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Planck intermediate results. XXIV. Constraints on variation of fundamental constants

Any variation of the fundamental physical constants, and more particularly of the fine structure constant, $\alpha$, or of the mass of the electron, $m_e$, would affect the recombination history of the Universe and cause an imprint on the cosmic microwave background angular power spectra. We show th...

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Detalles Bibliográficos
Autores principales: Ade, P.A.R., Aghanim, N., Arnaud, M., Ashdown, M., Aumont, J., Baccigalupi, C., Banday, A.J., Barreiro, R.B., Battaner, E., Benabed, K., Benoit-Levy, A., Bernard, J.P., Bersanelli, M., Bielewicz, P., Bond, J.R., Borrill, J., Bouchet, F.R., Burigana, C., Butler, R.C., Calabrese, E., Chamballu, A., Chiang, H.C., Christensen, P.R., Clements, D.L., Colombo, L.P.L., Couchot, F., Curto, A., Cuttaia, F., Danese, L., Davies, R.D., Davis, R.J., de Bernardis, P., de Rosa, A., de Zotti, G., Delabrouille, J., Diego, J.M., Dole, H., Dore, O., Dupac, X., Ensslin, T.A., Eriksen, H.K., Fabre, O., Finelli, F., Forni, O., Frailis, M., Franceschi, E., Galeotta, S., Galli, S., Ganga, K., Giard, M., Gonzalez-Nuevo, J., Gorski, K.M., Gregorio, A., Gruppuso, A., Hansen, F.K., Hanson, D., Harrison, D.L., 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., Jaffe, A.H., Jones, W.C., Keihanen, E., Keskitalo, R., Kneissl, R., Knoche, J., Kunz, M., Kurki-Suonio, H., Lamarre, J.M., Lasenby, A., Lawrence, C.R., Leonardi, R., Lesgourgues, J., Liguori, M., Lilje, P.B., Linden-Vornle, M., Lopez-Caniego, M., Lubin, P.M., Macias-Perez, J.F., Mandolesi, N., Maris, M., Martin, P.G., Martinez-Gonzalez, E., Masi, S., Matarrese, S., Mazzotta, P., Meinhold, P.R., Melchiorri, A., Mendes, L., Menegoni, E., Mennella, A., Migliaccio, M., Miville-Deschenes, M.A., Moneti, A., Montier, L., Morgante, G., Moss, A., Munshi, D., Murphy, J.A., Naselsky, P., Nati, F., Natoli, P., Norgaard-Nielsen, H.U., Noviello, F., Novikov, D., Novikov, I., Oxborrow, C.A., Pagano, L., Pajot, F., Paoletti, D., Pasian, F., Patanchon, G., Perdereau, O., Perotto, L., Perrotta, F., Piacentini, F., Piat, M., Pierpaoli, E., Pietrobon, D., Plaszczynski, S., Pointecouteau, E., Polenta, G., Ponthieu, N., Popa, L., Pratt, G.W., Prunet, S., Rachen, J.P., Rebolo, R., Reinecke, M., Remazeilles, M., Renault, C., Ricciardi, S., Ristorcelli, I., Rocha, G., Roudier, G., Rusholme, B., Sandri, M., Savini, G., Scott, D., Spencer, L.D., Stolyarov, V., Sudiwala, R., Sutton, D., Suur-Uski, A.S., Sygnet, J.F., Tauber, J.A., Tavagnacco, D., Terenzi, L., Toffolatti, L., Tomasi, M., Tristram, M., Tucci, M., Uzan, J.P., Valenziano, L., Valiviita, J., Van Tent, B., Vielva, P., Villa, F., Wade, L.A., Yvon, D., Zacchei, A., Zonca, A.
Lenguaje:eng
Publicado: 2014
Materias:
Acceso en línea:https://dx.doi.org/10.1051/0004-6361/201424496
http://cds.cern.ch/record/1712716
_version_ 1780936774338478080
author Ade, P.A.R.
Aghanim, N.
Arnaud, M.
Ashdown, M.
Aumont, J.
Baccigalupi, C.
Banday, A.J.
Barreiro, R.B.
Battaner, E.
Benabed, K.
Benoit-Levy, A.
