Low-temperature dynamics of amorphous polymers and evolution over time of spectra of single impurity molecules: II. Model calculations and analysis of results

2003 ◽  
Vol 94 (6) ◽  
pp. 873-884 ◽  
Author(s):  
Yu. G. Vainer ◽  
A. V. Naumov ◽  
M. Bauer ◽  
L. Kador
Keyword(s):  
Low Temperature ◽  
Amorphous Polymers ◽  
Model Calculations ◽  
Single Impurity ◽  
Temperature Dynamics ◽  
Analysis Of Results ◽  
Over Time

scholarly journals Low-temperature dynamics in amorphous polymers and low-molecular-weight glasses—what is the difference?

2011 ◽  
Vol 13 (5) ◽  
pp. 1843-1848 ◽  
Author(s):  
Ivan Yu. Eremchev ◽  
Yury G. Vainer ◽  
Andrei V. Naumov ◽  
Lothar Kador
Keyword(s):  
Molecular Weight ◽  
Low Temperature ◽  
Amorphous Polymers ◽  
Low Molecular Weight ◽  
Temperature Dynamics ◽  
The Difference

Low temperature dynamics of surface and bulk electronic structure of quantum dots

2017 ◽  
Vol 4 (9) ◽  
pp. 094001
Author(s):  
G Krishnamurthy Grandhi ◽  
Renu Tomar ◽  
Ranjani Viswanatha
Keyword(s):  
Quantum Dots ◽  
Electronic Structure ◽  
Low Temperature ◽  
Temperature Dynamics

scholarly journals Low-temperature dynamics of magnetic colloids studied by time-resolved small-angle neutron scattering

2008 ◽  
Vol 77 (18) ◽  
Author(s):  
A. Wiedenmann ◽  
U. Keiderling ◽  
M. Meissner ◽  
D. Wallacher ◽  
R. Gähler ◽  
...  
Keyword(s):  
Low Temperature ◽  
Neutron Scattering ◽  
Small Angle ◽  
Small Angle Neutron Scattering ◽  
Time Resolved ◽  
Temperature Dynamics ◽  
Magnetic Colloids

The spectrum of gaseous methane at 77 K in the 1.1 – 2.6 μm region: a benchmark for planetary astronomy

1989 ◽  
Vol 67 (11) ◽  
pp. 1027-1035 ◽  
Author(s):  
A. R. W. McKellar
Keyword(s):  
Fourier Transform ◽  
High Resolution ◽  
Low Temperature ◽  
Spectral Resolution ◽  
Fourier Transform Spectrometer ◽  
Absorption Cell ◽  
Model Calculations ◽  
Testing Model ◽  
Medium Resolution ◽  
Spectrometer Data

The spectrum of CH4 obtained in CH4 plus N2 mixtures at a temperature of 77 K has been recorded with a spectral resolution of 0.14 cm−1 in the region 3800 to 9100 cm−1. The experiments were performed with long paths (66 or 88 m) in a cooled absorption cell using a Fourier-transform spectrometer. Data are presented here at low and medium resolution, and examples of some spectral regions are also shown at high resolution. The complete results are available from the author in an Appendix. Comparisons are made with previous model calculations of CH4 absorption, and with the observed spectrum of Neptune's satellite, Triton. The results should be useful for the interpretation of the spectra of Triton, Titan, and Pluto. They will also be of value for testing model calculations of low-temperature CH4 absorption, which, thus verified, can be used with greater confidence to analyze observations of Jupiter, Saturn Uranus, and Neptune.

Overview of Family Needs after Critical Illness: From Assessment to Intervention

1991 ◽  
Vol 2 (2) ◽  
pp. 220-226 ◽  
Author(s):  
Jane Stover Leske
Keyword(s):  
Critical Care ◽  
Critical Illness ◽  
Critically Ill ◽  
Critical Care Nurses ◽  
Nursing Interventions ◽  
Family Needs ◽  
Analysis Of Results ◽  
Family Centered ◽  
Primary Family ◽  
Over Time

Results of numerous independent studies suggest that families of a critically ill hospitalized member have similar needs that they can readily identify as very important. Empirical analysis of results compiled from many studies across patient populations, settings, geographic locations, and over time indicates that families have primary needs for assurance, proximity, and information. These primary family needs provide a research-based framework to guide critical care nurses in implementing and evaluating family-centered nursing interventions

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