Search for chameleons with CAST
In this work we present a search for (solar) chameleons with the CERN Axion Solar Telescope (CAST). This novel experimental technique, in the field of dark energy research, exploits both the chameleon coupling to matter ( β m ) and to photons ( β γ ) via the Primakoff effect. By reducing the X-ray d...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Anastassopoulos, V. [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2015transfer abstract |
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| Schlagwörter: |
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| Umfang: |
9 |
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| Übergeordnetes Werk: |
Enthalten in: Applying the Go/NoGo processing schema to a visual oddball task in older adults - Steiner, Genevieve Z. ELSEVIER, 2016, Amsterdam |
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| Übergeordnetes Werk: |
volume:749 ; year:2015 ; day:7 ; month:10 ; pages:172-180 ; extent:9 |
| Links: |
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| DOI / URN: |
10.1016/j.physletb.2015.07.049 |
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| 520 | |a In this work we present a search for (solar) chameleons with the CERN Axion Solar Telescope (CAST). This novel experimental technique, in the field of dark energy research, exploits both the chameleon coupling to matter ( β m ) and to photons ( β γ ) via the Primakoff effect. By reducing the X-ray detection energy threshold used for axions from 1 keV to 400 eV CAST became sensitive to the converted solar chameleon spectrum which peaks around 600 eV. Even though we have not observed any excess above background, we can provide a 95% C.L. limit for the coupling strength of chameleons to photons of β γ ≲ 10 11 for 1 < β m < 10 6 . | ||
| 520 | |a In this work we present a search for (solar) chameleons with the CERN Axion Solar Telescope (CAST). This novel experimental technique, in the field of dark energy research, exploits both the chameleon coupling to matter ( β m ) and to photons ( β γ ) via the Primakoff effect. By reducing the X-ray detection energy threshold used for axions from 1 keV to 400 eV CAST became sensitive to the converted solar chameleon spectrum which peaks around 600 eV. Even though we have not observed any excess above background, we can provide a 95% C.L. limit for the coupling strength of chameleons to photons of β γ ≲ 10 11 for 1 < β m < 10 6 . | ||
| 650 | 7 | |a CAST |2 Elsevier | |
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| 650 | 7 | |a X-ray |2 Elsevier | |
| 650 | 7 | |a Dark energy |2 Elsevier | |
| 650 | 7 | |a Chameleon |2 Elsevier | |
| 700 | 1 | |a Arik, M. |4 oth | |
| 700 | 1 | |a Aune, S. |4 oth | |
| 700 | 1 | |a Barth, K. |4 oth | |
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10.1016/j.physletb.2015.07.049 doi GBVA2015012000011.pica (DE-627)ELV013044095 (ELSEVIER)S0370-2693(15)00559-6 DE-627 ger DE-627 rakwb eng 530 DE-600 610 VZ 77.50 bkl Anastassopoulos, V. verfasserin aut Search for chameleons with CAST 2015transfer abstract 9 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier In this work we present a search for (solar) chameleons with the CERN Axion Solar Telescope (CAST). This novel experimental technique, in the field of dark energy research, exploits both the chameleon coupling to matter ( β m ) and to photons ( β γ ) via the Primakoff effect. By reducing the X-ray detection energy threshold used for