Cosmological implications of baryon acoustic oscillation measurements

Éric Aubourg, Stephen Bailey, Julian E. Bautista, Florian Beutler, Vaishali Bhardwaj, Dmitry Bizyaev, Michael Blanton, Michael Blomqvist, Adam S. Bolton, Jo Bovy, Howard Brewington, J. Brinkmann, Joel R. Brownstein, Angela Burden, Nicolás G. Busca, William Carithers, Chia Hsun Chuang, Johan Comparat, Rupert A C Croft, Antonio J. Cuesta & 75 others Kyle S. Dawson, Timothée Delubac, Daniel J. Eisenstein, Andreu Font-Ribera, Jian Ge, J. M. Le Goff, Satya Gontcho A Gontcho, J. Richard Gott, James E. Gunn, Hong Guo, Julien Guy, Jean Christophe Hamilton, Shirley Ho, Klaus Honscheid, Cullan Howlett, David Kirkby, Francisco S. Kitaura, Jean Paul Kneib, Khee Gan Lee, Dan Long, Robert H. Lupton, Mariana Vargas Magaña, Viktor Malanushenko, Elena Malanushenko, Marc Manera, Claudia Maraston, Daniel Margala, Cameron K. McBride, Jordi Miralda-Escudé, Adam D. Myers, Robert C. Nichol, Pasquier Noterdaeme, Sebastián E. Nuza, Matthew D. Olmstead, Daniel Oravetz, Isabelle Pâris, Nikhil Padmanabhan, Nathalie Palanque-Delabrouille, Kaike Pan, Marcos Pellejero-Ibanez, Will J. Percival, Patrick Petitjean, Matthew M. Pieri, Francisco Prada, Beth Reid, James Rich, Natalie A. Roe, Ashley J. Ross, Nicholas P. Ross, Graziano Rossi, Jose Alberto Rubiño-Martín, Ariel G. Sánchez, Lado Samushia, Ricardo Tanausú Génova Santos, Claudia G. Scóccola, David J. Schlegel, Donald P. Schneider, Hee Jong Seo, Erin Sheldon, Audrey Simmons, Ramin A. Skibba, Anže Slosar, Michael A. Strauss, Daniel Thomas, Jeremy L. Tinker, Rita Tojeiro, Jose Alberto Vazquez, Matteo Viel, David A. Wake, Benjamin A. Weaver, David H. Weinberg, W. M. Wood-Vasey, Christophe Yèche, Idit Zehavi, Gong Bo Zhao

    Research output: Contribution to journalArticle

    Abstract

    We derive constraints on cosmological parameters and tests of dark energy models from the combination of baryon acoustic oscillation (BAO) measurements with cosmic microwave background (CMB) data and a recent reanalysis of Type Ia supernova (SN) data. In particular, we take advantage of high-precision BAO measurements from galaxy clustering and the Lyman-α forest (LyaF) in the SDSS-III Baryon Oscillation Spectroscopic Survey (BOSS). Treating the BAO scale as an uncalibrated standard ruler, BAO data alone yield a high confidence detection of dark energy; in combination with the CMB angular acoustic scale they further imply a nearly flat universe. Adding the CMB-calibrated physical scale of the sound horizon, the combination of BAO and SN data into an "inverse distance ladder" yields a measurement of H0=67.3±1.1 km s-1 Mpc-1, with 1.7% precision. This measurement assumes standard prerecombination physics but is insensitive to assumptions about dark energy or space curvature, so agreement with CMB-based estimates that assume a flat ΛCDM cosmology is an important corroboration of this minimal cosmological model. For constant dark energy (Λ), our BAO+SN+CMB combination yields matter density Ωm=0.301±0.008 and curvature Ωk=-0.003±0.003. When we allow more general forms of evolving dark energy, the BAO+SN+CMB parameter constraints are always consistent with flat ΛCDM values at ≈1σ. While the overall χ2 of model fits is satisfactory, the LyaF BAO measurements are in moderate (2-2.5σ) tension with model predictions. Models with early dark energy that tracks the dominant energy component at high redshift remain consistent with our expansion history constraints, and they yield a higher H0 and lower matter clustering amplitude, improving agreement with some low redshift observations. Expansion history alone yields an upper limit on the summed mass of neutrino species, mν

