Digital Asymmetric Wormhole-Like Object

In the context of digital physics, we can create a model for an asymmetric wormhole-like object with an inner region bounded by a 2-sphere radius and an asymptotically flat exterior. We can modify the radial function to incorporate the discrete nature of spacetime. Let's denote the modified line element for this asymmetric wormhole-like object as

$�{�}^2$.

The line element for this asymmetric wormhole-like object can be expressed as follows:

$�{�}^2=-(1-\frac{2�}{{�}_1}-\frac{2�}{{�}_2})�{�}^2+\frac{�{�}^2}{(1-\frac{2�}{�})}+{�}^2�{\mathrm{\Omega }}^2$

Here:

• $�{�}^2$ represents the modified line element of the asymmetric wormhole-like object in digital spacetime.
• $�$ represents the mass parameter of the object.
• ${�}_1$ and ${�}_2$ represent the discrete radial coordinates of the inner and outer boundaries, respectively.
• $�$ represents the discrete radial coordinate within the object.
• $��$ represents the discrete time interval between events.
• $�{\mathrm{\Omega }}^2$ represents the discrete angular components.

In this model, the inner region of the object is bounded by a 2-sphere with radius ${�}_1$. As $�$ moves from ${�}_1$ towards ${�}_2$, the spacetime geometry transitions from the inner region to the asymptotically flat exterior. The radial function is modified to reflect the discrete nature of spacetime in digital physics.

Please note that this representation provides a conceptual framework for an asymmetric wormhole-like object within the context of digital physics. The specific form of the radial function and the discrete intervals would depend on the rules and properties defined within the digital universe being modeled. Adjustments and refinements can be made based on the particular characteristics and constraints of the digital spacetime being considered.