axions from 1 keV to 400 eV CAST became sensitive to the converted solar chameleon spectrum which peaks around 600 eV. Even though we have not observed any excess above background, we can provide a 95% C.L. limit for the coupling strength of chameleons to photons of β γ ≲ 10 11 for 1 < β m < 10 6 . In this work we present a search for (solar) chameleons with the CERN Axion Solar Telescope (CAST). This novel experimental technique, in the field of dark energy research, exploits both the chameleon coupling to matter ( β m ) and to photons ( β γ ) via the Primakoff effect. By reducing the X-ray detection energy threshold used for axions from 1 keV to 400 eV CAST became sensitive to the converted solar chameleon spectrum which peaks around 600 eV. Even though we have not observed any excess above background, we can provide a 95% C.L. limit for the coupling strength of chameleons to photons of β γ ≲ 10 11 for 1 < β m < 10 6 . CAST Elsevier SDD Elsevier Tachocline Elsevier X-ray Elsevier Dark energy Elsevier Chameleon Elsevier Arik, M. oth Aune, S. oth Barth, K. oth Belov, A. oth Bräuninger, H. oth Cantatore, G. oth Carmona, J.M. oth Cetin, S.A. oth Christensen, F. oth Collar, J.I. oth Dafni, T. oth Davenport, M. oth Desch, K. oth Dermenev, A. oth Eleftheriadis, C. oth Fanourakis, G. oth Ferrer-Ribas, E. oth Friedrich, P. oth Galán, J. oth García, J.A. oth Gardikiotis, A. oth Garza, J.G. oth Gazis, E.N. oth Geralis, T. oth Giomataris, I. oth Hailey, C. oth Haug, F. oth Hasinoff, M.D. oth Hoffmann, D.H.H. oth Iguaz, F.J. oth Irastorza, I.G. oth Jacoby, J. oth Jakobsen, A. oth Jakovčić, K. oth Kaminski, J. oth Karuza, M. oth Kavuk, M. oth Krčmar, M. oth Krieger, C. oth Krüger, A. oth Lakić, B. oth Laurent, J.M. oth Liolios, A. oth Ljubičić, A. oth Luzón, G. oth Neff, S. oth Ortega, I. oth Papaevangelou, T. oth Pivovaroff, M.J. oth Raffelt, G. oth Riege, H. oth Rosu, M. oth Ruz, J. oth Savvidis, I. oth Solanki, S.K. oth Vafeiadis, T. oth Villar, J.A. oth Vogel, J.K. oth Yildiz, S.C. oth Zioutas, K. oth Brax, P. oth Lavrentyev, I. oth Upadhye, A. oth Enthalten in North-Holland Publ Steiner, Genevieve Z. ELSEVIER Applying the Go/NoGo processing schema to a visual oddball task in older adults 2016 Amsterdam (DE-627)ELV000151122 volume:749 year:2015 day:7 month:10 pages:172-180 extent:9 https://doi.org/10.1016/j.physletb.2015.07.049 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA 77.50 Psychophysiologie VZ AR 749 2015 7 1007 172-180 9 |
| spelling |
10.1016/j.physletb.2015.07.049 doi GBVA2015012000011.pica (DE-627)ELV013044095 (ELSEVIER)S0370-2693(15)00559-6 DE-627 ger DE-627 rakwb eng 530 DE-600 610 VZ 77.50 bkl Anastassopoulos, V. verfasserin aut Search for chameleons with CAST 2015transfer abstract 9 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier In this work we present a search for (solar) chameleons with the CERN Axion Solar Telescope (CAST). This novel experimental technique, in the field of dark energy research, exploits both the chameleon coupling to matter ( β m ) and to photons ( β γ ) via the Primakoff effect. By reducing the X-ray detection energy threshold used for axions from 1 keV to 400 eV CAST became sensitive to the converted solar chameleon spectrum which peaks around 600 eV. Even though we have not observed any excess above background, we can provide a 95% C.L. limit for the coupling strength of chameleons to photons of β γ ≲ 10 11 for 1 < β m < 10 6 . In this work we present a search for (solar) chameleons with the CERN Axion Solar Telescope (CAST). This novel experimental technique, in the field of dark energy research, exploits both the chameleon coupling to matter ( β m ) and to photons ( β γ ) via the Primakoff effect. By reducing the X-ray detection energy threshold used for axions from 1 keV to 400 eV CAST became sensitive to the converted solar chameleon spectrum which peaks around 600 eV. Even though we have not observed any excess above background, we can provide a 95% C.L. limit for the coupling strength of chameleons to photons of β γ ≲ 10 11 for 1 < β m < 10 6 . CAST Elsevier SDD Elsevier Tachocline Elsevier X-ray Elsevier Dark energy Elsevier Chameleon Elsevier Arik, M. oth Aune, S. oth Barth, K. oth Belov, A. oth Bräuninger, H. oth Cantatore, G. oth Carmona, J.M. oth Cetin, S.A. oth Christensen, F. oth Collar, J.I. oth Dafni, T. oth Davenport, M. oth Desch, K. oth Dermenev, A. oth Eleftheriadis, C. oth Fanourakis, G. oth Ferrer-Ribas, E. oth Friedrich, P. oth Galán, J. oth García, J.A. oth Gardikiotis, A. oth Garza, J.G. oth Gazis, E.N. oth Geralis, T. oth Giomataris, I. oth Hailey, C. oth Haug, F. oth Hasinoff, M.D. oth Hoffmann, D.H.H. oth Iguaz, F.J. oth Irastorza, I.G. oth Jacoby, J. oth Jakobsen, A. oth Jakovčić, K. oth Kaminski, J. oth Karuza, M. oth Kavuk, M. oth Krčmar, M. oth Krieger, C. oth Krüger, A. oth Lakić, B. oth Laurent, J.M. oth Liolios, A. oth Ljubičić, A. oth Luzón, G. oth Neff, S. oth Ortega, I. oth Papaevangelou, T. oth Pivovaroff, M.J. oth Raffelt, G. oth Riege, H. oth Rosu, M. oth Ruz, J. oth Savvidis, I. oth Solanki, S.K. oth Vafeiadis, T. oth Villar, J.A. oth Vogel, J.K. oth Yildiz, S.C. oth Zioutas, K. oth Brax, P. oth Lavrentyev, I. oth Upadhye, A. oth Enthalten in North-Holland Publ Steiner, Genevieve Z. ELSEVIER Applying the Go/NoGo processing schema to a visual oddball task in older adults 2016 Amsterdam (DE-627)ELV000151122 volume:749 year:2015 day:7 month:10 pages:172-180 extent:9 https://doi.org/10.1016/j.physletb.2015.07.049 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA 77.50 Psychophysiologie VZ AR 749 2015 7 1007 172-180 9 |
| allfields_unstemmed |
10.1016/j.physletb.2015.07.049 doi GBVA2015012000011.pica (DE-627)ELV013044095 (ELSEVIER)S0370-2693(15)00559-6 DE-627 ger DE-627 rakwb eng 530 DE-600 610 VZ 77.50 bkl Anastassopoulos, V. verfasserin aut Search for chameleons with CAST 2015transfer abstract 9 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier In this work we present a search for (solar) chameleons with the CERN Axion Solar Telescope (CAST). This novel experimental technique, in the field of dark energy research, exploits both the chameleon coupling to matter ( β m ) and to photons ( β γ ) via the Primakoff effect. By reducing the X-ray detection energy threshold used for axions from 1 keV to 400 eV CAST became sensitive to the converted solar chameleon spectrum which peaks around 600 eV. Even though we have not observed any excess above background, we can provide a 95% C.L. limit for the coupling strength of chameleons to photons of β γ ≲ 10 11 for 1 < β m < 10 6 . In this work we present a search for (solar) chameleons with the CERN Axion Solar Telescope (CAST). This novel experimental technique, in the field of dark energy research, exploits both the chameleon coupling to matter ( β m ) and to photons ( β γ ) via the Primakoff effect. By reducing the X-ray detection energy threshold used for axions from 1 keV to 400 eV CAST became