Problematic aspects of Kaluza–Klein excitations in multidimensional models with Einstein internal spaces
We consider Kaluza–Klein (KK) models where internal spaces are compact Einstein spaces. These spaces are stabilized by background matter (e.g., monopole form-fields). We perturb this background by a compact matter source (e.g., the system of gravitating masses) with the zero pressure in the external...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Chopovsky, Alexey [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2014transfer abstract |
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| Schlagwörter: |
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| Umfang: |
4 |
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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 |
|---|---|
| Übergeordnetes Werk: |
volume:736 ; year:2014 ; day:7 ; month:09 ; pages:329-332 ; extent:4 |
| Links: |
|---|
| DOI / URN: |
10.1016/j.physletb.2014.07.042 |
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ELV012365181 |
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| 520 | |a We consider Kaluza–Klein (KK) models where internal spaces are compact Einstein spaces. These spaces are stabilized by background matter (e.g., monopole form-fields). We perturb this background by a compact matter source (e.g., the system of gravitating masses) with the zero pressure in the external/our space and an arbitrary pressure in the internal space. We show that the Einstein equations are compatible only if the matter source is smeared over the internal space and perturbed metric components do not depend on coordinates of extra dimensions. The latter means the absence of KK modes corresponding to the metric fluctuations. Maybe, the absence of KK particles in LHC experiments is explained by such mechanism. | ||
| 520 | |a We consider Kaluza–Klein (KK) models where internal spaces are compact Einstein spaces. These spaces are stabilized by background matter (e.g., monopole form-fields). We perturb this background by a compact matter source (e.g., the system of gravitating masses) with the zero pressure in the external/our space and an arbitrary pressure in the internal space. We show that the Einstein equations are compatible only if the matter source is smeared over the internal space and perturbed metric components do not depend on coordinates of extra dimensions. The latter means the absence of KK modes corresponding to the metric fluctuations. Maybe, the absence of KK particles in LHC experiments is explained by such mechanism. | ||
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10.1016/j.physletb.2014.07.042 doi GBVA2014012000011.pica (DE-627)ELV012365181 (ELSEVIER)S0370-2693(14)00544-9 DE-627 ger DE-627 rakwb eng 530 DE-600 610 VZ 77.50 bkl Chopovsky, Alexey verfasserin aut Problematic aspects of Kaluza–Klein excitations in multidimensional models with Einstein internal spaces 2014transfer abstract 4 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier We consider Kaluza–Klein (KK) models where internal spaces are compact Einstein spaces. These spaces are stabilized by background matter (e.g., monopole form-fields). We perturb this background by a compact matter source (e.g., the system of gravitating masses) with the zero pressure in the external/our space and an arbitrary pressure in the internal space. We show that the Einstein equations are compatible only if the matter source is smeared over the internal space and perturbed metric components do not depend on coordinates of extra dimensions. The latter means the absence of KK modes corresponding to the metric fluctuations. Maybe, the absence of KK particles in LHC experiments is explained by such mechanism. We consider Kaluza–Klein (KK) models where internal spaces are compact Einstein spaces. These spaces are stabilized by background matter (e.g., monopole form-fields). We perturb this background by a compact matter source (e.g., the system of gravitating masses) with the zero pressure in the external/our space and an arbitrary pressure in the internal space. We show that the Einstein equations are compatible only if the matter source is smeared over the internal space and perturbed metric components do not depend on coordinates of extra dimensions. The latter means the absence of KK modes corresponding to the metric fluctuations. Maybe, the absence of KK particles in LHC experiments is explained by such mechanism. Kaluza–Klein models Elsevier Einstein spaces Elsevier Kaluza–Klein excitations/modes Elsevier Gravitational tests Elsevier Multidimensional models Elsevier Black strings/branes Elsevier Eingorn, Maxim oth Zhuk, Alexander 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:736 year:2014 day:7 month:09 pages:329-332 extent:4 https://doi.org/10.1016/j.physletb.2014.07.042 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA 77.50 Psychophysiologie VZ AR 736 2014 7 0907 329-332 4 |
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10.1016/j.physletb.2014.07.042 doi GBVA2014012000011.pica (DE-627)ELV012365181 (ELSEVIER)S0370-2693(14)00544-9 DE-627 ger DE-627 rakwb eng 530 DE-600 610 VZ 77.50 bkl Chopovsky, Alexey verfasserin aut Problematic aspects of Kaluza–Klein excitations in multidimensional models with Einstein internal spaces 2014transfer abstract 4 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier We consider Kaluza–Klein (KK) models where internal spaces are compact Einstein spaces. These spaces are stabilized by background matter (e.g., monopole form-fields). We perturb this background by a compact matter source (e.g., the system of gravitating masses) with the zero pressure in the external/our space and an arbitrary pressure in the internal space. We show that the Einstein equations are compatible only if the matter source is smeared over the internal space and perturbed metric components do not depend on coordinates of extra dimensions. The latter means the absence of KK modes corresponding to the metric fluctuations. Maybe, the absence of KK particles in LHC experiments is explained by such mechanism. We consider Kaluza–Klein (KK) models where internal spaces are compact Einstein spaces. These spaces are