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Sunyaev–Zeldovich effect

August 23, 2023

The Sunyaev–Zeldovich effect (named after Rashid Sunyaev and Yakov B. Zeldovich and often abbreviated as the SZ effect) is the spectral distortion of the cosmic microwave background (CMB) through inverse Compton scattering by high-energy electrons in galaxy clusters, in which the low-energy CMB photons receive an average energy boost during collision with the high-energy cluster electrons. Observed distortions of the cosmic microwave background spectrum are used to detect the disturbance of density in the universe. Using the Sunyaev–Zeldovich effect, dense clusters of galaxies have been observed.

Overview

The Sunyaev–Zeldovich effect was predicted by Rashid Sunyaev and Yakov Zeldovich to describe anisotropies in the CMB. The effect is caused by the CMB interacting with high energy electrons. These high energy electrons cause inverse Compton scattering of CMB photons which causes a distortion in the radiation spectrum of the CMB. The Sunyaev–Zeldovich effect is most apparent when observing galactic clusters. Analysis of CMB data at higher angular resolution (high  -values) requires taking into account the Sunyaev–Zeldovich effect.

The Sunyaev–Zeldovich effect can be divided into different types:

  • Thermal effects, where the CMB photons interact with electrons that have high energies due to their temperature
  • Kinematic effects, a second-order effect where the CMB photons interact with electrons that have high energies due to their bulk motion (also called the Ostriker–Vishniac effect, after Jeremiah P. Ostriker and Ethan Vishniac.[1])
  • Polarization

The Sunyaev–Zeldovich effect is of major astrophysical and cosmological interest. It can help determine the value of the Hubble constant, determine the location of new galaxy clusters, and in the study of cluster structure and mass. Since the Sunyaev–Zeldovich effect is a scattering effect, its magnitude is independent of redshift, which means that clusters at high redshift can be detected just as easily as those at low redshift.

Thermal effects

The distortion of the CMB resulting from a large number of high energy electrons is known as the thermal Sunyaev–Zeldovich effect. The thermal Sunyaev–Zeldovich effect is most commonly studied in galaxy clusters. By comparing the Sunyaev–Zeldovich effect and X-ray emission data, the thermal structure of the cluster can be studied, and if the temperature profile is known, Sunyaev–Zeldovich data can be used to determine the baryonic mass of the cluster along the line of sight.[2] Comparing Sunyaev–Zeldovich and X-ray data can also be used to determine the Hubble constant using the angular diameter distance of the cluster.[3] These thermal distortions can also be measured in superclusters and in gases in the local group, although they are less significant and more difficult to detect. In superclusters, the effect is not strong (< 8 μK), but with precise enough equipment, measuring this distortion can give a glimpse into large-scale structure formation. Gases in the local group may also cause anisotropies in the CMB due to the thermal Sunyaev–Zeldovich effect which must be taken into account when measuring the CMB for certain angular scales.[2]

Kinematic effects

The kinematic Sunyaev–Zeldovich effect is caused when a galaxy cluster is moving relative to the Hubble flow. The kinematic Sunyaev–Zeldovich effect gives a method for calculating the peculiar velocity:

 
where   is the peculiar velocity, and   is the optical depth.[4] In order to use this equation, the thermal and kinematic effects need to be separated. The effect is relatively weak for most galaxy clusters. Using gravitational lensing, the peculiar velocity can be used to determine other velocity components for a specific galaxy cluster.[2] These kinematic effects can be used to determine the Hubble constant and the behavior of clusters.

Research

Current research is focused on modelling how the effect is generated by the intracluster plasma in galaxy clusters, and on using the effect to estimate the Hubble constant and to separate different components in the angular average statistics of fluctuations in the background. Hydrodynamic structure formation simulations are being studied to gain data on thermal and kinetic effects in the theory.[5] Observations are difficult due to the small amplitude of the effect and to confusion with experimental error and other sources of CMB temperature fluctuations. To distinguish the SZ effect due to galaxy clusters from ordinary density perturbations, both the spectral dependence and the spatial dependence of fluctuations in the cosmic microwave background are used.

