2016A&A...594A..19P


Query : 2016A&A...594A..19P

2016A&A...594A..19P - Astronomy and Astrophysics, volume 594A19-19 (2016/10-1)

Planck 2015 results. XIX. Constraints on primordial magnetic fields.

PLANCK COLLABORATION, ADE P.A.R., AGHANIM N., ARNAUD M., ARROJA F., ASHDOWN M., AUMONT J., BACCIGALUPI C., BALLARDINI M., BANDAY A.J., BARREIRO R.B., BARTOLO N., BATTANER E., BENABED K., BENOIT A., BENOIT-LEVY A., BERNARD J.-P., BERSANELLI M., BIELEWICZ P., BOCK J.J., BONALDI A., BONAVERA L., BOND J.R., BORRILL J., BOUCHET F.R., BUCHER M., BURIGANA C., BUTLER R.C., CALABRESE E., CARDOSO J.-F., CATALANO A., CHAMBALLU A., CHIANG H.C., CHLUBA J., CHRISTENSEN P.R., CHURCH S., CLEMENTS D.L., COLOMBI S., COLOMBO L.P.L., COMBET C., COUCHOT F., COULAIS A., CRILL B.P., CURTO A., CUTTAIA F., DANESE L., DAVIES R.D., DAVIS R.J., DE BERNARDIS P., DE ROSA A., DE ZOTTI G., DELABROUILLE J., DESERT F.-X., DIEGO J.M., DOLAG K., DOLE H., DONZELLI S., DORE O., DOUSPIS M., DUCOUT A., DUPAC X., EFSTATHIOU G., ELSNER F., ENSSLIN T.A., ERIKSEN H.K., FERGUSSON J., FINELLI F., FLORIDO E., FORNI O., FRAILIS M., FRAISSE A.A., FRANCESCHI E., FREJSEL A., GALEOTTA S., GALLI S., GANGA K., GIARD M., GIRAUD-HERAUD Y., GJERLOW E., GONZALEZ-NUEVO J., GORSKI K.M., GRATTON S., GREGORIO A., GRUPPUSO A., GUDMUNDSSON J.E., HANSEN F.K., HANSON D., HARRISON D.L., HELOU G., HENROT-VERSILLE S., HERNANDEZ-MONTEAGUDO C., HERRANZ D., HILDEBRANDT S.R., HIVON E., HOBSON M., HOLMES W.A., HORNSTRUP A., HOVEST W., HUFFENBERGER K.M., HURIER G., JAFFE A.H., JAFFE T.R., JONES W.C., JUVELA M., KEIHANEN E., KESKITALO R., KIM J., KISNER T.S., KNOCHE J., KUNZ M., KURKI-SUONIO H., LAGACHE G., LAHTEENMAKI A., LAMARRE J.-M., LASENBY A., LATTANZI M., LAWRENCE C.R., LEAHY J.P., LEONARDI R., LESGOURGUES J., LEVRIER F., LIGUORI M., LILJE P.B., LINDEN-VORNLE M., LOPEZ-CANIEGO M., LUBIN P.M., MACIAS-PEREZ J.F., MAGGIO G., MAINO D., MANDOLESI N., MANGILLI A., MARIS M., MARTIN P.G., MARTINEZ-GONZALEZ E., MASI S., MATARRESE S., McGEHEE P., MEINHOLD P.R., MELCHIORRI A., MENDES L., MENNELLA A., MIGLIACCIO M., MITRA S., MIVILLE-DESCHENES M.-A., MOLINARI D., MONETI A., MONTIER L., MORGANTE G., MORTLOCK D., MOSS A., MUNSHI D., MURPHY J.A., NASELSKY P., NATI F., NATOLI P., NETTERFIELD C.B., NORGAARD-NIELSEN H.U., NOVIELLO F., NOVIKOV D., NOVIKOV I., OPPERMANN N., OXBORROW C.A., PACI F., PAGANO L., PAJOT F., PAOLETTI D., PASIAN F., PATANCHON G., PERDEREAU O., PEROTTO L., PERROTTA F., PETTORINO V., PIACENTINI F., PIAT M., PIERPAOLI E., PIETROBON D., PLASZCZYNSKI S., POINTECOUTEAU E., POLENTA G., POPA L., PRATT G.W., PREZEAU G., PRUNET S., PUGET J.-L., RACHEN J.P., REBOLO R., REINECKE M., REMAZEILLES M., RENAULT C., RENZI A., RISTORCELLI I., ROCHA G., ROSSET C., ROSSETTI M., ROUDIER G., RUBINO-MARTIN J.A., RUIZ-GRANADOS B., RUSHOLME B., SANDRI M., SANTOS D., SAVELAINEN M., SAVINI G., SCOTT D., SEIFFERT M.D., SHELLARD E.P.S., SHIRAISHI M., SPENCER L.D., STOLYAROV V., STOMPOR R., SUDIWALA R., SUNYAEV R., SUTTON D., SUUR-USKI A.-S., SYGNET J.-F., TAUBER J.A., TERENZI L., TOFFOLATTI L., TOMASI M., TRISTRAM M., TUCCI M., TUOVINEN J., UMANA G., VALENZIANO L., VALIVIITA J., VAN TENT B., VIELVA P., VILLA F., WADE L.A., WANDELT B.D., WEHUS I.K., YVON D., ZACCHEI A. and ZONCA A.

