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Hauptverfasser: Paoletti, D., Rubino-Martin, J., Shiraishi, M., Molinari, D., Chluba, J., Finelli, F., Baccigalupi, C., Errard, J., Gruppuso, A., Lonappan, A. I., Tartari, A., Allys, E., Anand, A., Aumont, J., Ballardini, M., Banday, A. J., Barreiro, R. B., Bartolo, N., Bersanelli, M., Bortolami, M., Brinckmann, T., Calabrese, E., Campeti, P., Carones, A., Casas, F. J., Cheung, K., Clermont, L., Columbro, F., Conenna, G., Coppolecchia, A., Cuttaia, F., D'Alessandro, G., de Bernardis, P., Della Torre, S., Diego-Palazuelos, P., Eriksen, H. K., Fuskeland, U., Galloni, G., Galloway, M., Gerbino, M., Gervasi, M., Ghigna, T., Giardiello, S., Gimeno-Amo, C., Gjerløw, E., Grupp, F., Hazumi, M., Henrot-Versillé, S., Hergt, L. T., Hivon, E., Ichiki, K., Ishino, H., Kohri, K., Komatsu, E., Krachmalnicoff, N., Lamagna, L., Lattanzi, M., Lembo, M., Levrier, F., López-Caniego, M., Luzzi, G., Martínez-González, E., Masi, S., Matarrese, S., Micheli, S., Migliaccio, M., Monelli, M., Montier, L., Morgante, G., Mousset, L., Nagata, R., Namikawa, T., Natoli, P., Novelli, A., Obata, I., Occhiuzzi, A., Odagiri, K., Pagano, L., Paiella, A., Pascual-Cisneros, G., Piacentini, F., Piccirilli, G., Remazeilles, M., Ritacco, A., Ruiz-Granda, M., Sakurai, Y., Scott, D., Stever, S. L., Sullivan, R. M., Takase, Y., Tassis, K., Terenzi, L., Tristram, M., Vacher, L., van Tent, B., Vielva, P., Wehus, I. K., Weymann-Despres, G., Zannoni, M., Zhou, Y.
Format: Preprint
Veröffentlicht: 2024
Schlagworte:
Cosmology and Nongalactic Astrophysics
Online-Zugang:https://arxiv.org/abs/2403.16763
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author Paoletti, D.
Rubino-Martin, J.
Shiraishi, M.
Molinari, D.
Chluba, J.
Finelli, F.
Baccigalupi, C.
Errard, J.
Gruppuso, A.
Lonappan, A. I.
Tartari, A.
Allys, E.
Anand, A.
Aumont, J.
Ballardini, M.
Banday, A. J.
Barreiro, R. B.
Bartolo, N.
Bersanelli, M.
Bortolami, M.
Brinckmann, T.
Calabrese, E.
Campeti, P.
Carones, A.
Casas, F. J.
Cheung, K.
Clermont, L.
Columbro, F.
Conenna, G.
Coppolecchia, A.
Cuttaia, F.
D'Alessandro, G.
de Bernardis, P.
Della Torre, S.
Diego-Palazuelos, P.
Eriksen, H. K.
Fuskeland, U.
Galloni, G.
Galloway, M.
Gerbino, M.
Gervasi, M.
Ghigna, T.
Giardiello, S.
Gimeno-Amo, C.
Gjerløw, E.
Grupp, F.
Hazumi, M.
Henrot-Versillé, S.
Hergt, L. T.
Hivon, E.
Ichiki, K.
Ishino, H.
Kohri, K.
Komatsu, E.
Krachmalnicoff, N.
Lamagna, L.
Lattanzi, M.
Lembo, M.
Levrier, F.
López-Caniego, M.
Luzzi, G.
Martínez-González, E.
Masi, S.
Matarrese, S.
Micheli, S.
Migliaccio, M.
Monelli, M.
Montier, L.
Morgante, G.
Mousset, L.
Nagata, R.
Namikawa, T.
Natoli, P.
Novelli, A.
Obata, I.
Occhiuzzi, A.
Odagiri, K.
Pagano, L.
Paiella, A.
Pascual-Cisneros, G.
Piacentini, F.
Piccirilli, G.
Remazeilles, M.
Ritacco, A.
Ruiz-Granda, M.
Sakurai, Y.
Scott, D.
Stever, S. L.
Sullivan, R. M.
Takase, Y.
Tassis, K.
Terenzi, L.
Tristram, M.