    Original languageEnglish (US)
    Article number123516
    JournalPhysical Review D - Particles, Fields, Gravitation and Cosmology
    Volume92
    Issue number12
    DOIs
    StatePublished - Dec 14 2015

    Fingerprint

    baryons
    oscillations
    dark energy
    acoustics
    microwaves
    supernovae
    curvature
    histories
    expansion
    ladders
    cosmology
    horizon
    confidence
    neutrinos
    universe
    galaxies
    physics
    estimates
    predictions

    ASJC Scopus subject areas

    • Nuclear and High Energy Physics

    Cite this

    Aubourg, É., Bailey, S., Bautista, J. E., Beutler, F., Bhardwaj, V., Bizyaev, D., ... Zhao, G. B. (2015). Cosmological implications of baryon acoustic oscillation measurements. Physical Review D - Particles, Fields, Gravitation and Cosmology, 92(12), [123516]. https://doi.org/10.1103/PhysRevD.92.123516

    Cosmological implications of baryon acoustic oscillation measurements. / Aubourg, Éric; Bailey, Stephen; Bautista, Julian E.; Beutler, Florian; Bhardwaj, Vaishali; Bizyaev, Dmitry; Blanton, Michael; Blomqvist, Michael; Bolton, Adam S.; Bovy, Jo; Brewington, Howard; Brinkmann, J.; Brownstein, Joel R.; Burden, Angela; Busca, Nicolás G.; Carithers, William; Chuang, Chia Hsun; Comparat, Johan; Croft, Rupert A C; Cuesta, Antonio J.; Dawson, Kyle S.; Delubac, Timothée; Eisenstein, Daniel J.; Font-Ribera, Andreu; Ge, Jian; Le Goff, J. M.; Gontcho, Satya Gontcho A; Gott, J. Richard; Gunn, James E.; Guo, Hong; Guy, Julien; Hamilton, Jean Christophe; Ho, Shirley; Honscheid, Klaus; Howlett, Cullan; Kirkby, David; Kitaura, Francisco S.; Kneib, Jean Paul; Lee, Khee Gan; Long, Dan; Lupton, Robert H.; Magaña, Mariana Vargas; Malanushenko, Viktor; Malanushenko, Elena; Manera, Marc; Maraston, Claudia; Margala, Daniel; McBride, Cameron K.; Miralda-Escudé, Jordi; Myers, Adam D.; Nichol, Robert C.; Noterdaeme, Pasquier; Nuza, Sebastián E.; Olmstead, Matthew D.; Oravetz, Daniel; Pâris, Isabelle; Padmanabhan, Nikhil; Palanque-Delabrouille, Nathalie; Pan, Kaike; Pellejero-Ibanez, Marcos; Percival, Will J.; Petitjean, Patrick; Pieri, Matthew M.; Prada, Francisco; Reid, Beth; Rich, James; Roe, Natalie A.; Ross, Ashley J.; Ross, Nicholas P.; Rossi, Graziano; Rubiño-Martín, Jose Alberto; Sánchez, Ariel G.; Samushia, Lado; Santos, Ricardo Tanausú Génova; Scóccola, Claudia G.; Schlegel, David J.; Schneider, Donald P.; Seo, Hee Jong; Sheldon, Erin; Simmons, Audrey; Skibba, Ramin A.; Slosar, Anže; Strauss, Michael A.; Thomas, Daniel; Tinker, Jeremy L.; Tojeiro, Rita; Vazquez, Jose Alberto; Viel, Matteo; Wake, David A.; Weaver, Benjamin A.; Weinberg, David H.; Wood-Vasey, W. M.; Yèche, Christophe; Zehavi, Idit; Zhao, Gong Bo.

    In: Physical Review D - Particles, Fields, Gravitation and Cosmology, Vol. 92, No. 12, 123516, 14.12.2015.

