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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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Lenguaje: | eng |
Publicado: |
2014
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1051/0004-6361/201424496 http://cds.cern.ch/record/1712716 |
_version_ | 1780936774338478080 |
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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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planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT leonardir planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT lesgourguesj planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT liguorim planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT liljepb planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT lindenvornlem planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT lopezcaniegom planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT lubinpm planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT maciasperezjf planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT mandolesin planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT marism planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT martinpg planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT martinezgonzaleze planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT masis planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT matarreses planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT mazzottap planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT meinholdpr planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT melchiorria planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT mendesl planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT menegonie planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT mennellaa planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT migliacciom planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT mivilledeschenesma planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT monetia planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT montierl planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT morganteg planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT mossa planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT munshid planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT murphyja planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT naselskyp planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT natif planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT natolip planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT norgaardnielsenhu planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT noviellof planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT novikovd planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT novikovi planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT oxborrowca planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT paganol planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT pajotf planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT paolettid planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT pasianf planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT patanchong planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT perdereauo planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT perottol planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT perrottaf planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT piacentinif planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT piatm planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT pierpaolie planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT pietrobond planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT plaszczynskis planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT pointecouteaue planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT polentag planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT ponthieun planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT popal planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT prattgw planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT prunets planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT rachenjp planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT rebolor planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT reineckem planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT remazeillesm planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT renaultc planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT ricciardis planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT ristorcellii planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT rochag planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT roudierg planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT rusholmeb planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT sandrim planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT savinig planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT scottd planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT spencerld planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT stolyarovv planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT sudiwalar planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT suttond planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT suuruskias planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT sygnetjf planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT tauberja planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT tavagnaccod planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT terenzil planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT toffolattil planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT tomasim planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT tristramm planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT tuccim planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT uzanjp planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT valenzianol planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT valiviitaj planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT vantentb planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT vielvap planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT villaf planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT wadela planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT yvond planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT zaccheia planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants AT zoncaa planckintermediateresultsxxivconstraintsonvariationoffundamentalconstants |