Bernard, J.P.
Bersanelli, M.
Bielewicz, P.
Bond, J.R.
Borrill, J.
Bouchet, F.R.
Burigana, C.
Butler, R.C.
Calabrese, E.
Chamballu, A.
Chiang, H.C.
Christensen, P.R.
Clements, D.L.
Colombo, L.P.L.
Couchot, F.
Curto, A.
Cuttaia, F.
Danese, L.
Davies, R.D.
Davis, R.J.
de Bernardis, P.
de Rosa, A.
de Zotti, G.
Delabrouille, J.
Diego, J.M.
Dole, H.
Dore, O.
Dupac, X.
Ensslin, T.A.
Eriksen, H.K.
Fabre, O.
Finelli, F.
Forni, O.
Frailis, M.
Franceschi, E.
Galeotta, S.
Galli, S.
Ganga, K.
Giard, M.
Gonzalez-Nuevo, J.
Gorski, K.M.
Gregorio, A.
Gruppuso, A.
Hansen, F.K.
Hanson, D.
Harrison, D.L.
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.
Jaffe, A.H.
Jones, W.C.
Keihanen, E.
Keskitalo, R.
Kneissl, R.
Knoche, J.
Kunz, M.
Kurki-Suonio, H.
Lamarre, J.M.
Lasenby, A.
Lawrence, C.R.
Leonardi, R.
Lesgourgues, J.
Liguori, M.
Lilje, P.B.
Linden-Vornle, M.
Lopez-Caniego, M.
Lubin, P.M.
Macias-Perez, J.F.
Mandolesi, N.
Maris, M.
Martin, P.G.
Martinez-Gonzalez, E.
Masi, S.
Matarrese, S.
Mazzotta, P.
Meinhold, P.R.
Melchiorri, A.
Mendes, L.
Menegoni, E.
Mennella, A.
Migliaccio, M.
Miville-Deschenes, M.A.
Moneti, A.
Montier, L.
Morgante, G.
Moss, A.
Munshi, D.
Murphy, J.A.
Naselsky, P.
Nati, F.
Natoli, P.
Norgaard-Nielsen, H.U.
Noviello, F.
Novikov, D.
Novikov, I.
Oxborrow, C.A.
Pagano, L.
Pajot, F.
Paoletti, D.
Pasian, F.
Patanchon, G.
Perdereau, O.
Perotto, L.
Perrotta, F.
Piacentini, F.
Piat, M.
Pierpaoli, E.
Pietrobon, D.
Plaszczynski, S.
Pointecouteau, E.
Polenta, G.
Ponthieu, N.
Popa, L.
Pratt, G.W.
Prunet, S.
Rachen, J.P.
Rebolo, R.
Reinecke, M.
Remazeilles, M.
Renault, C.
Ricciardi, S.
Ristorcelli, I.
Rocha, G.
Roudier, G.
Rusholme, B.
Sandri, M.
Savini, G.
Scott, D.
Spencer, L.D.
Stolyarov, V.
Sudiwala, R.
Sutton, D.
Suur-Uski, A.S.
Sygnet, J.F.
Tauber, J.A.
Tavagnacco, D.
Terenzi, L.
Toffolatti, L.
Tomasi, M.
Tristram, M.
Tucci, M.
Uzan, J.P.
Valenziano, L.
Valiviita, J.
Van Tent, B.
Vielva, P.
Villa, F.
Wade, L.A.
Yvon, D.
Zacchei, A.
Zonca, A.
author_facet Ade, P.A.R.
Aghanim, N.
Arnaud, M.
Ashdown, M.
Aumont, J.
Baccigalupi, C.
Banday, A.J.
Barreiro, R.B.
Battaner, E.
Benabed, K.
Benoit-Levy, A.
Bernard, J.P.
Bersanelli, M.
Bielewicz, P.
Bond, J.R.
Borrill, J.
Bouchet, F.R.
Burigana, C.
Butler, R.C.
Calabrese, E.
Chamballu, A.
Chiang, H.C.
Christensen, P.R.
Clements, D.L.
Colombo, L.P.L.
Couchot, F.
Curto, A.
Cuttaia, F.
Danese, L.