    Research output: Contribution to journalArticle

    Aubourg, É, Bailey, S, Bautista, JE, Beutler, F, Bhardwaj, V, Bizyaev, D, Blanton, M, Blomqvist, M, Bolton, AS, Bovy, J, Brewington, H, Brinkmann, J, Brownstein, JR, Burden, A, Busca, NG, Carithers, W, Chuang, CH, Comparat, J, Croft, RAC, Cuesta, AJ, Dawson, KS, Delubac, T, Eisenstein, DJ, Font-Ribera, A, Ge, J, Le Goff, JM, Gontcho, SGA, Gott, JR, Gunn, JE, Guo, H, Guy, J, Hamilton, JC, Ho, S, Honscheid, K, Howlett, C, Kirkby, D, Kitaura, FS, Kneib, JP, Lee, KG, Long, D, Lupton, RH, Magaña, MV, Malanushenko, V, Malanushenko, E, Manera, M, Maraston, C, Margala, D, McBride, CK, Miralda-Escudé, J, Myers, AD, Nichol, RC, Noterdaeme, P, Nuza, SE, Olmstead, MD, Oravetz, D, Pâris, I, Padmanabhan, N, Palanque-Delabrouille, N, Pan, K, Pellejero-Ibanez, M, Percival, WJ, Petitjean, P, Pieri, MM, Prada, F, Reid, B, Rich, J, Roe, NA, Ross, AJ, Ross, NP, Rossi, G, Rubiño-Martín, JA, Sánchez, AG, Samushia, L, Santos, RTG, Scóccola, CG, Schlegel, DJ, Schneider, DP, Seo, HJ, Sheldon, E, Simmons, A, Skibba, RA, Slosar, A, Strauss, MA, Thomas, D, Tinker, JL, Tojeiro, R, Vazquez, JA, Viel, M, Wake, DA, Weaver, BA, Weinberg, DH, Wood-Vasey, WM, Yèche, C, Zehavi, I & Zhao, GB 2015, 'Cosmological implications of baryon acoustic oscillation measurements', Physical Review D - Particles, Fields, Gravitation and Cosmology, vol. 92, no. 12, 123516. https://doi.org/10.1103/PhysRevD.92.123516
    Aubourg, Éric ; Bailey, Stephen ; Bautista, Julian E. ; Beutler, Florian ; Bhardwaj, Vaishali ; Bizyaev, Dmitry ; Blanton, Michael ; Blomqvist, Michael ; Bolton, Adam S. ; Bovy, Jo ; Brewington, Howard ; Brinkmann, J. ; Brownstein, Joel R. ; Burden, Angela ; Busca, Nicolás G. ; Carithers, William ; Chuang, Chia Hsun ; Comparat, Johan ; Croft, Rupert A C ; Cuesta, Antonio J. ; Dawson, Kyle S. ; Delubac, Timothée ; Eisenstein, Daniel J. ; Font-Ribera, Andreu ; Ge, Jian ; Le Goff, J. M. ; Gontcho, Satya Gontcho A ; Gott, J. Richard ; Gunn, James E. ; Guo, Hong ; Guy, Julien ; Hamilton, Jean Christophe ; Ho, Shirley ; Honscheid, Klaus ; Howlett, Cullan ; Kirkby, David ; Kitaura, Francisco S. ; Kneib, Jean Paul ; Lee, Khee Gan ; Long, Dan ; Lupton, Robert H. ; Magaña, Mariana Vargas ; Malanushenko, Viktor ; Malanushenko, Elena ; Manera, Marc ; Maraston, Claudia ; Margala, Daniel ; McBride, Cameron K. ; Miralda-Escudé, Jordi ; Myers, Adam D. ; Nichol, Robert C. ; Noterdaeme, Pasquier ; Nuza, Sebastián E. ; Olmstead, Matthew D. ; Oravetz, Daniel ; Pâris, Isabelle ; Padmanabhan, Nikhil ; Palanque-Delabrouille, Nathalie ; Pan, Kaike ; Pellejero-Ibanez, Marcos ; Percival, Will J. ; Petitjean, Patrick ; Pieri, Matthew M. ; Prada, Francisco ; Reid, Beth ; Rich, James ; Roe, Natalie A. ; Ross, Ashley J. ; Ross, Nicholas P. ; Rossi, Graziano ; Rubiño-Martín, Jose Alberto ; Sánchez, Ariel G. ; Samushia, Lado ; Santos, Ricardo Tanausú Génova ; Scóccola, Claudia G. ; Schlegel, David J. ; Schneider, Donald P. ; Seo, Hee Jong ; Sheldon, Erin ; Simmons, Audrey ; Skibba, Ramin A. ; Slosar, Anže ; Strauss, Michael A. ; Thomas, Daniel ; Tinker, Jeremy L. ; Tojeiro, Rita ; Vazquez, Jose Alberto ; Viel, Matteo ; Wake, David A. ; Weaver, Benjamin A. ; Weinberg, David H. ; Wood-Vasey, W. M. ; Yèche, Christophe ; Zehavi, Idit ; Zhao, Gong Bo. / Cosmological implications of baryon acoustic oscillation measurements. In: Physical Review D - Particles, Fields, Gravitation and Cosmology. 2015 ; Vol. 92, No. 12.
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    title = "Cosmological implications of baryon acoustic oscillation measurements",
