Cosmology from MAXIMA-1, BOOMERANG, and COBE DMR cosmic microwave background observations

A. H. Jaffe; P. A.R. Ade; A. Balbi; J. J. Bock; J. R. Bond; J. Borrill; A. Boscaleri; K. Coble; B. P. Crill; P. De Bernardis; P. Farese; P. G. Ferreira; K. Ganga; M. Giacometti; S. Hanany; E. Hivon; V. V. Hristov; A. Iacoangeli; A. E. Lange; A. T. Lee; L. Martinis; S. Masi; P. D. Mauskopf; A. Melchiorri; T. Montroy; C. B. Netterfield; S. Oh; E. Pascale; F. Piacentini; D. Pogosyan; S. Prunet; B. Rabii; S. Rao; P. L. Richards; G. Romeo; J. E. Ruhl; F. Scaramuzzi; D. Sforna; G. F. Smoot; R. Stompor; C. D. Winant; J. H.P. Wu

doi:10.1103/PhysRevLett.86.3475

Cosmology from MAXIMA-1, BOOMERANG, and COBE DMR cosmic microwave background observations

A. H. Jaffe, P. A.R. Ade, A. Balbi, J. J. Bock, J. R. Bond, J. Borrill, A. Boscaleri, K. Coble, B. P. Crill, P. De Bernardis, P. Farese, P. G. Ferreira, K. Ganga, M. Giacometti, S. Hanany, E. Hivon, V. V. Hristov, A. Iacoangeli, A. E. Lange, A. T. LeeL. Martinis, S. Masi, P. D. Mauskopf, A. Melchiorri, T. Montroy, C. B. Netterfield, S. Oh, E. Pascale, F. Piacentini, D. Pogosyan, S. Prunet, B. Rabii, S. Rao, P. L. Richards, G. Romeo, J. E. Ruhl, F. Scaramuzzi, D. Sforna, G. F. Smoot, R. Stompor, C. D. Winant, J. H.P. Wu

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Abstract

To obtain further estimates of several cosmological parameters, the recent BOOMERANG-98 (B98) and MAXIMA-1 cosmic microwave background (CMB) anisotropy data, as well as COBE DMR, were analyzed. The resulting data support the chief predictions of the inflation paradigm, that the geometry of the Universe is flat, and that the initial density perturbations are scale invariant, and with the corollary that the density of mass energy in the Universe is dominated by a form other than ordinary matter.

Original language	English (US)
Pages (from-to)	3475-3479
Number of pages	5
Journal	Physical Review Letters
Volume	86
Issue number	16
DOIs	https://doi.org/10.1103/PhysRevLett.86.3475
State	Published - Apr 16 2001
Externally published	Yes

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Physics and Astronomy(all)

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10.1103/PhysRevLett.86.3475

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Jaffe, A. H., Ade, P. A. R., Balbi, A., Bock, J. J., Bond, J. R., Borrill, J., Boscaleri, A., Coble, K., Crill, B. P., De Bernardis, P., Farese, P., Ferreira, P. G., Ganga, K., Giacometti, M., Hanany, S., Hivon, E., Hristov, V. V., Iacoangeli, A., Lange, A. E., ... Wu, J. H. P. (2001). Cosmology from MAXIMA-1, BOOMERANG, and COBE DMR cosmic microwave background observations. Physical Review Letters, 86(16), 3475-3479. https://doi.org/10.1103/PhysRevLett.86.3475

Jaffe, AH, Ade, PAR, Balbi, A, Bock, JJ, Bond, JR, Borrill, J, Boscaleri, A, Coble, K, Crill, BP, De Bernardis, P, Farese, P, Ferreira, PG, Ganga, K, Giacometti, M, Hanany, S, Hivon, E, Hristov, VV, Iacoangeli, A, Lange, AE, Lee, AT, Martinis, L, Masi, S, Mauskopf, PD, Melchiorri, A, Montroy, T, Netterfield, CB, Oh, S, Pascale, E, Piacentini, F, Pogosyan, D, Prunet, S, Rabii, B, Rao, S, Richards, PL, Romeo, G, Ruhl, JE, Scaramuzzi, F, Sforna, D, Smoot, GF, Stompor, R, Winant, CD & Wu, JHP 2001, 'Cosmology from MAXIMA-1, BOOMERANG, and COBE DMR cosmic microwave background observations', Physical Review Letters, vol. 86, no. 16, pp. 3475-3479. https://doi.org/10.1103/PhysRevLett.86.3475