A factor which facilitates high redshift cluster detection is the angular scale versus redshift relation: it changes little between redshifts of 0.3 and 2, meaning that clusters between these redshifts have similar sizes on the sky. The use of surveys of clusters detected by their Sunyaev–Zeldovich effect for the determination of cosmological parameters has been demonstrated by Barbosa et al. (1996). This might help in understanding the dynamics of dark energy in surveys (South Pole Telescope, Atacama Cosmology Telescope, Planck).

Observations

 
First measurements of the thermal Sunyaev–Zeldovich effect from the Atacama Large Millimeter Array with one of the most massive galaxy clusters known, RX J1347.5-1145.[6]

In 1984, researchers from the Cambridge Radio Astronomy Group and the Owens Valley Radio Observatory first detected the Sunyaev–Zeldovich effect from clusters of galaxies.[7] Ten years later, the Ryle Telescope was used to image a cluster of galaxies in the Sunyaev–Zeldovich effect for the first time.[8]

In 1987 the Cosmic Background Explorer (COBE) satellite observed the CMB and gave more accurate data for anisotropies in the CMB, allowing for more accurate analysis of the Sunyaev–Zeldovich effect.[2]

Instruments built specifically to study the effect include the Sunyaev–Zeldovich camera on the Atacama Pathfinder Experiment,[9] and the Sunyaev–Zeldovich Array, which both saw first light in 2005. In 2012, the Atacama Cosmology Telescope (ACT) performed the first statistical detection of the kinematic SZ effect.[10] In 2012 the kinematic SZ effect was detected in an individual object for the first time in MACS J0717.5+3745.[11]

As of 2015, the South Pole Telescope (SPT) had used the Sunyaev–Zeldovich effect to discover 415 galaxy clusters.[12] The Sunyaev–Zeldovich effect has been and will continue to be an important tool in discovering hundreds of galaxy clusters.

Recent experiments such as the OLIMPO balloon-borne telescope try to collect data in specific frequency bands and specific regions of the sky in order to pinpoint the Sunyaev–Zeldovich effect and give a more accurate map of certain regions of the sky.[13]

