussion highlights the challenge of quantizing energy without clear boundary conditions and suggests exploring the center of mass frame for a more familiar hydrogen atom analogy.

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  • Understanding of quantum mechanics principles, particularly Hamiltonian mechanics.
  • Familiarity with gravitational potential energy and its mathematical representation.
  • Knowledge of ordinary differential equations (ODEs) and their applications in quantum systems.
  • Concept of quantization and boundary conditions in quantum mechanics.
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  • Study the quantization of energy levels in gravitational systems.
  • Learn about the center of mass frame in multi-particle quantum systems.
  • Explore the mathematical techniques for solving second-order ordinary differential equations.
  • Investigate the similarities between gravitational atoms and hydrogen-like atoms in quantum mechanics.
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Students and researchers in quantum mechanics, particularly those interested in gravitational systems and energy quantization, as well as physicists exploring multi-particle interactions.

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Homework Statement



Two neutral spinless particles of mass m are gravitationally bound to one another. What is the ground state energy of this two-particle gravitational atom?

Homework Equations





The Attempt at a Solution



So, it's a two particle system, but

[tex]H_{total} = H_1 + H_2[/tex] and [tex]\psi_{12} = \psi_1 \psi_2[/tex] implies

[tex]H_{total} \psi_{12} = (H_1 + H_2) \psi_1 \psi_2 = (E_1 + E_2) \psi_1 \psi_2[/tex].

So I should be able to find the energy eigenvalues for one of the particles since they're identical, then (assuming spinless = zero spin = bosons), I should just be able to add the two ground state energies together.

My Hamiltonian for a single particle is

[tex]\frac{p^2}{2m} - \frac{Gm^2}{x^2} = -\frac{\hbar^2}{2m} \frac{\partial^2}{\partial x ^2} - \frac{Gm^2}{x^2}[/tex]

so I get an ODE of the form

[tex]\frac{\partial^2\psi}{\partial x^2} - \frac{2 G m^3}{\hbar^2 x^2}\psi + \frac{2 mE}{\hbar^2} \psi = 0[/tex]

What I don't see is how on Earth energy is quantized. I guess I am under the impression that to quantize any observable, we need boundary conditions (i.e., isn't it usually the presence of a boundary condition that causes quantization)? In any case, for a bound state, the total energy must be less than the potential for the system... but how do I fit that into this problem?

Or, option 2: have I set it up totally wrong? I could try to use the center of mass frame, in which things might start to look more like the hydrogen atom. Maybe I'll work on that until this gets some replies.
 
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What makes you think this is a one-dimensional problem? I would treat it in 3-d, just like the hydrogen atom, except that the constants are different.
 

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