stabilized by background matter (e.g., monopole form-fields). We perturb this background by a compact matter source (e.g., the system of gravitating masses) with the zero pressure in the external/our space and an arbitrary pressure in the internal space. We show that the Einstein equations are compatible only if the matter source is smeared over the internal space and perturbed metric components do not depend on coordinates of extra dimensions. The latter means the absence of KK modes corresponding to the metric fluctuations. Maybe, the absence of KK particles in LHC experiments is explained by such mechanism. Kaluza–Klein models Elsevier Einstein spaces Elsevier Kaluza–Klein excitations/modes Elsevier Gravitational tests Elsevier Multidimensional models Elsevier Black strings/branes Elsevier Eingorn, Maxim oth Zhuk, Alexander 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:736 year:2014 day:7 month:09 pages:329-332 extent:4 https://doi.org/10.1016/j.physletb.2014.07.042 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA 77.50 Psychophysiologie VZ AR 736 2014 7 0907 329-332 4 |
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10.1016/j.physletb.2014.07.042 doi GBVA2014012000011.pica (DE-627)ELV012365181 (ELSEVIER)S0370-2693(14)00544-9 DE-627 ger DE-627 rakwb eng 530 DE-600 610 VZ 77.50 bkl Chopovsky, Alexey verfasserin aut Problematic aspects of Kaluza–Klein excitations in multidimensional models with Einstein internal spaces 2014transfer abstract 4 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier We consider Kaluza–Klein (KK) models where internal spaces are compact Einstein spaces. These spaces are stabilized by background matter (e.g., monopole form-fields). We perturb this background by a compact matter source (e.g., the system of gravitating masses) with the zero pressure in the external/our space and an arbitrary pressure in the internal space. We show that the Einstein equations are compatible only if the matter source is smeared over the internal space and perturbed metric components do not depend on coordinates of extra dimensions. The latter means the absence of KK modes corresponding to the metric fluctuations. Maybe, the absence of KK particles in LHC experiments is explained by such mechanism. We consider Kaluza–Klein (KK) models where internal spaces are compact Einstein spaces. These spaces are stabilized by background matter (e.g., monopole form-fields). We perturb this background by a compact matter source (e.g., the system of gravitating masses) with the zero pressure in the external/our space and an arbitrary pressure in the internal space. We show that the Einstein equations are compatible only if the matter source is smeared over the internal space and perturbed metric components do not depend on coordinates of extra dimensions. The latter means the absence of KK modes corresponding to the metric fluctuations. Maybe, the absence of KK particles in LHC experiments is explained by such mechanism. Kaluza–Klein models Elsevier Einstein spaces Elsevier Kaluza–Klein excitations/modes Elsevier Gravitational tests Elsevier Multidimensional models Elsevier Black strings/branes Elsevier Eingorn, Maxim oth Zhuk, Alexander 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:736 year:2014 day:7 month:09 pages:329-332 extent:4 https://doi.org/10.1016/j.physletb.2014.07.042 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA 77.50 Psychophysiologie VZ AR 736 2014 7 0907 329-332 4 |
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10.1016/j.physletb.2014.07.042 doi GBVA2014012000011.pica (DE-627)ELV012365181 (ELSEVIER)S0370-2693(14)00544-9 DE-627 ger DE-627 rakwb eng 530 DE-600 610 VZ 77.50 bkl Chopovsky, Alexey verfasserin aut Problematic aspects of Kaluza–Klein excitations in multidimensional models with Einstein internal spaces 2014transfer abstract 4 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier We consider Kaluza–Klein (KK) models where internal spaces are compact Einstein spaces. These spaces are stabilized by background matter (e.g., monopole form-fields). We perturb this background by a compact matter source (e.g., the system of gravitating masses) with the zero pressure in the external/our space and an arbitrary pressure in the internal space. We show that the Einstein equations are compatible only if the matter source is smeared over the internal space and perturbed metric components do not depend on coordinates of extra dimensions. The latter means the absence of KK modes corresponding to the metric fluctuations. Maybe, the absence of KK particles in LHC experiments is explained by such mechanism. We consider Kaluza–Klein (KK) models where internal spaces are compact Einstein spaces. These spaces are stabilized by background matter (e.g., monopole form-fields). We perturb this background by a compact matter source (e.g., the system of gravitating masses) with the zero pressure in the external/our space and an arbitrary pressure in the internal space. We show that the Einstein equations are compatible only if the matter source is smeared over the internal space and perturbed metric components do not depend on coordinates of extra dimensions. The latter means the absence of KK modes corresponding to the metric fluctuations. Maybe, the absence of KK particles in LHC experiments is explained by such mechanism. Kaluza–Klein models Elsevier Einstein spaces Elsevier Kaluza–Klein excitations/modes Elsevier Gravitational tests Elsevier Multidimensional models Elsevier Black strings/branes Elsevier Eingorn, Maxim oth Zhuk, Alexander 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:736 year:2014 day:7 month:09 pages:329-332 extent:4 https://doi.org/10.1016/j.physletb.2014.07.042 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA 77.50 Psychophysiologie VZ AR 736 2014 7 0907 329-332 4 |