See also

References

  1. ^ Ostriker, Jeremiah P. & Vishniac, Ethan T. (1986). "Generation of Microwave Background Fluctuations from Nonlinear Perturbations at the Era of Galaxy Formation". Astrophysical Journal Letters. 306: L51. Bibcode:1986ApJ...306L..51O. doi:10.1086/184704.
  2. ^ a b c d Birkinshaw, M (March 1999). "The Sunyaev–Zel'dovich effect". Physics Reports. 310 (2–3): 97–195. arXiv:astro-ph/9808050. Bibcode:1999PhR...310...97B. doi:10.1016/S0370-1573(98)00080-5. hdl:1983/5d24f14a-26e0-44d3-8496-5843b108fec5. S2CID 119330362.
  3. ^ Birkinshaw, M.; Hughes, J. P. (January 1994). "A measurement of the Hubble constant from the X-ray properties and the Sunyaev-Zel'dovich effect of Abell 2218". The Astrophysical Journal. 420: 33. Bibcode:1994ApJ...420...33B. doi:10.1086/173540. ISSN 0004-637X.
  4. ^ Tartari, A.; Boella, G.; Candotti, M.; Gervasi, M.; Natale, V.; Passerini, A.; Sironi, G.; Zannoni, M. (9 July 2003). "Sunyaev Zel'dovich effect studies with MASTER". Memorie della Societa Astronomica Italiana Supplementi. 2: 44. arXiv:astro-ph/0307166. Bibcode:2003MSAIS...2...44T.
  5. ^ Cunnama D., Faltenbacher F.; Passmoor S., Cress C.; Cress, C.; Passmoor, S. (2009). "The velocity-shape alignment of clusters and the kinetic Sunyaev–Zeldovich effect". MNRAS Letters. 397 (1): L41–L45. arXiv:0904.4765. Bibcode:2009MNRAS.397L..41C. doi:10.1111/j.1745-3933.2009.00680.x. S2CID 9809159.
  6. ^ "ALMA's Hole in the Universe". eso.org. Retrieved 20 February 2017.
  7. ^ Birkinshaw, M.; Gull, S.F.; Hardebeck, H. (1984). "The Sunyaev-Zeldovich effect towards three clusters of galaxies". Nature. 309 (5963): 34–35. Bibcode:1984Natur.309...34B. doi:10.1038/309034a0. S2CID 4276748.
  8. ^ Saunders, Richard (26 November 1996). "Sunyaev-Zel'dovich observations with the Ryle Telescope". arXiv:astro-ph/9611213.
  9. ^ Schwan, D.; Ade, P. a. R.; Basu, K.; Bender, A. N.; Bertoldi, F.; Cho, H.-M.; Chon, G.; Clarke, John; Dobbs, M.; Ferrusca, D.; Güsten, R. (1 September 2011). "Invited Article: Millimeter-wave bolometer array receiver for the Atacama pathfinder experiment Sunyaev-Zel'dovich (APEX-SZ) instrument". Review of Scientific Instruments. 82 (9): 091301. arXiv:1008.0342. Bibcode:2011RScI...82i1301S. doi:10.1063/1.3637460. ISSN 0034-6748. PMID 21974566. S2CID 33402455.
  10. ^ Hand, Nick; Addison, Graeme E.; Aubourg, Eric; Battaglia, Nick; Battistelli, Elia S.; Bizyaev, Dmitry; Bond, J. Richard; Brewington, Howard; Brinkmann, Jon; Brown, Benjamin R.; Das, Sudeep; Dawson, Kyle S.; Devlin, Mark J.; Dunkley, Joanna; Dunner, Rolando; Eisenstein, Daniel J.; Fowler, Joseph W.; Gralla, Megan B.; Hajian, Amir; Halpern, Mark; Hilton, Matt; Hincks, Adam D.; Hlozek, Renée; Hughes, John P.; Infante, Leopoldo; Irwin, Kent D.; Kosowsky, Arthur; Lin, Yen-Ting; Malanushenko, Elena; et al. (2012). "Detection of Galaxy Cluster Motions with the Kinematic Sunyaev–Zeldovich Effect". Physical Review Letters. 109 (4): 041101. arXiv:1203.4219. Bibcode:2012PhRvL.109d1101H. doi:10.1103/PhysRevLett.109.041101. PMID 23006072. S2CID 11392448.
  11. ^ Mroczkowski, Tony; Dicker, Simon; Sayers, Jack; Reese, Erik D.; Mason, Brian; Czakon, Nicole; Romero, Charles; Young, Alexander; Devlin, Mark; Golwala, Sunil; Korngut, Phillip (10 December 2012). "A Multi-Wavelength Study of the Sunyaev-Zel'dovich Effect in the Triple-Merger Cluster Macs J0717.5+3745 with Mustang and Bolocam". The Astrophysical Journal. 761 (1): 47. arXiv:1205.0052. Bibcode:2012ApJ...761...47M. doi:10.1088/0004-637X/761/1/47. ISSN 0004-637X. S2CID 50951413.
  12. ^ Bleem, L. E.; Stalder, B.; de Haan, T.; Aird, K. A.; Allen, S. W.; Applegate, D. E.; Ashby, M. L. N.; Bautz, M.; Bayliss, M.; Benson, B. A.; Bocquet, S. (29 January 2015). "Galaxy Clusters Discovered Via the Sunyaev-Zel'dovich Effect in the 2500-Square-Degree SPT-Sz Survey". The Astrophysical Journal Supplement Series. 216 (2): 27. arXiv:1409.0850. Bibcode:2015ApJS..216...27B. doi:10.1088/0067-0049/216/2/27. hdl:1721.1/96784. ISSN 1538-4365. S2CID 6663564.
  13. ^ Nati, F.; et al. (1 March 2007). "The OLIMPO experiment". New Astronomy Reviews. 51 (3–4): 385–389. Bibcode:2007NewAR..51..385N. doi:10.1016/j.newar.2006.11.066. ISSN 1387-6473.

