Editing Strange star (section)

==Strange dwarf stars==
Hypothetical strange-quark dwarfs would be [[white dwarf stars]] with strange-quark cores. Some studies predict these objects would be stable, while others predict instability.<ref>{{Cite book |last1=Di Clemente |first1=Francesco |url=https://www.mdpi.com/2218-1997/10/8/322 |title=Universe |last2=Drago |first2=Alessandro |last3=Pagliara |first3=Giuseppe |date=2024-08-09 |volume=10 |pages=322 |language=en |doi=10.3390/universe10080322 |doi-access=free |issn=2218-1997}}</ref> A survey examined the mass–radius relation for 40,000 white dwarfs and found eight exceptions were much smaller in size and matched predictions for a strange dwarf.<ref>{{Cite journal|arxiv=2012.05748|title=Searching for strange quark matter objects among white dwarfs|first1=Abdusattar|last1=Kurban|first2=Yong-Feng|last2=Huang|first3=Jin-Jun|last3=Geng|first4=Hong-Shi|last4=Zong|journal=Physics Letters B |date=May 27, 2022|volume=832 |page=137204 |doi=10.1016/j.physletb.2022.137204 |bibcode=2022PhLB..83237204K |s2cid=228083632 }}</ref>