Davies, R.D.
Davis, R.J.
de Bernardis, P.
de Rosa, A.
de Zotti, G.
Delabrouille, J.
Diego, J.M.
Dole, H.
Dore, O.
Dupac, X.
Ensslin, T.A.
Eriksen, H.K.
Fabre, O.
Finelli, F.
Forni, O.
Frailis, M.
Franceschi, E.
Galeotta, S.
Galli, S.
Ganga, K.
Giard, M.
Gonzalez-Nuevo, J.
Gorski, K.M.
Gregorio, A.
Gruppuso, A.
Hansen, F.K.
Hanson, D.
Harrison, D.L.
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.
Jaffe, A.H.
Jones, W.C.
Keihanen, E.
Keskitalo, R.
Kneissl, R.
Knoche, J.
Kunz, M.
Kurki-Suonio, H.
Lamarre, J.M.
Lasenby, A.
Lawrence, C.R.
Leonardi, R.
Lesgourgues, J.
Liguori, M.
Lilje, P.B.
Linden-Vornle, M.
Lopez-Caniego, M.
Lubin, P.M.
Macias-Perez, J.F.
Mandolesi, N.
Maris, M.
Martin, P.G.
Martinez-Gonzalez, E.
Masi, S.
Matarrese, S.
Mazzotta, P.
Meinhold, P.R.
Melchiorri, A.
Mendes, L.
Menegoni, E.
Mennella, A.
Migliaccio, M.
Miville-Deschenes, M.A.
Moneti, A.
Montier, L.
Morgante, G.
Moss, A.
Munshi, D.
Murphy, J.A.
Naselsky, P.
Nati, F.
Natoli, P.
Norgaard-Nielsen, H.U.
Noviello, F.
Novikov, D.
Novikov, I.
Oxborrow, C.A.
Pagano, L.
Pajot, F.
Paoletti, D.
Pasian, F.
Patanchon, G.
Perdereau, O.
Perotto, L.
Perrotta, F.
Piacentini, F.
Piat, M.
Pierpaoli, E.
Pietrobon, D.
Plaszczynski, S.
Pointecouteau, E.
Polenta, G.
Ponthieu, N.
Popa, L.
Pratt, G.W.
Prunet, S.
Rachen, J.P.
Rebolo, R.
Reinecke, M.
Remazeilles, M.
Renault, C.
Ricciardi, S.
Ristorcelli, I.
Rocha, G.
Roudier, G.
Rusholme, B.
Sandri, M.
Savini, G.
Scott, D.
Spencer, L.D.
Stolyarov, V.
Sudiwala, R.
Sutton, D.
Suur-Uski, A.S.
Sygnet, J.F.
Tauber, J.A.
Tavagnacco, D.
Terenzi, L.
Toffolatti, L.
Tomasi, M.
Tristram, M.
Tucci, M.
Uzan, J.P.
Valenziano, L.
Valiviita, J.
Van Tent, B.
Vielva, P.
Villa, F.
Wade, L.A.
Yvon, D.
Zacchei, A.
Zonca, A.
author_sort Ade, P.A.R.
collection CERN
description Any variation of the fundamental physical constants, and more particularly of the fine structure constant, $\alpha$, or of the mass of the electron, $m_e$, would affect the recombination history of the Universe and cause an imprint on the cosmic microwave background angular power spectra. We show that the Planck data allow one to improve the constraint on the time variation of the fine structure constant at redshift $z\sim 10^3$ by about a factor of 5 compared to WMAP data, as well as to break the degeneracy with the Hubble constant, $H_0$. In addition to $\alpha$, we can set a constraint on the variation of the mass of the electron, $m_{\rm e}$, and on the simultaneous variation of the two constants. We examine in detail the degeneracies between fundamental constants and the cosmological parameters, in order to compare the limits obtained from Planck and WMAP and to determine the constraining power gained by including other cosmological probes. We conclude that independent time variations of the fine structure constant and of the mass of the electron are constrained by Planck to ${\Delta\alpha}/{\alpha}= (3.6\pm 3.7)\times10^{-3}$ and ${\Delta m_{\rm e}}/{m_{\rm e}}= (4 \pm 11)\times10^{-3}$ at the 68% confidence level. We also investigate the possibility of a spatial variation of the fine structure constant. The relative amplitude of a dipolar spatial variation of $\alpha$ (corresponding to a gradient across our Hubble volume) is constrained to be $\delta\alpha/\alpha=(-2.4\pm 3.7)\times 10^{-2}$.