Further reading

  • Rephaeli, Y. (1995). "Comptonization of the Cosmic Microwave Background: The Sunyaev–Zeldovich Effect". Annual Review of Astronomy and Astrophysics. 33 (1): 541–580. Bibcode:1995ARA&A..33..541R. doi:10.1146/annurev.aa.33.090195.002545.
  • Barbosa, D.; Bartlett, J. G.; Blanchard, A.; Oukbir, J. (1996). "The Sunyaev–Zel'dovich effect and the value of Ω0". Astronomy and Astrophysics. 314: 13–17. arXiv:astro-ph/9511084. Bibcode:1996A&A...314...13B.
  • Birkinshaw, M.; Gull, S. F.; Hardebeck, H. (1984). "The Sunyaev–Zel'dovich effect towards three clusters of galaxies". Nature. 309 (5963): 34–35. Bibcode:1984Natur.309...34B. doi:10.1038/309034a0. S2CID 4276748.
  • Birkinshaw, Mark (1999). "The Sunyaev Zel'dovich Effect". Physics Reports. 310 (2–3): 97–195. arXiv:astro-ph/9808050. Bibcode:1999PhR...310...97B. doi:10.1016/S0370-1573(98)00080-5. hdl:1983/5d24f14a-26e0-44d3-8496-5843b108fec5. S2CID 119330362.
  • Cen, Renyue; Jeremiah P. Ostriker (1994). . The Astrophysical Journal. 431 (1994): 451. arXiv:astro-ph/9404011. Bibcode:1994ApJ...431..451C. CiteSeerX 10.1.1.254.3635. doi:10.1086/174499. S2CID 1284598. Archived from the original on 22 February 2004.
  • Hu, Jian; Yu-Qing Lou (2004). "Magnetic Sunyaev–Zel'dovich effect in galaxy clusters". Astrophysical Journal Letters. 606 (1): L1–L4. arXiv:astro-ph/0402669. Bibcode:2004ApJ...606L...1H. doi:10.1086/420896. S2CID 10520376.
  • Ma, Chung-Pei; J. N. Fry (27 May 2002). "Nonlinear Kinetic Sunyaev–Zel'dovich Effect". Physical Review Letters. 88 (21): 211301. arXiv:astro-ph/0106342. Bibcode:2002PhRvL..88u1301M. doi:10.1103/PhysRevLett.88.211301. PMID 12059470. S2CID 5655238.
  • Myers, A. D.; Shanks, T.; et al. (2004). "Evidence for an Extended SZ Effect in WMAP Data". Monthly Notices of the Royal Astronomical Society. 347 (4): L67–L72. arXiv:astro-ph/0306180. Bibcode:2004MNRAS.347L..67M. doi:10.1111/j.1365-2966.2004.07449.x. S2CID 53119165.
  • Springel, Volker; White, Martin; Hernquist, Lars (2001). "Hydrodynamic Simulations of the Sunyaev–Zel'dovich effect(s)". The Astrophysical Journal. 549 (2): 681–687. arXiv:astro-ph/0008133. Bibcode:2001ApJ...549..681S. doi:10.1086/319473. S2CID 6728519.
  • Sunyaev, R. A.; Ya. B. Zel'dovich (1970). "Small-Scale Fluctuations of Relic Radiation". Astrophysics and Space Science. 7 (1): 3–19. Bibcode:1970Ap&SS...7....3S. doi:10.1007/BF00653471. S2CID 117050217.
  • Sunyaev, R. A.; Ia. B. Zel'dovich (1980). "Microwave background radiation as a probe of the contemporary structure and history of the universe". Annual Review of Astronomy and Astrophysics. 18 (1): 537–560. Bibcode:1980ARA&A..18..537S. doi:10.1146/annurev.aa.18.090180.002541.
  • Diego, J. M.; Martinez, E.; Sanz, J. L.; Benitez, N.; Silk, J. (2002). "The Sunyaev–Zel'dovich effect as a cosmological discriminator". Monthly Notices of the Royal Astronomical Society. 331 (3): 556–568. arXiv:astro-ph/0103512. Bibcode:2002MNRAS.331..556D. doi:10.1046/j.1365-8711.2002.05039.x. S2CID 10486016.
  • Royal Astronomical Society, Corrupted echoes from the Big Bang? RAS Press Notice PN 04/01