Abstract (from CDS):

We compute and investigate four types of imprint of a stochastic background of primordial magnetic fields (PMFs) on the cosmic microwave background (CMB) anisotropies: the impact of PMFs on the CMB temperature and polarization spectra, which is related to their contribution to cosmological perturbations; the effect on CMB polarization induced by Faraday rotation; the impact of PMFs on the ionization history; magnetically-induced non-Gaussianities and related non-zero bispectra; and the magnetically-induced breaking of statistical isotropy. We present constraints on the amplitude of PMFs that are derived from different Planck data products, depending on the specific effect that is being analysed. Overall, Planck data constrain the amplitude of PMFs to less than a few nanoGauss, with different bounds that depend on the considered model. In particular, individual limits coming from the analysis of the CMB angular power spectra, using the Planck likelihood, are B1Mpc<4.4nG (where B1Mpc is the comoving field amplitude at a scale of 1Mpc) at 95% confidence level, assuming zero helicity. By considering the Planck likelihood, based only on parity-even angular power spectra, we obtain B1Mpc<5.6nG for a maximally helical field. For nearly scale-invariant PMFs we obtain B1Mpc<2.0nG and B1Mpc<0.9nG if the impact of PMFs on the ionization history of the Universe is included in the analysis. From the analysis of magnetically-induced non-Gaussianity, we obtain three different values, corresponding to three applied methods, all below 5 nG. The constraint from the magnetically-induced passive-tensor bispectrum is B1Mpc<2.8nG. A search for preferred directions in the magnetically-induced passive bispectrum yields B1Mpc<4.5nG, whereas the compensated-scalar bispectrum gives B1Mpc<3nG. The analysis of the Faraday rotation of CMB polarization by PMFs uses the Planck power spectra in EE and BB at 70GHz and gives B1Mpc<1380nG. In our final analysis, we consider the harmonic-space correlations produced by Alfven waves, finding no significant evidence for the presence of these waves. Together, these results comprise a comprehensive set of constraints on possible PMFs with Planck data.

Abstract Copyright: © ESO, 2016

Journal keyword(s): magnetic fields - cosmic background radiation - early Universe

Simbad objects: 1

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Number of rows : 1
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 NAME Hydra I Cluster ClG 10 36 36.0 -27 31 04           ~ 905 1

Query : 2016A&A...594A..19P

Basic data :
NAME Hydra I Cluster -- Cluster of Galaxies
Other object types:
otypes_help
ClG (2004A&A,ACO,...), X (2A,3A,...), GrG ([FWB89]), gLe (2011A&A), C?G (XCLASS), gam (INTREF)
ICRS coord. (ep=J2000) :
10 36 36.0 -27 31 04 [ ] E 2007MNRAS.379..260M
FK4 coord. (ep=B1950 eq=1950) :
10 34 14.7 -27 15 29 [ ]
Gal coord. (ep=J2000) :
269.5723 +26.4819 [ ]
Radial velocity / Redshift / cz :
V(km/s) 3842 [1499] / z(spectroscopic) 0.0129 [0.0050] / cz 3867 [1499]
   (Opt) D 2022A&A...658A..59X
Angular size (arcmin):
20.416666031 20.416666031 0 (Xray) E 2021A&A...652A..12K
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Hierarchy : number of linked objects
whatever the membership probability is (see description here ) :

: 1
: 277
: 10 Display criteria :

Identifiers (28) :
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ACO 1060 FR 54 NAME Hya Cluster RX J1036.8-2730
2A 1033-270 1H 1033-273 NAME Hya I Cluster 3U 1044-30
3A 1035-272 H 1034-273 NAME Hydra Cluster 4U 1033-26
BAX 159.2137-27.5265 HMS 1034-2716 NAME Hydra I Cluster XCLASS 1940
ClG 1034.5-2716 INTREF 423 PLCKESZ G269.51+26.42 XSS J10376-2732
1E 1034.3-2716 2MAXI J1036-275 RXC J1036.6-2731 [F81] 183
1ES 1034-27.2 MCXC J1036.6-2731 RXGCC 366 [FWB89] GrG 47

References (905 between 1850 and 2026) (Total 905)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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Collections of Measurements Description of Measurements

Velocities : 8    Distance : 1   

   

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XMM : 1   

   


External archives :

Archive data at HEASARC - High-Energy Astrophysics Science Archive Research Center

Data at NED - NASA/IPAC Extragalactic Database : NAME Hydra I Cluster

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ACO 1060 RXC J1036.6-2731

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