Use my Search Websuite to scan PubMed, PMCentral, Journal Hosts and Journal Archives, FullText. Kick-your-searchterm to multiple Engines kick-your-query now !>

A dictionary by aggregated review articles of nephrology, medicine and the life sciences Your one-stop-run pathway from word to the immediate pdf of peer-reviewed on-topic knowledge.

10.1140/epjc/s10052-017-5046-8 http://scihub22266oqcxt.onion/10.1140/epjc/s10052-017-5046-8 C5586974!5586974!28943798     free     free     free Warning: file_get_contents(https://eutils.ncbi.nlm.nih.gov/entrez/eutils/elink.fcgi?dbfrom=pubmed&id=28943798&cmd=llinks): Failed to open stream: HTTP request failed! HTTP/1.1 429 Too Many Requests in C:\Inetpub\vhosts\kidney.de\httpdocs\pget.php on line 215 Warning: imagejpeg(C:\Inetpub\vhosts\kidney.de\httpdocs\phplern\28943798.jpg): Failed to open stream: No such file or directory in C:\Inetpub\vhosts\kidney.de\httpdocs\pget.php on line 117       Eur+Phys+J+C+Part+Fields 2017 ; 77 (7): ä Nephropedia Template TP {{tp|p=28943798|t=2017. Impact of topology in foliated quantum Einstein gravity |pdf=|usr=}}{{28943798}} gab.com Text Impact of topology in foliated quantum Einstein gravity JO: Eur Phys J C Part Fields http://www.kidney.de/pget.php?&tw=1&pmid=28943798 #FOAvip We use a functional renormalization group equation tailored to the Arnowitt?Deser?Misner formulation of gravity to study the scale dependence of Newton?s coupling and the cosmological constant on a background spacetime with topology \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$S^1 \times S^d$$\end{document}S1×Sd. The resulting beta functions possess a non-trivial renormalization group fixed point, which may provide the high-energy completion of the theory through the asymptotic safety mechanism. The fixed point is robust with respect to changing the parametrization of the metric fluctuations and regulator scheme. The phase diagrams show that this fixed point is connected to a classical regime through a crossover. In addition the flow may exhibit a regime of ?gravitational instability?, modifying the theory in the deep infrared. Our work complements earlier studies of the gravitational renormalization group flow on a background topology \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$S^1 \times T^d$$\end{document}S1×Td (Biemans et al. Phys Rev D 95:086013, 2017, Biemans et al. arXiv:1702.06539, 2017) and establishes that the flow is essentially independent of the background topology. Twit Text FOAVip Impact of topology in foliated quantum Einstein gravity ????Eur Phys J C Part Fields http://www.kidney.de/pget.php?&tw=1&pmid=28943798 #FOAvip Twit Text # Free Paper on # # # # # LINK http://www.kidney.de/pget.php?&tw=1&pmid=28943798 #FOAvip English Wikipedia <ref>{{Cite pmid|28943798}}</ref> Impact of topology in foliated quantum Einstein gravity #MMPMID28943798 Houthoff WB; Kurov A; Saueressig F Eur Phys J C Part Fields 2017[]; 77 (7): ä PMID28943798show ga We use a functional renormalization group equation tailored to the Arnowitt?Deser?Misner formulation of gravity to study the scale dependence of Newton?s coupling and the cosmological constant on a background spacetime with topology \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$S^1 \times S^d$$\end{document}S1×Sd. The resulting beta functions possess a non-trivial renormalization group fixed point, which may provide the high-energy completion of the theory through the asymptotic safety mechanism. The fixed point is robust with respect to changing the parametrization of the metric fluctuations and regulator scheme. The phase diagrams show that this fixed point is connected to a classical regime through a crossover. In addition the flow may exhibit a regime of ?gravitational instability?, modifying the theory in the deep infrared. Our work complements earlier studies of the gravitational renormalization group flow on a background topology \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$S^1 \times T^d$$\end{document}S1×Td (Biemans et al. Phys Rev D 95:086013, 2017, Biemans et al. arXiv:1702.06539, 2017) and establishes that the flow is essentially independent of the background topology. äImpact of topology in foliated quantum Einstein gravity (epmc).pdf DeepDyve Pubget Overpricing