Analysis of the Principle, Facility and Observation Applications for CMB Detection
DOI:
https://doi.org/10.54097/0kvn2c09Keywords:
CMB, inflation theory, cosmological parameters, Hubble constant, early universe.Abstract
The CMB, or Cosmic Microwave Background Radiation, stands as a cornerstone in the evolving understanding of the universe's fabric. This piece traces the CMB's journey, starting from its unexpected discovery by Arno Penzias and Robert Wilson back in 1964, which went on to play a crucial role in validating the Big Bang theory. Further, it unravels the challenge of the isotropy dilemma and sheds light on how inflation theory provided clarity. The CMB's significance spans a broad spectrum, offering a window into the primordial state of the universe, revealing nuances about density shifts and gravitational waves, and influencing realms like particle physics and cosmology. The study also touches upon the exciting strides being made in CMB studies, underscored by refined research methods and analytical advances. Additionally, the article underscores the CMB's contribution of the determine cosmological parameters, with a specific focus on employing the Sunyaev-Zel'dovich effect and the CMB's angular power spectrum to ascertain the Hubble constant (H0). As one looks ahead, further observations, increased precision, and refined calibration techniques hold the promise of advancing the comprehension of the CMB and its pivotal role in the realm of cosmology.
Downloads
References
Penzias A A, Wilson R W. A measurement of excess antenna temperature at 4080 MHz. A Source Book in Astronomy and Astrophysics, 1900–1975. Harvard University Press, 1979: 873-876.
Kamionkowski M, Kosowsky A. The cosmic microwave background and particle physics. Annual Review of Nuclear and Particle Science, 1999, 49(1): 77-123.
Kamionkowski M, Ratra B, Spergel D N, et al. CBR anisotropy in an open inflation, CDM cosmogony. arXiv preprint astro-ph/9406069, 1994.
Spergel D N, Bean R, Doré O, et al. Three-year Wilkinson Microwave Anisotropy Probe (WMAP) observations: implications for cosmology. The astrophysical journal supplement series, 2007, 170(2): 377.
Staggs S, Dunkley J, Page L. Recent discoveries from the cosmic microwave background: a review of recent progress. Reports on Progress in Physics, 2018, 81(4): 044901.
Ivezić Ž, Axelrod T, Brandt W N, et al. Large Synoptic Survey Telescope: From science drivers to reference design. Serbian Astronomical Journal, 2008 (176): 1-13.
Spergel D, Gehrels N, Baltay C, et al. Wide-field infrarred survey telescope-astrophysics focused telescope assets WFIRST-AFTA 2015 report. arXiv preprint arXiv:1503.03757, 2015.
Vavrek R D, Laureijs R J, Alvarez J L, et al. Mission-level performance verification approach for the Euclid space mission. Modeling, Systems Engineering, and Project Management for Astronomy VII. SPIE, 2016, 9911: 23-40.
Naess S, Hasselfield M, McMahon J, et al. The Atacama cosmology telescope: CMB polarization at 200< ℓ< 9000. Journal of Cosmology and Astroparticle Physics, 2014, 2014(10): 007.
Fixsen D J. The temperature of the cosmic microwave background. The Astrophysical Journal, 2009, 707(2): 916.
Fixsen D J, Cheng E S, Gales J M, et al. The cosmic microwave background spectrum from the full cobe* firas data set. The Astrophysical Journal, 1996, 473(2): 576.
Boggess N W. The Cosmic Background Explorer (COBE): Mission and Science Overview. Highlights of Astronomy, 1992, 9: 273-274.
Spergel D N, Verde L, Peiris H V, et al. First-year Wilkinson Microwave Anisotropy Probe (WMAP)* observations: determination of cosmological parameters. The Astrophysical Journal Supplement Series, 2003, 148(1): 175.
Kodali S K, Williams M R, Smith C R, et al. Two-year outcomes after transcatheter or surgical aortic-valve replacement. New England Journal of Medicine, 2012, 366(18): 1686-1695.
Benson B A, Ade P A R, Ahmed Z, et al. SPT-3G: a next-generation cosmic microwave background polarization experiment on the South Pole telescope. Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VII. SPIE, 2014, 9153: 552-572.
Tauber J A, Mandolesi N, Puget J L, et al. Planck pre-launch status: The Planck mission. Astronomy & Astrophysics, 2010, 520: A1.
Bertone G, Hooper D. History of dark matter. Reviews of Modern Physics, 2018, 90(4): 045002.
Burles S, Nollett K M, Turner M S. Big bang nucleosynthesis predictions for precision cosmology. The Astrophysical Journal, 2001, 552(1): L1.
Fields B D, Freese K, Graff D S. Massive compact halo objects viewed from a cosmological perspective: Contribution to the baryonic mass density of the universe. New Astronomy, 1998, 3(6): 347-361.
Bennett C L, Larson D, Weiland J L, et al. Nine-year Wilkinson Microwave Anisotropy Probe (WMAP) observations: final maps and results. The Astrophysical Journal Supplement Series, 2013, 208(2): 20.
Ade P A R, Aghanim N, Ahmed Z, et al. Joint analysis of BICEP2/Keck Array and Planck data. Physical review letters, 2015, 114(10): 101301.
Aylor K, Hou Z, Knox L, et al. A comparison of cosmological parameters determined from CMB temperature power spectra from the south pole telescope and the planck satellite. The Astrophysical Journal, 2017, 850(1): 101.
Downloads
Published
Issue
Section
License
Copyright (c) 2024 Highlights in Science, Engineering and Technology
This work is licensed under a Creative Commons Attribution-NonCommercial 4.0 International License.