    abstract = "We derive constraints on cosmological parameters and tests of dark energy models from the combination of baryon acoustic oscillation (BAO) measurements with cosmic microwave background (CMB) data and a recent reanalysis of Type Ia supernova (SN) data. In particular, we take advantage of high-precision BAO measurements from galaxy clustering and the Lyman-α forest (LyaF) in the SDSS-III Baryon Oscillation Spectroscopic Survey (BOSS). Treating the BAO scale as an uncalibrated standard ruler, BAO data alone yield a high confidence detection of dark energy; in combination with the CMB angular acoustic scale they further imply a nearly flat universe. Adding the CMB-calibrated physical scale of the sound horizon, the combination of BAO and SN data into an {"}inverse distance ladder{"} yields a measurement of H0=67.3±1.1 km s-1 Mpc-1, with 1.7{\%} precision. This measurement assumes standard prerecombination physics but is insensitive to assumptions about dark energy or space curvature, so agreement with CMB-based estimates that assume a flat ΛCDM cosmology is an important corroboration of this minimal cosmological model. For constant dark energy (Λ), our BAO+SN+CMB combination yields matter density Ωm=0.301±0.008 and curvature Ωk=-0.003±0.003. When we allow more general forms of evolving dark energy, the BAO+SN+CMB parameter constraints are always consistent with flat ΛCDM values at ≈1σ. While the overall χ2 of model fits is satisfactory, the LyaF BAO measurements are in moderate (2-2.5σ) tension with model predictions. Models with early dark energy that tracks the dominant energy component at high redshift remain consistent with our expansion history constraints, and they yield a higher H0 and lower matter clustering amplitude, improving agreement with some low redshift observations. Expansion history alone yields an upper limit on the summed mass of neutrino species, mν",
    author = "{\'E}ric Aubourg and Stephen Bailey and Bautista, {Julian E.} and Florian Beutler and Vaishali Bhardwaj and Dmitry Bizyaev and Michael Blanton and Michael Blomqvist and Bolton, {Adam S.} and Jo Bovy and Howard Brewington and J. Brinkmann and Brownstein, {Joel R.} and Angela Burden and Busca, {Nicol{\'a}s G.} and William Carithers and Chuang, {Chia Hsun} and Johan Comparat and Croft, {Rupert A C} and Cuesta, {Antonio J.} and Dawson, {Kyle S.} and Timoth{\'e}e Delubac and Eisenstein, {Daniel J.} and Andreu Font-Ribera and Jian Ge and {Le Goff}, {J. M.} and Gontcho, {Satya Gontcho A} and Gott, {J. Richard} and Gunn, {James E.} and Hong Guo and Julien Guy and Hamilton, {Jean Christophe} and Shirley Ho and Klaus Honscheid and Cullan Howlett and David Kirkby and Kitaura, {Francisco S.} and Kneib, {Jean Paul} and Lee, {Khee Gan} and Dan Long and Lupton, {Robert H.} and Maga{\~n}a, {Mariana Vargas} and Viktor Malanushenko and Elena Malanushenko and Marc Manera and Claudia Maraston and Daniel Margala and McBride, {Cameron K.} and Jordi Miralda-Escud{\'e} and Myers, {Adam D.} and Nichol, {Robert C.} and Pasquier Noterdaeme and Nuza, {Sebasti{\'a}n E.} and Olmstead, {Matthew D.} and Daniel Oravetz and Isabelle P{\^a}ris and Nikhil Padmanabhan and Nathalie Palanque-Delabrouille and Kaike Pan and Marcos Pellejero-Ibanez and Percival, {Will J.} and Patrick Petitjean and Pieri, {Matthew M.} and Francisco Prada and Beth Reid and James Rich and Roe, {Natalie A.} and Ross, {Ashley J.} and Ross, {Nicholas P.} and Graziano Rossi and Rubi{\~n}o-Mart{\'i}n, {Jose Alberto} and S{\'a}nchez, {Ariel G.} and Lado Samushia and Santos, {Ricardo Tanaus{\'u} G{\'e}nova} and Sc{\'o}ccola, {Claudia G.} and Schlegel, {David J.} and Schneider, {Donald P.} and Seo, {Hee Jong} and Erin Sheldon and Audrey Simmons and Skibba, {Ramin A.} and Anže Slosar and Strauss, {Michael A.} and Daniel Thomas and Tinker, {Jeremy L.} and Rita Tojeiro and Vazquez, {Jose Alberto} and Matteo Viel and Wake, {David A.} and Weaver, {Benjamin A.} and Weinberg, {David H.} and Wood-Vasey, {W. M.} and Christophe Y{\`e}che and Idit Zehavi and Zhao, {Gong Bo}",
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    doi = "10.1103/PhysRevD.92.123516",
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    T1 - Cosmological implications of baryon acoustic oscillation measurements