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title = "Cosmology from MAXIMA-1, BOOMERANG, and COBE DMR cosmic microwave background observations",

abstract = "To obtain further estimates of several cosmological parameters, the recent BOOMERANG-98 (B98) and MAXIMA-1 cosmic microwave background (CMB) anisotropy data, as well as COBE DMR, were analyzed. The resulting data support the chief predictions of the inflation paradigm, that the geometry of the Universe is flat, and that the initial density perturbations are scale invariant, and with the corollary that the density of mass energy in the Universe is dominated by a form other than ordinary matter.",

author = "Jaffe, {A. H.} and Ade, {P. A.R.} and A. Balbi and Bock, {J. J.} and Bond, {J. R.} and J. Borrill and A. Boscaleri and K. Coble and Crill, {B. P.} and {De Bernardis}, P. and P. Farese and Ferreira, {P. G.} and K. Ganga and M. Giacometti and S. Hanany and E. Hivon and Hristov, {V. V.} and A. Iacoangeli and Lange, {A. E.} and Lee, {A. T.} and L. Martinis and S. Masi and Mauskopf, {P. D.} and A. Melchiorri and T. Montroy and Netterfield, {C. B.} and S. Oh and E. Pascale and F. Piacentini and D. Pogosyan and S. Prunet and B. Rabii and S. Rao and Richards, {P. L.} and G. Romeo and Ruhl, {J. E.} and F. Scaramuzzi and D. Sforna and Smoot, {G. F.} and R. Stompor and Winant, {C. D.} and Wu, {J. H.P.}",

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doi = "10.1103/PhysRevLett.86.3475",

language = "English (US)",

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AU - Jaffe, A. H.

AU - Ade, P. A.R.

AU - Balbi, A.

AU - Bock, J. J.

AU - Bond, J. R.

AU - Borrill, J.

AU - Boscaleri, A.

AU - Coble, K.

AU - Crill, B. P.

AU - De Bernardis, P.

AU - Farese, P.

AU - Ferreira, P. G.

AU - Ganga, K.

AU - Giacometti, M.

AU - Hanany, S.

AU - Hivon, E.

AU - Hristov, V. V.

AU - Iacoangeli, A.

AU - Lange, A. E.

AU - Lee, A. T.

AU - Martinis, L.

AU - Masi, S.

AU - Mauskopf, P. D.

AU - Melchiorri, A.

AU - Montroy, T.

AU - Netterfield, C. B.

AU - Oh, S.

AU - Pascale, E.

AU - Piacentini, F.

AU - Pogosyan, D.

AU - Prunet, S.

AU - Rabii, B.

AU - Rao, S.

AU - Richards, P. L.

AU - Romeo, G.

AU - Ruhl, J. E.

AU - Scaramuzzi, F.

AU - Sforna, D.

AU - Smoot, G. F.

AU - Stompor, R.

AU - Winant, C. D.

AU - Wu, J. H.P.

PY - 2001/4/16

Y1 - 2001/4/16

N2 - To obtain further estimates of several cosmological parameters, the recent BOOMERANG-98 (B98) and MAXIMA-1 cosmic microwave background (CMB) anisotropy data, as well as COBE DMR, were analyzed. The resulting data support the chief predictions of the inflation paradigm, that the geometry of the Universe is flat, and that the initial density perturbations are scale invariant, and with the corollary that the density of mass energy in the Universe is dominated by a form other than ordinary matter.

AB - To obtain further estimates of several cosmological parameters, the recent BOOMERANG-98 (B98) and MAXIMA-1 cosmic microwave background (CMB) anisotropy data, as well as COBE DMR, were analyzed. The resulting data support the chief predictions of the inflation paradigm, that the geometry of the Universe is flat, and that the initial density perturbations are scale invariant, and with the corollary that the density of mass energy in the Universe is dominated by a form other than ordinary matter.

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Cosmology from MAXIMA-1, BOOMERANG, and COBE DMR cosmic microwave background observations

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