Searching for Cosmic Strings in New Observational Windows
Cosmic strings are predicted in many models beyond the Standard Model of particle physics. In such models, a network of strings will inevitably be formed in a phase transition in the early universe and will persist to the present time. Strings leave behind distinctive features in cosmology. Searchin...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Brandenberger, Robert H. [verfasserIn] |
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Englisch |
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2014transfer abstract |
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13 |
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Enthalten in: Fire safety risks of external living walls and implications for regulatory guidance in England - Kotzen, Benz ELSEVIER, 2023, Amsterdam |
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volume:246 ; year:2014 ; pages:45-57 ; extent:13 |
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| DOI / URN: |
10.1016/j.nuclphysbps.2013.10.064 |
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| 520 | |a Cosmic strings are predicted in many models beyond the Standard Model of particle physics. In such models, a network of strings will inevitably be formed in a phase transition in the early universe and will persist to the present time. Strings leave behind distinctive features in cosmology. Searching for these signatures in new observational windows provides a way to constrain particle physics at the high energy scale and is thus complementary to searches for new physics at the low energy end, for example at the LHC. Specifically, I will discuss signatures of cosmic strings in cosmic microwave background polarization maps and in 21cm redshift surveys. | ||
| 520 | |a Cosmic strings are predicted in many models beyond the Standard Model of particle physics. In such models, a network of strings will inevitably be formed in a phase transition in the early universe and will persist to the present time. Strings leave behind distinctive features in cosmology. Searching for these signatures in new observational windows provides a way to constrain particle physics at the high energy scale and is thus complementary to searches for new physics at the low energy end, for example at the LHC. Specifically, I will discuss signatures of cosmic strings in cosmic microwave background polarization maps and in 21cm redshift surveys. | ||
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| 650 | 7 | |a 21cm Redshift Surveys |2 Elsevier | |
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10.1016/j.nuclphysbps.2013.10.064 doi GBVA2014014000012.pica (DE-627)ELV022859071 (ELSEVIER)S0920-5632(13)00653-1 DE-627 ger DE-627 rakwb eng 530 530 DE-600 690 VZ 50.17 bkl Brandenberger, Robert H. verfasserin aut Searching for Cosmic Strings in New Observational Windows 2014transfer abstract 13 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Cosmic strings are predicted in many models beyond the Standard Model of particle physics. In such models, a network of strings will inevitably be formed in a phase transition in the early universe and will persist to the present time. Strings leave behind distinctive features in cosmology. Searching for these signatures in new observational windows provides a way to constrain particle physics at the high energy scale and is thus complementary to searches for new physics at the low energy end, for example at the LHC. Specifically, I will discuss signatures of cosmic strings in cosmic microwave background polarization maps and in 21cm redshift surveys. Cosmic strings are predicted in many models beyond the Standard Model of particle physics. In such models, a network of strings will inevitably be formed in a phase transition in the early universe and will persist to the present time. Strings leave behind distinctive features in cosmology. Searching for these signatures in new observational windows provides a way to constrain particle physics at the high energy scale and is thus complementary to searches for new physics at the low energy end, for example at the LHC. Specifically, I will discuss signatures of cosmic strings in cosmic microwave background polarization maps and in 21cm redshift surveys. Cosmic Strings Elsevier CMB Polarization Elsevier 21cm Redshift Surveys Elsevier Enthalten in Elsevier Kotzen, Benz ELSEVIER Fire safety risks of external living walls and implications for regulatory guidance in England 2023 Amsterdam (DE-627)ELV010483918 volume:246 year:2014 pages:45-57 extent:13 https://doi.org/10.1016/j.nuclphysbps.2013.10.064 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U GBV_ILN_24 GBV_ILN_110 GBV_ILN_2008 GBV_ILN_2018 50.17 Sicherheitstechnik VZ AR 246 2014 45-57 13 045F 530 |