External links

  • Corrupted echoes from the Big Bang? innovations-report.com.
  • Sunyaev–Zel'dovich effect on arxiv.org

August 23, 2023
sunyaev, zeldovich, effect, named, after, rashid, sunyaev, yakov, zeldovich, often, abbreviated, effect, spectral, distortion, cosmic, microwave, background, through, inverse, compton, scattering, high, energy, electrons, galaxy, clusters, which, energy, photo. The Sunyaev Zeldovich effect named after Rashid Sunyaev and Yakov B Zeldovich and often abbreviated as the SZ effect is the spectral distortion of the cosmic microwave background CMB through inverse Compton scattering by high energy electrons in galaxy clusters in which the low energy CMB photons receive an average energy boost during collision with the high energy cluster electrons Observed distortions of the cosmic microwave background spectrum are used to detect the disturbance of density in the universe Using the Sunyaev Zeldovich effect dense clusters of galaxies have been observed Contents 1 Overview 2 Thermal effects 3 Kinematic effects 4 Research 5 Observations 6 See also 7 References 8 Further reading 9 External linksOverview EditThe Sunyaev Zeldovich effect was predicted by Rashid Sunyaev and Yakov Zeldovich to describe anisotropies in the CMB The effect is caused by the CMB interacting with high energy electrons These high energy electrons cause inverse Compton scattering of CMB photons which causes a distortion in the radiation spectrum of the CMB The Sunyaev Zeldovich effect is most apparent when observing galactic clusters Analysis of CMB data at higher angular resolution high ℓ displaystyle ell values requires taking into account the Sunyaev Zeldovich effect The Sunyaev Zeldovich effect can be divided into different types Thermal effects where the CMB photons interact with electrons that have high energies due to their temperature Kinematic effects a second order effect where the CMB photons interact with electrons that have high energies due to their bulk motion also called the Ostriker Vishniac effect after Jeremiah P Ostriker and Ethan Vishniac 1 PolarizationThe Sunyaev Zeldovich effect is of major astrophysical and cosmological interest It can help determine the value of the Hubble constant determine the location of new galaxy clusters and in the study of cluster structure and mass Since the Sunyaev Zeldovich effect is a scattering effect its magnitude is independent of redshift which means that clusters at high redshift can be detected just as easily as those at low redshift Thermal effects EditThe distortion of the CMB resulting from a large number of high energy electrons is known as the thermal Sunyaev Zeldovich effect The thermal Sunyaev Zeldovich effect is most commonly studied in galaxy clusters By comparing the Sunyaev Zeldovich effect and X ray emission data the thermal structure of the cluster can be studied and if the temperature profile is known Sunyaev Zeldovich data can be used to determine the baryonic mass of the cluster along the line of sight 2 Comparing Sunyaev Zeldovich and X ray data can also be used to determine the Hubble constant using the angular diameter distance of the cluster 3 These thermal distortions can also be measured in superclusters and in gases in the local group although they are less significant and more difficult to detect In superclusters the effect is not strong lt 8 mK but with precise enough equipment measuring this distortion can give a glimpse into large scale structure formation Gases in the local group may also cause anisotropies in the CMB due to the thermal Sunyaev