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10.1016/j.physletb.2014.07.042 doi GBVA2014012000011.pica (DE-627)ELV012365181 (ELSEVIER)S0370-2693(14)00544-9 DE-627 ger DE-627 rakwb eng 530 DE-600 610 VZ 77.50 bkl Chopovsky, Alexey verfasserin aut Problematic aspects of Kaluza–Klein excitations in multidimensional models with Einstein internal spaces 2014transfer abstract 4 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier We consider Kaluza–Klein (KK) models where internal spaces are compact Einstein spaces. These spaces are stabilized by background matter (e.g., monopole form-fields). We perturb this background by a compact matter source (e.g., the system of gravitating masses) with the zero pressure in the external/our space and an arbitrary pressure in the internal space. We show that the Einstein equations are compatible only if the matter source is smeared over the internal space and perturbed metric components do not depend on coordinates of extra dimensions. The latter means the absence of KK modes corresponding to the metric fluctuations. Maybe, the absence of KK particles in LHC experiments is explained by such mechanism. We consider Kaluza–Klein (KK) models where internal spaces are compact Einstein spaces. These spaces are stabilized by background matter (e.g., monopole form-fields). We perturb this background by a compact matter source (e.g., the system of gravitating masses) with the zero pressure in the external/our space and an arbitrary pressure in the internal space. We show that the Einstein equations are compatible only if the matter source is smeared over the internal space and perturbed metric components do not depend on coordinates of extra dimensions. The latter means the absence of KK modes corresponding to the metric fluctuations. Maybe, the absence of KK particles in LHC experiments is explained by such mechanism. Kaluza–Klein models Elsevier Einstein spaces Elsevier Kaluza–Klein excitations/modes Elsevier Gravitational tests Elsevier Multidimensional models Elsevier Black strings/branes Elsevier Eingorn, Maxim oth Zhuk, Alexander 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:736 year:2014 day:7 month:09 pages:329-332 extent:4 https://doi.org/10.1016/j.physletb.2014.07.042 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA 77.50 Psychophysiologie VZ AR 736 2014 7 0907 329-332 4 |
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Problematic aspects of Kaluza–Klein excitations in multidimensional models with Einstein internal spaces |
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Problematic aspects of Kaluza–Klein excitations in multidimensional models with Einstein internal spaces |
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Chopovsky, Alexey |
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Applying the Go/NoGo processing schema to a visual oddball task in older adults |
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Applying the Go/NoGo processing schema to a visual oddball task in older adults |
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2014 |
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Chopovsky, Alexey |
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Elektronische Aufsätze |
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Chopovsky, Alexey |
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10.1016/j.physletb.2014.07.042 |
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530 610 |
| title_sort |
problematic aspects of kaluza–klein excitations in multidimensional models with einstein internal spaces |
| title_auth |
Problematic aspects of Kaluza–Klein excitations in multidimensional models with Einstein internal spaces |
| abstract |
We consider Kaluza–Klein (KK) models where internal spaces are compact Einstein spaces. These spaces are stabilized by background matter (e.g., monopole form-fields). We perturb this background by a compact matter source (e.g., the system of gravitating masses) with the zero pressure in the external/our space and an arbitrary pressure in the internal space. We show that the Einstein equations are compatible only if the matter source is smeared over the internal space and perturbed metric components do not depend on coordinates of extra dimensions. The latter means the absence of KK modes corresponding to the metric fluctuations. Maybe, the absence of KK particles in LHC experiments is explained by such mechanism. |
| abstractGer |
We consider Kaluza–Klein (KK) models where internal spaces are compact Einstein spaces. These spaces are stabilized by background matter (e.g., monopole form-fields). We perturb this background by a compact matter source (e.g., the system of gravitating masses) with the zero pressure in the external/our space and an arbitrary pressure in the internal space. We show that the Einstein equations are compatible only if the matter source is smeared over the internal space and perturbed metric components do not depend on coordinates of extra dimensions. The latter means the absence of KK modes corresponding to the metric fluctuations. Maybe, the absence of KK particles in LHC experiments is explained by such mechanism. |
| abstract_unstemmed |
We consider Kaluza–Klein (KK) models where internal spaces are compact Einstein spaces. These spaces are stabilized by background matter (e.g., monopole form-fields). We perturb this background by a compact matter source (e.g., the system of gravitating masses) with the zero pressure in the external/our space and an arbitrary pressure in the internal space. We show that the Einstein equations are compatible only if the matter source is smeared over the internal space and perturbed metric components do not depend on coordinates of extra dimensions. The latter means the absence of KK modes corresponding to the metric fluctuations. Maybe, the absence of KK particles in LHC experiments is explained by such mechanism. |
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GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA |
| title_short |
Problematic aspects of Kaluza–Klein excitations in multidimensional models with Einstein internal spaces |
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https://doi.org/10.1016/j.physletb.2014.07.042 |
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Eingorn, Maxim Zhuk, Alexander |
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Eingorn, Maxim Zhuk, Alexander |
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10.1016/j.physletb.2014.07.042 |
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