id cern-1712716
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2014
record_format invenio
spelling cern-17127162021-05-03T20:02:46Zdoi:10.1051/0004-6361/201424496http://cds.cern.ch/record/1712716engAde, P.A.R.Aghanim, N.Arnaud, M.Ashdown, M.Aumont, J.Baccigalupi, C.Banday, A.J.Barreiro, R.B.Battaner, E.Benabed, K.Benoit-Levy, A.Bernard, J.P.Bersanelli, M.Bielewicz, P.Bond, J.R.Borrill, J.Bouchet, F.R.Burigana, C.Butler, R.C.Calabrese, E.Chamballu, A.Chiang, H.C.Christensen, P.R.Clements, D.L.Colombo, L.P.L.Couchot, F.Curto, A.Cuttaia, F.Danese, L.Davies, R.D.Davis, R.J.de Bernardis, P.de Rosa, A.de Zotti, G.Delabrouille, J.Diego, J.M.Dole, H.Dore, O.Dupac, X.Ensslin, T.A.Eriksen, H.K.Fabre, O.Finelli, F.Forni, O.Frailis, M.Franceschi, E.Galeotta, S.Galli, S.Ganga, K.Giard, M.Gonzalez-Nuevo, J.Gorski, K.M.Gregorio, A.Gruppuso, A.Hansen, F.K.Hanson, D.Harrison, D.L.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.Jaffe, A.H.Jones, W.C.Keihanen, E.Keskitalo, R.Kneissl, R.Knoche, J.Kunz, M.Kurki-Suonio, H.Lamarre, J.M.Lasenby, A.Lawrence, C.R.Leonardi, R.Lesgourgues, J.Liguori, M.Lilje, P.B.Linden-Vornle, M.Lopez-Caniego, M.Lubin, P.M.Macias-Perez, J.F.Mandolesi, N.Maris, M.Martin, P.G.Martinez-Gonzalez, E.Masi, S.Matarrese, S.Mazzotta, P.Meinhold, P.R.Melchiorri, A.Mendes, L.Menegoni, E.Mennella, A.Migliaccio, M.Miville-Deschenes, M.A.Moneti, A.Montier, L.Morgante, G.Moss, A.Munshi, D.Murphy, J.A.Naselsky, P.Nati, F.Natoli, P.Norgaard-Nielsen, H.U.Noviello, F.Novikov, D.Novikov, I.Oxborrow, C.A.Pagano, L.Pajot, F.Paoletti, D.Pasian, F.Patanchon, G.Perdereau, O.Perotto, L.Perrotta, F.Piacentini, F.Piat, M.Pierpaoli, E.Pietrobon, D.Plaszczynski, S.Pointecouteau, E.Polenta, G.Ponthieu, N.Popa, L.Pratt, G.W.Prunet, S.Rachen, J.P.Rebolo, R.Reinecke, M.Remazeilles, M.Renault, C.Ricciardi, S.Ristorcelli, I.Rocha, G.Roudier, G.Rusholme, B.Sandri, M.Savini, G.Scott, D.Spencer, L.D.Stolyarov, V.Sudiwala, R.Sutton, D.Suur-Uski, A.S.Sygnet, J.F.Tauber, J.A.Tavagnacco, D.Terenzi, L.Toffolatti, L.Tomasi, M.Tristram, M.Tucci, M.Uzan, J.P.Valenziano, L.Valiviita, J.Van Tent, B.Vielva, P.Villa, F.Wade, L.A.Yvon, D.Zacchei, A.Zonca, A.Planck intermediate results. XXIV. Constraints on variation of fundamental constantsastro-ph.COAny variation of the fundamental physical constants, and more particularly of the fine structure constant, $\alpha$, or of the mass of the electron, $m_e$, would affect the recombination history of the Universe and cause an imprint on the cosmic microwave background angular power spectra. We show that the Planck data allow one to improve the constraint on the time variation of the fine structure constant at redshift $z\sim 10^3$ by about a factor of 5 compared to WMAP data, as well as to break the degeneracy with the Hubble constant, $H_0$. In addition to $\alpha$, we can set a constraint on the variation of the mass of the electron, $m_{\rm e}$, and on the simultaneous variation of the two constants. We examine in detail the degeneracies between fundamental constants and the cosmological parameters, in order to compare the limits obtained from Planck and WMAP and to determine the constraining power gained by including other cosmological probes. We conclude that independent time variations of the fine structure constant and of the mass of the electron are constrained by Planck to ${\Delta\alpha}/{\alpha}= (3.6\pm 3.7)\times10^{-3}$ and ${\Delta m_{\rm e}}/{m_{\rm e}}= (4 \pm 11)\times10^{-3}$ at the 