Our long-term goal is to develop a new supernova equation of state that meets the observational 2 M⊙ neutron star constraint and that includes quark matter. In this work, we perform a parameter scan to systematically investigate the hadron-quark phase transition in cold neutron stars using the state-of-the-art supernova equation of state HS(DD2) for the hadronic phase. We find neutron star configurations with maximum masses above 2 M⊙ and even above the maximum mass of HS(DD2). Our results show good agreement with other parameter scans.
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from #AlexandrosSfakianakis via Alexandros G.Sfakianakis on Inoreader http://ift.tt/2oLOayI via IFTTT
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Publication date: 18 April 2017 Source: Cell Reports, Volume 19, Issue 3 Author(s): David Estoppey, Chia Min Lee, Marco Janoschke, Boon He...
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Abstract Functionalised electrospun polyamide-6 (PA-6) nanofibres incorporating gadolinium oxide nanoparticles conjugated to zinc tetracar...
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Cytokine-dependent renewal of stem cells is a fundamental requisite for tissue homeostasis and regeneration. Spermatogonial progenitor cells...
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Yahoo Health Ken Brookes Lost 102 Pounds: 'I Never Want to Go Back to Being Unhealthy' Yahoo Health My wife died of ovarian ...
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Own a website? Manage your page to keep your users updated View some of our premium pages: . . . . Upgrade to a Premium Page from #Alexand...
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Abstract Background Cells in the intervertebral disc have unique phenotypes and marker genes that separate the nucleus pulposus (NP), an...
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Radiation Research, Volume 187, Issue 6 , Page 647-658, June 2017. from #AlexandrosSfakianakis via Alexandros G.Sfakianakis on Inoreader ...
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Publication date: Available online 23 February 2017 Source: Journal of Biomechanics Author(s): Lipika Parida, Udita Uday Ghosh, Venkat Pad...
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