    AU - Aubourg, Éric

    AU - Bailey, Stephen

    AU - Bautista, Julian E.

    AU - Beutler, Florian

    AU - Bhardwaj, Vaishali

    AU - Bizyaev, Dmitry

    AU - Blanton, Michael

    AU - Blomqvist, Michael

    AU - Bolton, Adam S.

    AU - Bovy, Jo

    AU - Brewington, Howard

    AU - Brinkmann, J.

    AU - Brownstein, Joel R.

    AU - Burden, Angela

    AU - Busca, Nicolás G.

    AU - Carithers, William

    AU - Chuang, Chia Hsun

    AU - Comparat, Johan

    AU - Croft, Rupert A C

    AU - Cuesta, Antonio J.

    AU - Dawson, Kyle S.

    AU - Delubac, Timothée

    AU - Eisenstein, Daniel J.

    AU - Font-Ribera, Andreu

    AU - Ge, Jian

    AU - Le Goff, J. M.

    AU - Gontcho, Satya Gontcho A

    AU - Gott, J. Richard

    AU - Gunn, James E.

    AU - Guo, Hong

    AU - Guy, Julien

    AU - Hamilton, Jean Christophe

    AU - Ho, Shirley

    AU - Honscheid, Klaus

    AU - Howlett, Cullan

    AU - Kirkby, David

    AU - Kitaura, Francisco S.

    AU - Kneib, Jean Paul

    AU - Lee, Khee Gan

    AU - Long, Dan

    AU - Lupton, Robert H.

    AU - Magaña, Mariana Vargas

    AU - Malanushenko, Viktor

    AU - Malanushenko, Elena

    AU - Manera, Marc

    AU - Maraston, Claudia

    AU - Margala, Daniel

    AU - McBride, Cameron K.

    AU - Miralda-Escudé, Jordi

    AU - Myers, Adam D.

    AU - Nichol, Robert C.

    AU - Noterdaeme, Pasquier

    AU - Nuza, Sebastián E.

    AU - Olmstead, Matthew D.

    AU - Oravetz, Daniel

    AU - Pâris, Isabelle

    AU - Padmanabhan, Nikhil

    AU - Palanque-Delabrouille, Nathalie

    AU - Pan, Kaike

    AU - Pellejero-Ibanez, Marcos

    AU - Percival, Will J.

    AU - Petitjean, Patrick

    AU - Pieri, Matthew M.

    AU - Prada, Francisco

    AU - Reid, Beth

    AU - Rich, James

    AU - Roe, Natalie A.

    AU - Ross, Ashley J.

    AU - Ross, Nicholas P.

    AU - Rossi, Graziano

    AU - Rubiño-Martín, Jose Alberto

    AU - Sánchez, Ariel G.

    AU - Samushia, Lado

    AU - Santos, Ricardo Tanausú Génova

    AU - Scóccola, Claudia G.

    AU - Schlegel, David J.

    AU - Schneider, Donald P.

    AU - Seo, Hee Jong

    AU - Sheldon, Erin

    AU - Simmons, Audrey

    AU - Skibba, Ramin A.