Vacher, L.
van Tent, B.
Vielva, P.
Wehus, I. K.
Weymann-Despres, G.
Zannoni, M.
Zhou, Y.
author_facet Paoletti, D.
Rubino-Martin, J.
Shiraishi, M.
Molinari, D.
Chluba, J.
Finelli, F.
Baccigalupi, C.
Errard, J.
Gruppuso, A.
Lonappan, A. I.
Tartari, A.
Allys, E.
Anand, A.
Aumont, J.
Ballardini, M.
Banday, A. J.
Barreiro, R. B.
Bartolo, N.
Bersanelli, M.
Bortolami, M.
Brinckmann, T.
Calabrese, E.
Campeti, P.
Carones, A.
Casas, F. J.
Cheung, K.
Clermont, L.
Columbro, F.
Conenna, G.
Coppolecchia, A.
Cuttaia, F.
D'Alessandro, G.
de Bernardis, P.
Della Torre, S.
Diego-Palazuelos, P.
Eriksen, H. K.
Fuskeland, U.
Galloni, G.
Galloway, M.
Gerbino, M.
Gervasi, M.
Ghigna, T.
Giardiello, S.
Gimeno-Amo, C.
Gjerløw, E.
Grupp, F.
Hazumi, M.
Henrot-Versillé, S.
Hergt, L. T.
Hivon, E.
Ichiki, K.
Ishino, H.
Kohri, K.
Komatsu, E.
Krachmalnicoff, N.
Lamagna, L.
Lattanzi, M.
Lembo, M.
Levrier, F.
López-Caniego, M.
Luzzi, G.
Martínez-González, E.
Masi, S.
Matarrese, S.
Micheli, S.
Migliaccio, M.
Monelli, M.
Montier, L.
Morgante, G.
Mousset, L.
Nagata, R.
Namikawa, T.
Natoli, P.
Novelli, A.
Obata, I.
Occhiuzzi, A.
Odagiri, K.
Pagano, L.
Paiella, A.
Pascual-Cisneros, G.
Piacentini, F.
Piccirilli, G.
Remazeilles, M.
Ritacco, A.
Ruiz-Granda, M.
Sakurai, Y.
Scott, D.
Stever, S. L.
Sullivan, R. M.
Takase, Y.
Tassis, K.
Terenzi, L.
Tristram, M.
Vacher, L.
van Tent, B.
Vielva, P.
Wehus, I. K.
Weymann-Despres, G.
Zannoni, M.
Zhou, Y.
contents We present detailed forecasts for the constraints on primordial magnetic fields (PMFs) that will be obtained with the LiteBIRD satellite. The constraints are driven by the effects of PMFs on the CMB anisotropies: the gravitational effects of magnetically-induced perturbations; the effects on the thermal and ionization history of the Universe; the Faraday rotation imprint on the CMB polarization; and the non-Gaussianities induced in polarization anisotropies. LiteBIRD represents a sensitive probe for PMFs and by exploiting all the physical effects, it will be able to improve the current limit coming from Planck. In particular, thanks to its accurate $B$-mode polarization measurement, LiteBIRD will improve the constraints on infrared configurations for the gravitational effect, giving $B_{\rm 1\,Mpc}^{n_{\rm B} =-2.9} < 0.8$ nG at 95% C.L., potentially opening the possibility to detect nanogauss fields with high significance. We also observe a significant improvement in the limits when marginalized over the spectral index, $B_{1\,{\rm Mpc}}^{\rm marg}< 2.2$ nG at 95% C.L. From the thermal history effect, which relies mainly on $E$-mode polarization data, we obtain a significant improvement for all PMF configurations, with the marginalized case, $\sqrt{\langle B^2\rangle}^{\rm marg}<0.50$ nG at 95% C.L. Faraday rotation constraints will take advantage of the wide frequency coverage of LiteBIRD and the high sensitivity in $B$ modes, improving the limits by orders of magnitude with respect to current results, $B_{1\,{\rm Mpc}}^{n_{\rm B} =-2.9} < 3.2$ nG at 95% C.L. Finally, non-Gaussianities of the $B$-mode polarization can probe PMFs at the level of 1 nG, again significantly improving the current bounds from Planck. Altogether our forecasts represent a broad collection of complementary probes, providing conservative limits on PMF characteristics that will be achieved with LiteBIRD.
format Preprint
id arxiv_https___arxiv_org_abs_2403_16763
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle LiteBIRD Science Goals and Forecasts: Primordial Magnetic Fields
Paoletti, D.