Zeldovich effect which must be taken into account when measuring the CMB for certain angular scales 2 Kinematic effects EditThe kinematic Sunyaev Zeldovich effect is caused when a galaxy cluster is moving relative to the Hubble flow The kinematic Sunyaev Zeldovich effect gives a method for calculating the peculiar velocity D T kin T CMB V p c t displaystyle Delta T text kin T text CMB frac V p c tau where V p displaystyle V p is the peculiar velocity and t displaystyle tau is the optical depth 4 In order to use this equation the thermal and kinematic effects need to be separated The effect is relatively weak for most galaxy clusters Using gravitational lensing the peculiar velocity can be used to determine other velocity components for a specific galaxy cluster 2 These kinematic effects can be used to determine the Hubble constant and the behavior of clusters Research EditCurrent research is focused on modelling how the effect is generated by the intracluster plasma in galaxy clusters and on using the effect to estimate the Hubble constant and to separate different components in the angular average statistics of fluctuations in the background Hydrodynamic structure formation simulations are being studied to gain data on thermal and kinetic effects in the theory 5 Observations are difficult due to the small amplitude of the effect and to confusion with experimental error and other sources of CMB temperature fluctuations To distinguish the SZ effect due to galaxy clusters from ordinary density perturbations both the spectral dependence and the spatial dependence of fluctuations in the cosmic microwave background are used A factor which facilitates high redshift cluster detection is the angular scale versus redshift relation it changes little between redshifts of 0 3 and 2 meaning that clusters between these redshifts have similar sizes on the sky The use of surveys of clusters detected by their Sunyaev Zeldovich effect for the determination of cosmological parameters has been demonstrated by Barbosa et al 1996 This might help in understanding the dynamics of dark energy in surveys South Pole Telescope Atacama Cosmology Telescope Planck Observations Edit First measurements of the thermal Sunyaev Zeldovich effect from the Atacama Large Millimeter Array with one of the most massive galaxy clusters known RX J1347 5 1145 6 In 1984 researchers from the Cambridge Radio Astronomy Group and the Owens Valley Radio Observatory first detected the Sunyaev Zeldovich effect from clusters of galaxies 7 Ten years later the Ryle Telescope was used to image a cluster of galaxies in the Sunyaev Zeldovich effect for the first time 8 In 1987 the Cosmic Background Explorer COBE satellite observed the CMB and gave more accurate data for anisotropies in the CMB allowing for more accurate analysis of the Sunyaev Zeldovich effect 2 Instruments built specifically to study the effect include the Sunyaev Zeldovich camera on the Atacama Pathfinder Experiment 9 and the Sunyaev Zeldovich Array which both saw first light in 2005 In 2012 the Atacama Cosmology Telescope ACT performed the first statistical detection of the kinematic SZ effect 10 In 2012 the kinematic SZ effect was detected in an individual object for the first time in MACS J0717 5 3745 11 As of 2015 the South Pole Telescope SPT had used the Sunyaev Zeldovich effect to discover 415 galaxy clusters 12 The Sunyaev Zeldovich effect has been and will continue to be an important tool in discovering hundreds of galaxy clusters Recent experiments such as the OLIMPO balloon borne telescope try to