Laboratory wavelengths for cosmological constraints on varying fundamental constants

Physica Scripta T

Volumn T134, Issue , 2009, Pages

  Aldenius, Maria ^a,b  

^a LUND UNIVERSITY   (Sweden)

^b EUROPEAN SOUTHERN OBSERVATORY   (Germany)

Author keywords

[No Author keywords available]

Indexed keywords

ATOMIC TRANSITION; FINE STRUCTURE CONSTANTS; FOURIER TRANSFORM SPECTROMETERS; FUNDAMENTAL CONSTANTS; HIGH DEGREE OF ACCURACY; HIGH RESOLUTION; HIGH-REDSHIFT; HOLLOW CATHODES; LINE STRUCTURES; PRESENT STATUS; PRESSURE SHIFT; QUASI-STELLAR OBJECTS; RELATIVE ACCURACY; RESONANCE LINE; RESONANCE TRANSITION; ULTRA-VIOLET; WAVE NUMBERS; WAVENUMBER SHIFTS;

ABSORPTION; ATOMS; CALIBRATION; COSMOLOGY; LABORATORIES; LIGHT; LIGHT SOURCES; RESONANCE; SEMICONDUCTOR QUANTUM DOTS; WAVELENGTH;

ATOMIC SPECTROSCOPY;

EID: 70350635973     PISSN: 02811847     EISSN: None     Source Type: Conference Proceeding    
DOI: 10.1088/0031-8949/2009/T134/014008     Document Type: Conference Paper

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