# Strangeon and Strangeon Star

**Authors:** Xiaoyu Lai (HUE), Renxin Xu (PKU)

arXiv: 1701.08463 · 2017-08-01

## TL;DR

This paper explores the concept of strangeon stars, a type of compact star composed of strangeons, proposing they could explain pulsar-like objects and offering a new perspective on the nature of dense matter in astrophysics.

## Contribution

It introduces the idea of strangeon stars as a new class of compact objects, expanding the Witten's conjecture to include strange cluster matter as stable.

## Key findings

- Strangeon stars can explain various pulsar-like phenomena.
- Strangeons are proposed as stable constituents of dense matter.
- Observational evidence may support the existence of strangeon stars.

## Abstract

The nature of pulsar-like compact stars is essentially a central question of the fundamental strong interaction (explained in quantum chromo-dynamics) at low energy scale, the solution of which still remains a challenge though tremendous efforts have been tried. This kind of compact objects could actually be strange quark stars if strange quark matter in bulk may constitute the true ground state of the strong-interaction matter rather than Fe^56 (the so-called Witten's conjecture). From astrophysical points of view, however, it is proposed that strange cluster matter could be absolutely stable and thus those compact stars could be strange cluster stars in fact. This proposal could be regarded as a general Witten's conjecture: strange matter in bulk could be absolutely stable, in which quarks are either free (for strange quark matter) or localized (for strange cluster matter). Strange cluster with three-light-flavor symmetry is renamed strangeon, being coined by combining "strange nucleon" for the sake of simplicity. A strangeon star can then be thought as a 3-flavored gigantic nucleus, and strangeons are its constituent as an analogy of nucleons which are the constituent of a normal (micro) nucleus. The observational consequences of strangeon stars show that different manifestations of pulsar-like compact stars could be understood in the regime of strangeon stars, and we are expecting more evidence for strangeon star by advanced facilities (e.g., FAST, SKA, and eXTP).

## Full text

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## Figures

4 figures with captions in the complete paper: https://tomesphere.com/paper/1701.08463/full.md

## References

41 references — full list in the complete paper: https://tomesphere.com/paper/1701.08463/full.md

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Source: https://tomesphere.com/paper/1701.08463