sensitive to the converted solar chameleon spectrum which peaks around 600 eV. Even though we have not observed any excess above background, we can provide a 95% C.L. limit for the coupling strength of chameleons to photons of β γ ≲ 10 11 for 1 < β m < 10 6 . CAST Elsevier SDD Elsevier Tachocline Elsevier X-ray Elsevier Dark energy Elsevier Chameleon Elsevier Arik, M. oth Aune, S. oth Barth, K. oth Belov, A. oth Bräuninger, H. oth Cantatore, G. oth Carmona, J.M. oth Cetin, S.A. oth Christensen, F. oth Collar, J.I. oth Dafni, T. oth Davenport, M. oth Desch, K. oth Dermenev, A. oth Eleftheriadis, C. oth Fanourakis, G. oth Ferrer-Ribas, E. oth Friedrich, P. oth Galán, J. oth García, J.A. oth Gardikiotis, A. oth Garza, J.G. oth Gazis, E.N. oth Geralis, T. oth Giomataris, I. oth Hailey, C. oth Haug, F. oth Hasinoff, M.D. oth Hoffmann, D.H.H. oth Iguaz, F.J. oth Irastorza, I.G. oth Jacoby, J. oth Jakobsen, A. oth Jakovčić, K. oth Kaminski, J. oth Karuza, M. oth Kavuk, M. oth Krčmar, M. oth Krieger, C. oth Krüger, A. oth Lakić, B. oth Laurent, J.M. oth Liolios, A. oth Ljubičić, A. oth Luzón, G. oth Neff, S. oth Ortega, I. oth Papaevangelou, T. oth Pivovaroff, M.J. oth Raffelt, G. oth Riege, H. oth Rosu, M. oth Ruz, J. oth Savvidis, I. oth Solanki, S.K. oth Vafeiadis, T. oth Villar, J.A. oth Vogel, J.K. oth Yildiz, S.C. oth Zioutas, K. oth Brax, P. oth Lavrentyev, I. oth Upadhye, A. oth Enthalten in North-Holland Publ Steiner, Genevieve Z. ELSEVIER Applying the Go/NoGo processing schema to a visual oddball task in older adults 2016 Amsterdam (DE-627)ELV000151122 volume:749 year:2015 day:7 month:10 pages:172-180 extent:9 https://doi.org/10.1016/j.physletb.2015.07.049 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA 77.50 Psychophysiologie VZ AR 749 2015 7 1007 172-180 9 |
| allfieldsGer |
10.1016/j.physletb.2015.07.049 doi GBVA2015012000011.pica (DE-627)ELV013044095 (ELSEVIER)S0370-2693(15)00559-6 DE-627 ger DE-627 rakwb eng 530 DE-600 610 VZ 77.50 bkl Anastassopoulos, V. verfasserin aut Search for chameleons with CAST 2015transfer abstract 9 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier In this work we present a search for (solar) chameleons with the CERN Axion Solar Telescope (CAST). This novel experimental technique, in the field of dark energy research, exploits both the chameleon coupling to matter ( β m ) and to photons ( β γ ) via the Primakoff effect. By reducing the X-ray detection energy threshold used for axions from 1 keV to 400 eV CAST became sensitive to the converted solar chameleon spectrum which peaks around 600 eV. Even though we have not observed any excess above background, we can provide a 95% C.L. limit for the coupling strength of chameleons to photons of β γ ≲ 10 11 for 1 < β m < 10 6 . In this work we present a search for (solar) chameleons with the CERN Axion Solar Telescope (CAST). This novel experimental technique, in the field of dark energy research, exploits both the chameleon coupling to matter ( β m ) and to photons ( β γ ) via the Primakoff effect. By reducing the X-ray detection energy threshold used for axions from 1 keV to 400 eV CAST became sensitive to the converted solar chameleon spectrum which peaks around 600 eV. Even though we have not observed any excess above background, we can provide a 95% C.L. limit for the coupling strength of chameleons to photons of β γ ≲ 10 11 for 1 < β m < 10 6 . CAST Elsevier SDD Elsevier Tachocline Elsevier X-ray Elsevier Dark energy Elsevier