collect data in specific frequency bands and specific regions of the sky in order to pinpoint the Sunyaev Zeldovich effect and give a more accurate map of certain regions of the sky 13 See also EditSachs Wolfe effect Cosmic microwave background spectral distortionsReferences Edit Ostriker Jeremiah P amp Vishniac Ethan T 1986 Generation of Microwave Background Fluctuations from Nonlinear Perturbations at the Era of Galaxy Formation Astrophysical Journal Letters 306 L51 Bibcode 1986ApJ 306L 51O doi 10 1086 184704 a b c d Birkinshaw M March 1999 The Sunyaev Zel dovich effect Physics Reports 310 2 3 97 195 arXiv astro ph 9808050 Bibcode 1999PhR 310 97B doi 10 1016 S0370 1573 98 00080 5 hdl 1983 5d24f14a 26e0 44d3 8496 5843b108fec5 S2CID 119330362 Birkinshaw M Hughes J P January 1994 A measurement of the Hubble constant from the X ray properties and the Sunyaev Zel dovich effect of Abell 2218 The Astrophysical Journal 420 33 Bibcode 1994ApJ 420 33B doi 10 1086 173540 ISSN 0004 637X Tartari A Boella G Candotti M Gervasi M Natale V Passerini A Sironi G Zannoni M 9 July 2003 Sunyaev Zel dovich effect studies with MASTER Memorie della Societa Astronomica Italiana Supplementi 2 44 arXiv astro ph 0307166 Bibcode 2003MSAIS 2 44T Cunnama D Faltenbacher F Passmoor S Cress C Cress C Passmoor S 2009 The velocity shape alignment of clusters and the kinetic Sunyaev Zeldovich effect MNRAS Letters 397 1 L41 L45 arXiv 0904 4765 Bibcode 2009MNRAS 397L 41C doi 10 1111 j 1745 3933 2009 00680 x S2CID 9809159 ALMA s Hole in the Universe eso org Retrieved 20 February 2017 Birkinshaw M Gull S F Hardebeck H 1984 The Sunyaev Zeldovich effect towards three clusters of galaxies Nature 309 5963 34 35 Bibcode 1984Natur 309 34B doi 10 1038 309034a0 S2CID 4276748 Saunders Richard 26 November 1996 Sunyaev Zel dovich observations with the Ryle Telescope arXiv astro ph 9611213 Schwan D Ade P a R Basu K Bender A N Bertoldi F Cho H M Chon G Clarke John Dobbs M Ferrusca D Gusten R 1 September 2011 Invited Article Millimeter wave bolometer array receiver for the Atacama pathfinder experiment Sunyaev Zel dovich APEX SZ instrument Review of Scientific Instruments 82 9 091301 arXiv 1008 0342 Bibcode 2011RScI 82i1301S doi 10 1063 1 3637460 ISSN 0034 6748 PMID 21974566 S2CID 33402455 Hand Nick Addison Graeme E Aubourg Eric Battaglia Nick Battistelli Elia S Bizyaev Dmitry Bond J Richard Brewington Howard Brinkmann Jon Brown Benjamin R Das Sudeep Dawson Kyle S Devlin Mark J Dunkley Joanna Dunner Rolando Eisenstein Daniel J Fowler Joseph W Gralla Megan B Hajian Amir Halpern Mark Hilton Matt Hincks Adam D Hlozek Renee Hughes John P Infante Leopoldo Irwin Kent D Kosowsky Arthur Lin Yen Ting Malanushenko Elena et al 2012 Detection of Galaxy Cluster Motions with the Kinematic Sunyaev Zeldovich Effect Physical Review Letters 109 4 041101 arXiv 1203 4219 Bibcode 2012PhRvL 109d1101H doi 10 1103 PhysRevLett 109 041101 PMID 23006072 S2CID 11392448 Mroczkowski Tony Dicker Simon Sayers Jack Reese Erik D Mason Brian Czakon Nicole Romero Charles Young Alexander Devlin Mark Golwala Sunil Korngut Phillip 10 December 2012 A Multi Wavelength Study of the Sunyaev Zel dovich Effect in the Triple Merger Cluster Macs J0717 5 3745 with Mustang and Bolocam The Astrophysical Journal 761 1 47 arXiv 1205 0052 Bibcode 2012ApJ 761 47M doi 10 1088 0004 637X 761 1 47 ISSN 0004 637X S2CID 50951413 Bleem L E Stalder B de Haan T Aird K A Allen S W Applegate D E Ashby M L N Bautz M Bayliss M Benson B A Bocquet S 29 January 2015 Galaxy Clusters Discovered Via the Sunyaev Zel dovich Effect in the 2500 Square Degree