Rubino-Martin, J.
Shiraishi, M.
Molinari, D.
Chluba, J.
Finelli, F.
Baccigalupi, C.
Errard, J.
Gruppuso, A.
Lonappan, A. I.
Tartari, A.
Allys, E.
Anand, A.
Aumont, J.
Ballardini, M.
Banday, A. J.
Barreiro, R. B.
Bartolo, N.
Bersanelli, M.
Bortolami, M.
Brinckmann, T.
Calabrese, E.
Campeti, P.
Carones, A.
Casas, F. J.
Cheung, K.
Clermont, L.
Columbro, F.
Conenna, G.
Coppolecchia, A.
Cuttaia, F.
D'Alessandro, G.
de Bernardis, P.
Della Torre, S.
Diego-Palazuelos, P.
Eriksen, H. K.
Fuskeland, U.
Galloni, G.
Galloway, M.
Gerbino, M.
Gervasi, M.
Ghigna, T.
Giardiello, S.
Gimeno-Amo, C.
Gjerløw, E.
Grupp, F.
Hazumi, M.
Henrot-Versillé, S.
Hergt, L. T.
Hivon, E.
Ichiki, K.
Ishino, H.
Kohri, K.
Komatsu, E.
Krachmalnicoff, N.
Lamagna, L.
Lattanzi, M.
Lembo, M.
Levrier, F.
López-Caniego, M.
Luzzi, G.
Martínez-González, E.
Masi, S.
Matarrese, S.
Micheli, S.
Migliaccio, M.
Monelli, M.
Montier, L.
Morgante, G.
Mousset, L.
Nagata, R.
Namikawa, T.
Natoli, P.
Novelli, A.
Obata, I.
Occhiuzzi, A.
Odagiri, K.
Pagano, L.
Paiella, A.
Pascual-Cisneros, G.
Piacentini, F.
Piccirilli, G.
Remazeilles, M.
Ritacco, A.
Ruiz-Granda, M.
Sakurai, Y.
Scott, D.
Stever, S. L.
Sullivan, R. M.
Takase, Y.
Tassis, K.
Terenzi, L.
Tristram, M.
Vacher, L.
van Tent, B.
Vielva, P.
Wehus, I. K.
Weymann-Despres, G.
Zannoni, M.
Zhou, Y.
Cosmology and Nongalactic Astrophysics
We present detailed forecasts for the constraints on primordial magnetic fields (PMFs) that will be obtained with the LiteBIRD satellite. The constraints are driven by the effects of PMFs on the CMB anisotropies: the gravitational effects of magnetically-induced perturbations; the effects on the thermal and ionization history of the Universe; the Faraday rotation imprint on the CMB polarization; and the non-Gaussianities induced in polarization anisotropies. LiteBIRD represents a sensitive probe for PMFs and by exploiting all the physical effects, it will be able to improve the current limit coming from Planck. In particular, thanks to its accurate $B$-mode polarization measurement, LiteBIRD will improve the constraints on infrared configurations for the gravitational effect, giving $B_{\rm 1\,Mpc}^{n_{\rm B} =-2.9} < 0.8$ nG at 95% C.L., potentially opening the possibility to detect nanogauss fields with high significance. We also observe a significant improvement in the limits when marginalized over the spectral index, $B_{1\,{\rm Mpc}}^{\rm marg}< 2.2$ nG at 95% C.L. From the thermal history effect, which relies mainly on $E$-mode polarization data, we obtain a significant improvement for all PMF configurations, with the marginalized case, $\sqrt{\langle B^2\rangle}^{\rm marg}<0.50$ nG at 95% C.L. Faraday rotation constraints will take advantage of the wide frequency coverage of LiteBIRD and the high sensitivity in $B$ modes, improving the limits by orders of magnitude with respect to current results, $B_{1\,{\rm Mpc}}^{n_{\rm B} =-2.9} < 3.2$ nG at 95% C.L. Finally, non-Gaussianities of the $B$-mode polarization can probe PMFs at the level of 1 nG, again significantly improving the current bounds from Planck. Altogether our forecasts represent a broad collection of complementary probes, providing conservative limits on PMF characteristics that will be achieved with LiteBIRD.
title LiteBIRD Science Goals and Forecasts: Primordial Magnetic Fields
topic Cosmology and Nongalactic Astrophysics
url https://arxiv.org/abs/2403.16763

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