Chameleon Elsevier Arik, M. oth Aune, S. oth Barth, K. oth Belov, A. oth Bräuninger, H. oth Cantatore, G. oth Carmona, J.M. oth Cetin, S.A. oth Christensen, F. oth Collar, J.I. oth Dafni, T. oth Davenport, M. oth Desch, K. oth Dermenev, A. oth Eleftheriadis, C. oth Fanourakis, G. oth Ferrer-Ribas, E. oth Friedrich, P. oth Galán, J. oth García, J.A. oth Gardikiotis, A. oth Garza, J.G. oth Gazis, E.N. oth Geralis, T. oth Giomataris, I. oth Hailey, C. oth Haug, F. oth Hasinoff, M.D. oth Hoffmann, D.H.H. oth Iguaz, F.J. oth Irastorza, I.G. oth Jacoby, J. oth Jakobsen, A. oth Jakovčić, K. oth Kaminski, J. oth Karuza, M. oth Kavuk, M. oth Krčmar, M. oth Krieger, C. oth Krüger, A. oth Lakić, B. oth Laurent, J.M. oth Liolios, A. oth Ljubičić, A. oth Luzón, G. oth Neff, S. oth Ortega, I. oth Papaevangelou, T. oth Pivovaroff, M.J. oth Raffelt, G. oth Riege, H. oth Rosu, M. oth Ruz, J. oth Savvidis, I. oth Solanki, S.K. oth Vafeiadis, T. oth Villar, J.A. oth Vogel, J.K. oth Yildiz, S.C. oth Zioutas, K. oth Brax, P. oth Lavrentyev, I. oth Upadhye, A. oth Enthalten in North-Holland Publ Steiner, Genevieve Z. ELSEVIER Applying the Go/NoGo processing schema to a visual oddball task in older adults 2016 Amsterdam (DE-627)ELV000151122 volume:749 year:2015 day:7 month:10 pages:172-180 extent:9 https://doi.org/10.1016/j.physletb.2015.07.049 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA 77.50 Psychophysiologie VZ AR 749 2015 7 1007 172-180 9 |
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10.1016/j.physletb.2015.07.049 doi GBVA2015012000011.pica (DE-627)ELV013044095 (ELSEVIER)S0370-2693(15)00559-6 DE-627 ger DE-627 rakwb eng 530 DE-600 610 VZ 77.50 bkl Anastassopoulos, V. verfasserin aut Search for chameleons with CAST 2015transfer abstract 9 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier In this work we present a search for (solar) chameleons with the CERN Axion Solar Telescope (CAST). This novel experimental technique, in the field of dark energy research, exploits both the chameleon coupling to matter ( β m ) and to photons ( β γ ) via the Primakoff effect. By reducing the X-ray detection energy threshold used for axions from 1 keV to 400 eV CAST became sensitive to the converted solar chameleon spectrum which peaks around 600 eV. Even though we have not observed any excess above background, we can provide a 95% C.L. limit for the coupling strength of chameleons to photons of β γ ≲ 10 11 for 1 < β m < 10 6 . In this work we present a search for (solar) chameleons with the CERN Axion Solar Telescope (CAST). This novel experimental technique, in the field of dark energy research, exploits both the chameleon coupling to matter ( β m ) and to photons ( β γ ) via the Primakoff effect. By reducing the X-ray detection energy threshold used for axions from 1 keV to 400 eV CAST became sensitive to the converted solar chameleon spectrum which peaks around 600 eV. Even though we have not observed any excess above background, we can provide a 95% C.L. limit for the coupling strength of chameleons to photons of β γ ≲ 10 11 for 1 < β m < 10 6 . CAST Elsevier SDD Elsevier Tachocline Elsevier X-ray Elsevier Dark energy Elsevier Chameleon Elsevier Arik, M. oth Aune, S. oth Barth, K. oth Belov, A. oth Bräuninger, H. oth Cantatore, G. oth Carmona, J.M. oth Cetin, S.A. oth Christensen, F. oth Collar, J.I. oth Dafni, T. oth Davenport, M. oth Desch, K. oth Dermenev, A. oth Eleftheriadis, C. oth Fanourakis, G. oth Ferrer-Ribas, E. oth