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10.1016/j.nuclphysbps.2013.10.064 doi GBVA2014014000012.pica (DE-627)ELV022859071 (ELSEVIER)S0920-5632(13)00653-1 DE-627 ger DE-627 rakwb eng 530 530 DE-600 690 VZ 50.17 bkl Brandenberger, Robert H. verfasserin aut Searching for Cosmic Strings in New Observational Windows 2014transfer abstract 13 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Cosmic strings are predicted in many models beyond the Standard Model of particle physics. In such models, a network of strings will inevitably be formed in a phase transition in the early universe and will persist to the present time. Strings leave behind distinctive features in cosmology. Searching for these signatures in new observational windows provides a way to constrain particle physics at the high energy scale and is thus complementary to searches for new physics at the low energy end, for example at the LHC. Specifically, I will discuss signatures of cosmic strings in cosmic microwave background polarization maps and in 21cm redshift surveys. Cosmic strings are predicted in many models beyond the Standard Model of particle physics. In such models, a network of strings will inevitably be formed in a phase transition in the early universe and will persist to the present time. Strings leave behind distinctive features in cosmology. Searching for these signatures in new observational windows provides a way to constrain particle physics at the high energy scale and is thus complementary to searches for new physics at the low energy end, for example at the LHC. Specifically, I will discuss signatures of cosmic strings in cosmic microwave background polarization maps and in 21cm redshift surveys. Cosmic Strings Elsevier CMB Polarization Elsevier 21cm Redshift Surveys Elsevier Enthalten in Elsevier Kotzen, Benz ELSEVIER Fire safety risks of external living walls and implications for regulatory guidance in England 2023 Amsterdam (DE-627)ELV010483918 volume:246 year:2014 pages:45-57 extent:13 https://doi.org/10.1016/j.nuclphysbps.2013.10.064 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U GBV_ILN_24 GBV_ILN_110 GBV_ILN_2008 GBV_ILN_2018 50.17 Sicherheitstechnik VZ AR 246 2014 45-57 13 045F 530 |
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10.1016/j.nuclphysbps.2013.10.064 doi GBVA2014014000012.pica (DE-627)ELV022859071 (ELSEVIER)S0920-5632(13)00653-1 DE-627 ger DE-627 rakwb eng 530 530 DE-600 690 VZ 50.17 bkl Brandenberger, Robert H. verfasserin aut Searching for Cosmic Strings in New Observational Windows 2014transfer abstract 13 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Cosmic strings are predicted in many models beyond the Standard Model of particle physics. In such models, a network of strings will inevitably be formed in a phase transition in the early universe and will persist to the present time. Strings leave behind distinctive features in cosmology. Searching for these signatures in new observational windows provides a way to constrain particle physics at the high energy scale and is thus complementary to searches for new physics at the low energy end, for example at the LHC. Specifically, I will discuss signatures of cosmic strings in cosmic microwave background polarization maps and in 21cm redshift surveys. Cosmic strings are predicted in many models beyond the Standard Model of particle physics. In such models, a network of strings will inevitably be formed in a phase transition in the early universe and will persist to the present time. Strings leave behind distinctive features in cosmology. Searching for these signatures in new observational windows provides a way to constrain particle physics at the high energy scale and is thus complementary to searches for new physics at the low energy end, for example at the LHC. Specifically, I will discuss signatures of cosmic strings in cosmic microwave background polarization maps and in 21cm redshift surveys. Cosmic Strings Elsevier CMB Polarization Elsevier 21cm Redshift Surveys Elsevier Enthalten in Elsevier Kotzen, Benz ELSEVIER Fire safety risks of external living walls and implications for regulatory guidance in England 2023 Amsterdam (DE-627)ELV010483918 volume:246 year:2014 pages:45-57 extent:13 https://doi.org/10.1016/j.nuclphysbps.2013.10.064 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U GBV_ILN_24 GBV_ILN_110 GBV_ILN_2008 GBV_ILN_2018 50.17 Sicherheitstechnik VZ AR 246 2014 45-57 13 045F 530 |
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10.1016/j.nuclphysbps.2013.10.064 doi GBVA2014014000012.pica (DE-627)ELV022859071 (ELSEVIER)S0920-5632(13)00653-1 DE-627 ger DE-627 rakwb eng 530 530 DE-600 690 VZ 50.17 bkl Brandenberger, Robert H. verfasserin aut Searching for Cosmic Strings in New Observational Windows 2014transfer abstract 13 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Cosmic strings are predicted in many models beyond the Standard Model of particle physics. In such models, a network of strings will inevitably be formed in a phase transition in the early universe and will persist to the present time. Strings leave behind distinctive features in cosmology. Searching for these signatures in new observational windows provides a way to constrain particle physics at the high energy scale and is thus complementary to searches for new physics at the low energy end, for example at the LHC. Specifically, I will discuss signatures of cosmic strings in cosmic microwave background polarization maps and in 21cm redshift surveys. Cosmic strings are predicted in many models beyond the Standard Model of particle physics. In such models, a network of strings will inevitably be formed in a phase transition in the early universe and will persist to the present time. Strings leave behind distinctive features in