Abstract
In this paper we show a segregated universe in terms of Tolman–Bondi equations of pressure-free spherically symmetric systems of particles in general relativity . We demonstrate the agreement between our model of segregation with a size of astrophysical structures by using a comparison between quantum and astrophysical quantities. This is made within the framework of Mohamed El Naschie's ε (∞) Cantorian space–time.
Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
