2010
DOI: 10.1524/teme.2010.0043
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Zuverlässige Kalibrierung von pH-MesseinrichtungenTraceable Calibration of pH Measurement Devices

Abstract: Zusammenfassung DerpH-WertisteinewichtigeMessgröße zur Charakterisierung von wässrigen Lösungen und damit auch von biologischen Systemen. Von wenigen Ausnahmen der spektroskopischen Bestimmung abgesehen, wird der pH-Wert einer Lösung potenziometrisch, durch Messen der Kettenspannung einer pH-Messkette mit Glaselektrode mit Hilfe einer geeigneten pH-Messeinrichtung bestimmt. Eine Aussage darüber, ob der gemessene pH-Wert den Ansprüchen an die jeweilige Anwendung genügt, ist nur möglich, wenn die Zuverlässigkeit… Show more

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Cited by 3 publications
(3 citation statements)
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“…III, since κ is effectively a constant that controls the size of the kinetic function k 2 1 (ϕ) as can be seen in Eq. (21). We find that our numerical results for the evolution of dark energy are well approximated by the early dark energy parametrisation of Doran & Robbers [41], in which the dark energy density fraction is parametrised as follows:…”
Section: A Exponential Potentialsupporting
confidence: 54%
See 1 more Smart Citation
“…III, since κ is effectively a constant that controls the size of the kinetic function k 2 1 (ϕ) as can be seen in Eq. (21). We find that our numerical results for the evolution of dark energy are well approximated by the early dark energy parametrisation of Doran & Robbers [41], in which the dark energy density fraction is parametrised as follows:…”
Section: A Exponential Potentialsupporting
confidence: 54%
“…Such models are known as "growing neutrino quintessence" models [14,15], so called because the neutrino mass grows as the scalar field evolves. Growing neutrino quintessence models are closely related to "mass varying neutrino" (MaVaN) models, which also involve an interaction between dark energy and the neutrino mass [16][17][18][19][20][21][22][23]. As well as providing the right conditions for the scalar field to play the role of dark energy, the neutrino-scalar coupling can give rise to an attractive fifth-force acting on the neutrinos that is much stronger than gravity.…”
Section: Introductionmentioning
confidence: 99%
“…Note that due to the presence of a Majorana mass for the active neutrinos, the conclusion of Ref. [26] where a cascade of "nugget" formation occurs after the heaviest neutrino goes nonrelativistic does not apply.…”
Section: Acceleron As Dark Energymentioning
confidence: 96%