SPT Sz Survey The Astrophysical Journal Supplement Series 216 2 27 arXiv 1409 0850 Bibcode 2015ApJS 216 27B doi 10 1088 0067 0049 216 2 27 hdl 1721 1 96784 ISSN 1538 4365 S2CID 6663564 Nati F et al 1 March 2007 The OLIMPO experiment New Astronomy Reviews 51 3 4 385 389 Bibcode 2007NewAR 51 385N doi 10 1016 j newar 2006 11 066 ISSN 1387 6473 Further reading EditRephaeli Y 1995 Comptonization of the Cosmic Microwave Background The Sunyaev Zeldovich Effect Annual Review of Astronomy and Astrophysics 33 1 541 580 Bibcode 1995ARA amp A 33 541R doi 10 1146 annurev aa 33 090195 002545 Barbosa D Bartlett J G Blanchard A Oukbir J 1996 The Sunyaev Zel dovich effect and the value of W0 Astronomy and Astrophysics 314 13 17 arXiv astro ph 9511084 Bibcode 1996A amp A 314 13B Birkinshaw M Gull S F Hardebeck H 1984 The Sunyaev Zel dovich effect towards three clusters of galaxies Nature 309 5963 34 35 Bibcode 1984Natur 309 34B doi 10 1038 309034a0 S2CID 4276748 Birkinshaw Mark 1999 The Sunyaev Zel dovich Effect Physics Reports 310 2 3 97 195 arXiv astro ph 9808050 Bibcode 1999PhR 310 97B doi 10 1016 S0370 1573 98 00080 5 hdl 1983 5d24f14a 26e0 44d3 8496 5843b108fec5 S2CID 119330362 Cen Renyue Jeremiah P Ostriker 1994 A hydrodynamic approach to cosmology the mixed dark matter cosmological scenario The Astrophysical Journal 431 1994 451 arXiv astro ph 9404011 Bibcode 1994ApJ 431 451C CiteSeerX 10 1 1 254 3635 doi 10 1086 174499 S2CID 1284598 Archived from the original on 22 February 2004 Hu Jian Yu Qing Lou 2004 Magnetic Sunyaev Zel dovich effect in galaxy clusters Astrophysical Journal Letters 606 1 L1 L4 arXiv astro ph 0402669 Bibcode 2004ApJ 606L 1H doi 10 1086 420896 S2CID 10520376 Ma Chung Pei J N Fry 27 May 2002 Nonlinear Kinetic Sunyaev Zel dovich Effect Physical Review Letters 88 21 211301 arXiv astro ph 0106342 Bibcode 2002PhRvL 88u1301M doi 10 1103 PhysRevLett 88 211301 PMID 12059470 S2CID 5655238 Myers A D Shanks T et al 2004 Evidence for an Extended SZ Effect in WMAP Data Monthly Notices of the Royal Astronomical Society 347 4 L67 L72 arXiv astro ph 0306180 Bibcode 2004MNRAS 347L 67M doi 10 1111 j 1365 2966 2004 07449 x S2CID 53119165 Springel Volker White Martin Hernquist Lars 2001 Hydrodynamic Simulations of the Sunyaev Zel dovich effect s The Astrophysical Journal 549 2 681 687 arXiv astro ph 0008133 Bibcode 2001ApJ 549 681S doi 10 1086 319473 S2CID 6728519 Sunyaev R A Ya B Zel dovich 1970 Small Scale Fluctuations of Relic Radiation Astrophysics and Space Science 7 1 3 19 Bibcode 1970Ap amp SS 7 3S doi 10 1007 BF00653471 S2CID 117050217 Sunyaev R A Ia B Zel dovich 1980 Microwave background radiation as a probe of the contemporary structure and history of the universe Annual Review of Astronomy and Astrophysics 18 1 537 560 Bibcode 1980ARA amp A 18 537S doi 10 1146 annurev aa 18 090180 002541 Diego J M Martinez E Sanz J L Benitez N Silk J 2002 The Sunyaev Zel dovich effect as a cosmological discriminator Monthly Notices of the Royal Astronomical Society 331 3 556 568 arXiv astro ph 0103512 Bibcode 2002MNRAS 331 556D doi 10 1046 j 1365 8711 2002 05039 x S2CID 10486016 Royal Astronomical Society Corrupted echoes from the Big Bang RAS Press Notice PN 04 01External links EditCorrupted echoes from the Big Bang innovations report com Sunyaev Zel dovich effect on arxiv org Portals Astronomy Stars Spaceflight Outer space Solar System Science Retrieved from https en wikipedia org w index php title Sunyaev Zeldovich effect amp oldid 1170139986, wikipedia, wiki, book, books, library,

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