The CMBR spectrum:: new upper limits for the distortion parameters y and μ

被引:4
作者
Battistelli, ES [1 ]
Fulcoli, V [1 ]
Macculi, C [1 ]
机构
[1] Univ Roma La Sapienza, Dept Phys, I-00185 Rome, Italy
关键词
instrumentation : detectors; cosmic microwave background; COBE-FIRAS; cosmology : theory; distortion parameters;
D O I
10.1016/S1384-1076(00)00014-2
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The CMBR Spectrum has been measured by the COBE-FIRAS experiment. Upper limits only have been found for distortion parameters y and mu: y(up) = 1.5 x 10(-5) and mu(up) = 9 x 10(-5) at 95% of confidence. FIRAS made differential measurements between sky and blackbody calibrator. The knowledge of its emissivity is important as far as y and mu measurements as concerned. We have re-estimated the XCAL emissivity by using Ray-Tracing techniques. Diffraction problems have been analyzed by a model based on waveguide approximation: it allowed us to define a propagation function tau inside the XCAL V-groove. The emission of the external calibrator distorted with respect to the Black-Body emission may result in lower upper limits to y and mu. New upper limits for distortion parameters y and mu have been calculated considering the new XCAL emissivity. The results are: y(up) = 3.1 x 10(-5) and mu(up) = 4.5 x 10(-4) at 95% of confidence. (C) 2000 Elsevier Science B.V. All rights reserved.
引用
收藏
页码:77 / 90
页数:14
相关论文
共 20 条
[11]  
MATHER J, 1990, ASTROPHYS J LETT, V354, P37
[12]   Calibrator design for the COBE far infrared absolute spectrophotometer (FIRAS) [J].
Mather, JC ;
Fixsen, DJ ;
Shafer, RA ;
Mosier, C ;
Wilkinson, DT .
ASTROPHYSICAL JOURNAL, 1999, 512 (02) :511-520
[13]  
NARASIMHAN N, 1971, P IEE, V118
[14]  
NARASIMHAN N, 1973, IEEE T ANTENNAS PROP, V21
[15]  
PEEBLES PJE, 1970, PHYSICAL COSMOLOGY
[16]  
PETERSON P, 1984, INT INFRARED J MILLI, V5
[17]  
SCHOOR S, 1950, J APPL PHYSICS, V21
[18]  
SIGNORE M, 1992, INFRARED SUBMILLIMET, P143
[19]   MICROWAVE BACKGROUND-RADIATION AS A PROBE OF THE CONTEMPORARY STRUCTURE AND HISTORY OF THE UNIVERSE [J].
SUNYAEV, RA ;
ZELDOVICH, YB .
ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS, 1980, 18 :537-560
[20]  
WILLIAMS J, 1969, J OPT SOC AM, V59