68% confidence level. We also investigate the possibility of a spatial variation of the fine structure constant. The relative amplitude of a dipolar spatial variation of $\alpha$ (corresponding to a gradient across our Hubble volume) is constrained to be $\delta\alpha/\alpha=(-2.4\pm 3.7)\times 10^{-2}$.Any variation in the fundamental physical constants, more particularly in the fine structure constant, alpha, or in the mass of the electron, m_e, affects the recombination history of the Universe and cause an imprint on the cosmic microwave background angular power spectra. We show that the Planck data allow one to improve the constraint on the time variation of the fine structure constant at redshift z ~ 10^3 by about a factor of 5 compared to WMAP data, as well as to break the degeneracy with the Hubble constant, H_0. In addition to alpha, we can set a constraint on the variation in the mass of the electron, m_e, and in the simultaneous variation of the two constants. We examine in detail the degeneracies between fundamental constants and the cosmological parameters, in order to compare the limits obtained from Planck and WMAP and to determine the constraining power gained by including other cosmological probes. We conclude that independent time variations of the fine structure constant and of the mass of the electron are constrained by Planck to Deltaalpha/alpha = (3.6 +- 3.7) x 10^-3 and Deltam_e/m_e = (4 +- 11) x 10^-3 at the 68% confidence level. We also investigate the possibility of a spatial variation of the fine structure constant. The relative amplitude of a dipolar spatial variation in alpha (corresponding to a gradient across our Hubble volume) is constrained to be deltaalpha/alpha = (-2.4 +- 3.7) x 10^-2.Any variation of the fundamental physical constants, and more particularly of the fine structure constant, $\alpha$, or of the mass of the electron, $m_e$, would affect the recombination history of the Universe and cause an imprint on the cosmic microwave background angular power spectra. We show that the Planck data allow one to improve the constraint on the time variation of the fine structure constant at redshift $z\sim 10^3$ by about a factor of 5 compared to WMAP data, as well as to break the degeneracy with the Hubble constant, $H_0$. In addition to $\alpha$, we can set a constraint on the variation of the mass of the electron, $m_{\rm e}$, and on the simultaneous variation of the two constants. We examine in detail the degeneracies between fundamental constants and the cosmological parameters, in order to compare the limits obtained from Planck and WMAP and to determine the constraining power gained by including other cosmological probes. We conclude that independent time variations of the fine structure constant and of the mass of the electron are constrained by Planck to ${\Delta\alpha}/{\alpha}= (3.6\pm 3.7)\times10^{-3}$ and ${\Delta m_{\rm e}}/{m_{\rm e}}= (4 \pm 11)\times10^{-3}$ at the 68% confidence level. We also investigate the possibility of a spatial variation of the fine structure constant. The relative amplitude of a dipolar spatial variation of $\alpha$ (corresponding to a gradient across our Hubble volume) is constrained to be $\delta\alpha/\alpha=(-2.4\pm 3.7)\times 10^{-2}$.arXiv:1406.7482oai:cds.cern.ch:17127162014-06-29
spellingShingle astro-ph.CO
Ade, P.A.R.
Aghanim, N.
Arnaud, M.
Ashdown, M.
Aumont, J.
Baccigalupi, C.
Banday, A.J.
Barreiro, R.B.
Battaner, E.
Benabed, K.
Benoit-Levy, A.
