# On the Anisotropic Interior Solutions in Ho\v{r}ava Gravity and   Einstein-{\ae}ther Theory

**Authors:** Daniele Vernieri, Sante Carloni

arXiv: 1706.06608 · 2018-04-10

## TL;DR

This paper introduces a reconstruction algorithm for generating static spherically symmetric interior solutions with anisotropic fluids in Hořava gravity and Einstein-e6ther theory, revealing diverse stellar models and phenomenology.

## Contribution

It presents a novel reconstruction method to produce all interior solutions in these theories, focusing on static e6ther cases and exploring their rich phenomenology.

## Key findings

- Developed a comprehensive reconstruction algorithm.
- Generated a wide class of interior solutions.
- Analyzed an illustrative example in detail.

## Abstract

We find a reconstruction algorithm able to generate all the static spherically symmetric interior solutions in the framework of Ho\v{r}ava gravity and Einstein-\ae ther theory in presence of anisotropic fluids. We focus for simplicity on the case of a static \ae ther finding a large class of possible viable interior star solutions which present a very rich phenomenology. We study one illustrative example in more detail.

## Full text

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## Figures

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## References

29 references — full list in the complete paper: https://tomesphere.com/paper/1706.06608/full.md

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Source: https://tomesphere.com/paper/1706.06608