Friedrich, P. oth Galán, J. oth García, J.A. oth Gardikiotis, A. oth Garza, J.G. oth Gazis, E.N. oth Geralis, T. oth Giomataris, I. oth Hailey, C. oth Haug, F. oth Hasinoff, M.D. oth Hoffmann, D.H.H. oth Iguaz, F.J. oth Irastorza, I.G. oth Jacoby, J. oth Jakobsen, A. oth Jakovčić, K. oth Kaminski, J. oth Karuza, M. oth Kavuk, M. oth Krčmar, M. oth Krieger, C. oth Krüger, A. oth Lakić, B. oth Laurent, J.M. oth Liolios, A. oth Ljubičić, A. oth Luzón, G. oth Neff, S. oth Ortega, I. oth Papaevangelou, T. oth Pivovaroff, M.J. oth Raffelt, G. oth Riege, H. oth Rosu, M. oth Ruz, J. oth Savvidis, I. oth Solanki, S.K. oth Vafeiadis, T. oth Villar, J.A. oth Vogel, J.K. oth Yildiz, S.C. oth Zioutas, K. oth Brax, P. oth Lavrentyev, I. oth Upadhye, A. oth Enthalten in North-Holland Publ Steiner, Genevieve Z. ELSEVIER Applying the Go/NoGo processing schema to a visual oddball task in older adults 2016 Amsterdam (DE-627)ELV000151122 volume:749 year:2015 day:7 month:10 pages:172-180 extent:9 https://doi.org/10.1016/j.physletb.2015.07.049 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA 77.50 Psychophysiologie VZ AR 749 2015 7 1007 172-180 9 |
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Enthalten in Applying the Go/NoGo processing schema to a visual oddball task in older adults Amsterdam volume:749 year:2015 day:7 month:10 pages:172-180 extent:9 |
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Anastassopoulos, V. @@aut@@ Arik, M. @@oth@@ Aune, S. @@oth@@ Barth, K. @@oth@@ Belov, A. @@oth@@ Bräuninger, H. @@oth@@ Cantatore, G. @@oth@@ Carmona, J.M. @@oth@@ Cetin, S.A. @@oth@@ Christensen, F. @@oth@@ Collar, J.I. @@oth@@ Dafni, T. @@oth@@ Davenport, M. @@oth@@ Desch, K. @@oth@@ Dermenev, A. @@oth@@ Eleftheriadis, C. @@oth@@ Fanourakis, G. @@oth@@ Ferrer-Ribas, E. @@oth@@ Friedrich, P. @@oth@@ Galán, J. @@oth@@ García, J.A. @@oth@@ Gardikiotis, A. @@oth@@ Garza, J.G. @@oth@@ Gazis, E.N. @@oth@@ Geralis, T. @@oth@@ Giomataris, I. @@oth@@ Hailey, C. @@oth@@ Haug, F. @@oth@@ Hasinoff, M.D. @@oth@@ Hoffmann, D.H.H. @@oth@@ Iguaz, F.J. @@oth@@ Irastorza, I.G. @@oth@@ Jacoby, J. @@oth@@ Jakobsen, A. @@oth@@ Jakovčić, K. @@oth@@ Kaminski, J. @@oth@@ Karuza, M. @@oth@@ Kavuk, M. @@oth@@ Krčmar, M. @@oth@@ Krieger, C. @@oth@@ Krüger, A. @@oth@@ Lakić, B. @@oth@@ Laurent, J.M. @@oth@@ Liolios, A. @@oth@@ Ljubičić, A. @@oth@@ Luzón, G. @@oth@@ Neff, S. @@oth@@ Ortega, I. @@oth@@ Papaevangelou, T. @@oth@@ Pivovaroff, M.J. @@oth@@ Raffelt, G. @@oth@@ Riege, H. @@oth@@ Rosu, M. @@oth@@ Ruz, J. @@oth@@ Savvidis, I. @@oth@@ Solanki, S.K. @@oth@@ Vafeiadis, T. @@oth@@ Villar, J.A. @@oth@@ Vogel, J.K. @@oth@@ Yildiz, S.C. @@oth@@ Zioutas, K. @@oth@@ Brax, P. @@oth@@ Lavrentyev, I. @@oth@@ Upadhye, A. @@oth@@ |
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In this work we present a search for (solar) chameleons with the CERN Axion Solar Telescope (CAST). This novel experimental technique, in the field of dark energy research, exploits both the chameleon coupling to matter ( β m ) and to photons ( β γ ) via the Primakoff effect. By reducing the X-ray detection energy threshold used for axions from 1 keV to 400 eV CAST became sensitive to the converted solar chameleon spectrum which peaks around 600 eV. Even though we have not observed any excess above background, we can provide a 95% C.L. limit for the coupling strength of chameleons to photons of β γ ≲ 10 11 for 1 < β m < 10 6 . |
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