cosmology. Searching for these signatures in new observational windows provides a way to constrain particle physics at the high energy scale and is thus complementary to searches for new physics at the low energy end, for example at the LHC. Specifically, I will discuss signatures of cosmic strings in cosmic microwave background polarization maps and in 21cm redshift surveys. Cosmic Strings Elsevier CMB Polarization Elsevier 21cm Redshift Surveys Elsevier Enthalten in Elsevier Kotzen, Benz ELSEVIER Fire safety risks of external living walls and implications for regulatory guidance in England 2023 Amsterdam (DE-627)ELV010483918 volume:246 year:2014 pages:45-57 extent:13 https://doi.org/10.1016/j.nuclphysbps.2013.10.064 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U GBV_ILN_24 GBV_ILN_110 GBV_ILN_2008 GBV_ILN_2018 50.17 Sicherheitstechnik VZ AR 246 2014 45-57 13 045F 530 |
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10.1016/j.nuclphysbps.2013.10.064 doi GBVA2014014000012.pica (DE-627)ELV022859071 (ELSEVIER)S0920-5632(13)00653-1 DE-627 ger DE-627 rakwb eng 530 530 DE-600 690 VZ 50.17 bkl Brandenberger, Robert H. verfasserin aut Searching for Cosmic Strings in New Observational Windows 2014transfer abstract 13 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Cosmic strings are predicted in many models beyond the Standard Model of particle physics. In such models, a network of strings will inevitably be formed in a phase transition in the early universe and will persist to the present time. Strings leave behind distinctive features in cosmology. Searching for these signatures in new observational windows provides a way to constrain particle physics at the high energy scale and is thus complementary to searches for new physics at the low energy end, for example at the LHC. Specifically, I will discuss signatures of cosmic strings in cosmic microwave background polarization maps and in 21cm redshift surveys. Cosmic strings are predicted in many models beyond the Standard Model of particle physics. In such models, a network of strings will inevitably be formed in a phase transition in the early universe and will persist to the present time. Strings leave behind distinctive features in cosmology. Searching for these signatures in new observational windows provides a way to constrain particle physics at the high energy scale and is thus complementary to searches for new physics at the low energy end, for example at the LHC. Specifically, I will discuss signatures of cosmic strings in cosmic microwave background polarization maps and in 21cm redshift surveys. Cosmic Strings Elsevier CMB Polarization Elsevier 21cm Redshift Surveys Elsevier Enthalten in Elsevier Kotzen, Benz ELSEVIER Fire safety risks of external living walls and implications for regulatory guidance in England 2023 Amsterdam (DE-627)ELV010483918 volume:246 year:2014 pages:45-57 extent:13 https://doi.org/10.1016/j.nuclphysbps.2013.10.064 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U GBV_ILN_24 GBV_ILN_110 GBV_ILN_2008 GBV_ILN_2018 50.17 Sicherheitstechnik VZ AR 246 2014 45-57 13 045F 530 |
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Cosmic strings are predicted in many models beyond the Standard Model of particle physics. In such models, a network of strings will inevitably be formed in a phase transition in the early universe and will persist to the present time. Strings leave behind distinctive features in cosmology. Searching for these signatures in new observational windows provides a way to constrain particle physics at the high energy scale and is thus complementary to searches for new physics at the low energy end, for example at the LHC. Specifically, I will discuss signatures of cosmic strings in cosmic microwave background polarization maps and in 21cm redshift surveys. |
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Cosmic strings are predicted in many models beyond the Standard Model of particle physics. In such models, a network of strings will inevitably be formed in a phase transition in the early universe and will persist to the present time. Strings leave behind distinctive features in cosmology. Searching for these signatures in new observational windows provides a way to constrain particle physics at the high energy scale and is thus complementary to searches for new physics at the low energy end, for example at the LHC. Specifically, I will discuss signatures of cosmic strings in cosmic microwave background polarization maps and in 21cm redshift surveys. |
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Cosmic strings are predicted in many models beyond the Standard Model of particle physics. In such models, a network of strings will inevitably be formed in a phase transition in the early universe and will persist to the present time. Strings leave behind distinctive features in cosmology. Searching for these signatures in new observational windows provides a way to constrain particle physics at the high energy scale and is thus complementary to searches for new physics at the low energy end, for example at the LHC. Specifically, I will discuss signatures of cosmic strings in cosmic microwave background polarization maps and in 21cm redshift surveys. |
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