* amino acid* carbohydrate* chemical bond* chemical reaction* complementary base pair * compound* DNA* double helix* element* lipid* matter* monosaccharide* nucleic acid* nucleotide* organic compound* polynucleotide* polypeptide* polysaccharide* protein* RNA* saturated fatty acid* unsaturated fatty acid...
Halo abundance and structure play a central role for modeling structure formation and evolution. Without relying on a spherical or ellipsoidal collapse model, we analytically derive the halo mass function and cuspy halo density (inner slope of −4/3) based on the mass and energy cascade theory...
The nuclear matter parameters define the nuclear equation of state (EoS), they appear as coefficients of expansion around the saturation density of symmetric and asymmetric nuclear matter. We review their correlations with several properties of finite nuclei and of neutron stars within mean-field fram...
T Amelung, A Pohl, C Kaergel, G Tenbergen, H Gerwinn, S Mohnke, C Massau, W Matthias, S Weiß, V Marr, K M Beier, M Walter, J Ponseti, T H C Krüger, K Schiltz & H Walter Translational Psychiatry volume 7, page e1129 (2017)Cite this article 15k...
Stöckinger-Kim, The electroweak contributions to (g − 2)μ after the Higgs boson mass measurement, Phys. Rev. D 88 (2013) 053005 [arXiv:1306.5546] [INSPIRE]. Article ADS Google Scholar K. Melnikov and A. Vainshtein, Hadronic light-by-light scattering contribution to the muon ...
254–260.36In diesem Zusammenhang verkürzen soziologische Modelle massengesellschaftlichen Wahl-verhaltens, wie für die Jahrhundertmitte die von D.C. MOORE entwickelte Theorie der „de-ference“, die Vielgestaltigkeit der historischen Wirklichkeit ebenso, wie die Erklärung mitpolitischer ...
Mass-mailers and subsequent telephone screenings of 1100 people identified 299 candidates for invitation to an in-clinic assessment of general and neurological signs and symptoms, cognition, blood ω-3 status, and WMLs. The first clinic visit including ω-3 status yielded 233 candida...
It is also important to mention that the Fermi-Dirac statistics limits dark matter mass to be higher of few hundreds of eV, independent of the production mechanism [47], [48]. Therefore, a sub-keV dark matter model is perfectly conceivable once we invoke non-thermal processes. Moreover, ...
As it will be seen in next section, ϕ0 spans in the range ∼10−5 MP to MP, and therefore the inflaton mass 102 GeV ≲mϕ≲1011 GeV. 4 Reheating After the end of inflation, the universe is heated via the interactions between the inflaton and the SM Higgs. Before analyzing...
Scatter plots of projections of the results for the NUGM from MCMC runs with non-universal M1,2,3 but universal m0 and A0. These parameters and tanβ are allowed to vary over the ranges given in Eq. (4). We show the relic LSP density, Ωχh2 (top left); the Higgs mass, mH...