Bernard, J.P.
Bersanelli, M.
Bielewicz, P.
Bond, J.R.
Borrill, J.
Bouchet, F.R.
Burigana, C.
Butler, R.C.
Calabrese, E.
Chamballu, A.
Chiang, H.C.
Christensen, P.R.
Clements, D.L.
Colombo, L.P.L.
Couchot, F.
Curto, A.
Cuttaia, F.
Danese, L.
Davies, R.D.
Davis, R.J.
de Bernardis, P.
de Rosa, A.
de Zotti, G.
Delabrouille, J.
Diego, J.M.
Dole, H.
Dore, O.
Dupac, X.
Ensslin, T.A.
Eriksen, H.K.
Fabre, O.
Finelli, F.
Forni, O.
Frailis, M.
Franceschi, E.
Galeotta, S.
Galli, S.
Ganga, K.
Giard, M.
Gonzalez-Nuevo, J.
Gorski, K.M.
Gregorio, A.
Gruppuso, A.
Hansen, F.K.
Hanson, D.
Harrison, D.L.
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.
Jaffe, A.H.
Jones, W.C.
Keihanen, E.
Keskitalo, R.
Kneissl, R.
Knoche, J.
Kunz, M.
Kurki-Suonio, H.
Lamarre, J.M.
Lasenby, A.
Lawrence, C.R.
Leonardi, R.
Lesgourgues, J.
Liguori, M.
Lilje, P.B.
Linden-Vornle, M.
Lopez-Caniego, M.
Lubin, P.M.
Macias-Perez, J.F.
Mandolesi, N.
Maris, M.
Martin, P.G.
Martinez-Gonzalez, E.
Masi, S.
Matarrese, S.
Mazzotta, P.
Meinhold, P.R.
Melchiorri, A.
Mendes, L.
Menegoni, E.
Mennella, A.
Migliaccio, M.
Miville-Deschenes, M.A.
Moneti, A.
Montier, L.
Morgante, G.
Moss, A.
Munshi, D.
Murphy, J.A.
Naselsky, P.
Nati, F.
Natoli, P.
Norgaard-Nielsen, H.U.
Noviello, F.
Novikov, D.
Novikov, I.
Oxborrow, C.A.
Pagano, L.
Pajot, F.
Paoletti, D.
Pasian, F.
Patanchon, G.
Perdereau, O.
Perotto, L.
Perrotta, F.
Piacentini, F.
Piat, M.
Pierpaoli, E.
Pietrobon, D.
Plaszczynski, S.
Pointecouteau, E.
Polenta, G.
Ponthieu, N.
Popa, L.
Pratt, G.W.
Prunet, S.
Rachen, J.P.
Rebolo, R.
Reinecke, M.
Remazeilles, M.
Renault, C.
Ricciardi, S.
Ristorcelli, I.
Rocha, G.
Roudier, G.
Rusholme, B.
Sandri, M.
Savini, G.
Scott, D.
Spencer, L.D.
Stolyarov, V.
Sudiwala, R.
Sutton, D.
Suur-Uski, A.S.
Sygnet, J.F.
Tauber, J.A.
Tavagnacco, D.
Terenzi, L.
Toffolatti, L.
Tomasi, M.
Tristram, M.
Tucci, M.
Uzan, J.P.
Valenziano, L.
Valiviita, J.
Van Tent, B.
Vielva, P.
Villa, F.
Wade, L.A.
Yvon, D.
Zacchei, A.
Zonca, A.
Planck intermediate results. XXIV. Constraints on variation of fundamental constants
title Planck intermediate results. XXIV. Constraints on variation of fundamental constants
title_full Planck intermediate results. XXIV. Constraints on variation of fundamental constants
title_fullStr Planck intermediate results. XXIV. Constraints on variation of fundamental constants
title_full_unstemmed Planck intermediate results. XXIV. Constraints on variation of fundamental constants
title_short Planck intermediate results. XXIV. Constraints on variation of fundamental constants
title_sort planck intermediate results. xxiv. constraints on variation of fundamental constants
topic astro-ph.CO
url https://dx.doi.org/10.1051/0004-6361/201424496
http://cds.cern.ch/record/1712716
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