<?xml version="1.0" encoding="UTF-8"?>
<records>
<record>
<language>eng</language>
<publisher>Science and Education Publishing</publisher>
<journalTitle>International Journal of Physics</journalTitle>
<eissn>2333-4576</eissn>
<publicationDate>2018-11-19</publicationDate>
<volume>6</volume>
<issue>5</issue>
<startPage>161</startPage>
<endPage>165</endPage>
<doi>10.12691/ijp-6-5-4</doi>
<publisherRecordId>IJP2018654</publisherRecordId>
<documentType>article</documentType>
<title language="eng">The Momentum of New Matter Replaces Dark Energy and Explains the Expansion of the Universe</title>
<authors>
<author>
<name>Jarl-Thure Eriksson</name>
<email></email>
<affiliationId>1</affiliationId>
</author>
</authors>
<affiliationsList>
<affiliationName affiliationId="1">?bo Akademi University, Finland</affiliationName>

</affiliationsList>
<abstract language="eng">A new formulation of the Friedmann-Lema&#238;tre-Robertson-Walker equation has been developed in a previous paper. The present study analyses an alternative approach to the cosmological constant ' from the perspective of the so called CBU model (Continuously Breeding Universe). Instead of having a cosmological constant responsible for the expansion, an excess pressure is boosted by a &quot;bang factor&quot; β. It is assumed that expansion is caused by the continuous addition of matter, due to, say, electron-positron fluctuations. Even if only a fraction of virtual pairs &quot;stay alive&quot;, while the majority returns to nothingness, the phenomenon is vigorous enough to explain the expansion. The momentum change due to the inflow of new matter provides a force and accordingly a pressure explaining the expansion. An equation of said pressure is derived and then interpreted as the equivalent to the cosmological 'constant', Λeq. The momentum pressure provides a perfect match to the dark energy density.</abstract>
<fullTextUrl format="pdf">http://pubs.sciepub.com/ijp/6/5/4/ijp-6-5-4.pdf</fullTextUrl>
<keywords language="eng"><keyword>general relativity</keyword>
<keyword>cosmological constant</keyword>
<keyword>Friedmann's equation</keyword>
<keyword>Robertson-Walker metric</keyword>
<keyword>dark energy</keyword>
</keywords>
</record>
</records>