    AU - Slosar, Anže

    AU - Strauss, Michael A.

    AU - Thomas, Daniel

    AU - Tinker, Jeremy L.

    AU - Tojeiro, Rita

    AU - Vazquez, Jose Alberto

    AU - Viel, Matteo

    AU - Wake, David A.

    AU - Weaver, Benjamin A.

    AU - Weinberg, David H.

    AU - Wood-Vasey, W. M.

    AU - Yèche, Christophe

    AU - Zehavi, Idit

    AU - Zhao, Gong Bo

    PY - 2015/12/14

    Y1 - 2015/12/14

    N2 - We derive constraints on cosmological parameters and tests of dark energy models from the combination of baryon acoustic oscillation (BAO) measurements with cosmic microwave background (CMB) data and a recent reanalysis of Type Ia supernova (SN) data. In particular, we take advantage of high-precision BAO measurements from galaxy clustering and the Lyman-α forest (LyaF) in the SDSS-III Baryon Oscillation Spectroscopic Survey (BOSS). Treating the BAO scale as an uncalibrated standard ruler, BAO data alone yield a high confidence detection of dark energy; in combination with the CMB angular acoustic scale they further imply a nearly flat universe. Adding the CMB-calibrated physical scale of the sound horizon, the combination of BAO and SN data into an "inverse distance ladder" yields a measurement of H0=67.3±1.1 km s-1 Mpc-1, with 1.7% precision. This measurement assumes standard prerecombination physics but is insensitive to assumptions about dark energy or space curvature, so agreement with CMB-based estimates that assume a flat ΛCDM cosmology is an important corroboration of this minimal cosmological model. For constant dark energy (Λ), our BAO+SN+CMB combination yields matter density Ωm=0.301±0.008 and curvature Ωk=-0.003±0.003. When we allow more general forms of evolving dark energy, the BAO+SN+CMB parameter constraints are always consistent with flat ΛCDM values at ≈1σ. While the overall χ2 of model fits is satisfactory, the LyaF BAO measurements are in moderate (2-2.5σ) tension with model predictions. Models with early dark energy that tracks the dominant energy component at high redshift remain consistent with our expansion history constraints, and they yield a higher H0 and lower matter clustering amplitude, improving agreement with some low redshift observations. Expansion history alone yields an upper limit on the summed mass of neutrino species, mν

    AB - We derive constraints on cosmological parameters and tests of dark energy models from the combination of baryon acoustic oscillation (BAO) measurements with cosmic microwave background (CMB) data and a recent reanalysis of Type Ia supernova (SN) data. In particular, we take advantage of high-precision BAO measurements from galaxy clustering and the Lyman-α forest (LyaF) in the SDSS-III Baryon Oscillation Spectroscopic Survey (BOSS). Treating the BAO scale as an uncalibrated standard ruler, BAO data alone yield a high confidence detection of dark energy; in combination with the CMB angular acoustic scale they further imply a nearly flat universe. Adding the CMB-calibrated physical scale of the sound horizon, the combination of BAO and SN data into an "inverse distance ladder" yields a measurement of H0=67.3±1.1 km s-1 Mpc-1, with 1.7% precision. This measurement assumes standard prerecombination physics but is insensitive to assumptions about dark energy or space curvature, so agreement with CMB-based estimates that assume a flat ΛCDM cosmology is an important corroboration of this minimal cosmological model. For constant dark energy (Λ), our BAO+SN+CMB combination yields matter density Ωm=0.301±0.008 and curvature Ωk=-0.003±0.003. When we allow more general forms of evolving dark energy, the BAO+SN+CMB parameter constraints are always consistent with flat ΛCDM values at ≈1σ. While the overall χ2 of model fits is satisfactory, the LyaF BAO measurements are in moderate (2-2.5σ) tension with model predictions. Models with early dark energy that tracks the dominant energy component at high redshift remain consistent with our expansion history constraints, and they yield a higher H0 and lower matter clustering amplitude, improving agreement with some low redshift observations. Expansion history alone yields an upper limit on the summed mass of neutrino species, mν

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    U2 - 10.1103/PhysRevD.92.123516

    DO - 10.1103/PhysRevD.92.123516

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    JO - Physical review D: Particles and fields

    JF - Physical review D: Particles and fields

    SN - 1550-7998

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    ER -