The type Ia supernova SNLS-03D3bb from a super-Chandrasekhar-mass white dwarf star
Candle in the wind Type Ia supernovae are used as cosmological distance indicators. It is through them that the accelerating expansion of the Universe was detected, and with it the implied existence of dark energy. Their presumed reliability as 'standard candles' stems from the fact they h...
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| Published in | Nature Vol. 443; no. 7109; pp. 308 - 311 |
|---|---|
| Main Authors | , , , , , , , , , , , , , , , , |
| Format | Journal Article |
| Language | English |
| Published |
London
Nature Publishing Group UK
21.09.2006
Nature Publishing Group |
| Subjects | |
| Online Access | Get full text |
| ISSN | 0028-0836 1476-4687 1476-4687 1476-4679 |
| DOI | 10.1038/nature05103 |
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| Abstract | Candle in the wind
Type Ia supernovae are used as cosmological distance indicators. It is through them that the accelerating expansion of the Universe was detected, and with it the implied existence of dark energy. Their presumed reliability as 'standard candles' stems from the fact they have a fixed amount of fuel and a uniform trigger: they are predicted to explode when the mass of the white dwarf nears 1.4 solar masses, the 'Chandrasekhar' mass. Howell
et al
. now show that the high-redshift supernova SNLS-03D3bb does not play by these rules: its exceptionally high luminosity and low kinetic energy imply a super-Chandrasekhar mass progenitor. So future cosmological studies may need to consider possible contamination from such events when calculating distances.
The high-redshift supernova SNLS-03D3bb has an exceptionally high luminosity and low kinetic energy, which both imply a super-Chandrasekhar mass progenitor.
The accelerating expansion of the Universe, and the need for dark energy, were inferred from observations
1
,
2
of type Ia supernovae. There is a consensus that type Ia supernovae are thermonuclear explosions that destroy carbon–oxygen white dwarf stars that have accreted matter from a companion star
3
, although the nature of this companion remains uncertain. These supernovae are thought to be reliable distance indicators because they have a standard amount of fuel and a uniform trigger: they are predicted to explode when the mass of the white dwarf nears the Chandrasekhar mass
4
of 1.4 solar masses (
M
⊙
). Here we show that the high-redshift supernova SNLS-03D3bb has an exceptionally high luminosity and low kinetic energy that both imply a super-Chandrasekhar-mass progenitor. Super-Chandrasekhar-mass supernovae should occur preferentially in a young stellar population, so this may provide an explanation for the observed trend that overluminous type Ia supernovae occur only in ‘young’ environments
5
,
6
. As this supernova does not obey the relations that allow type Ia supernovae to be calibrated as standard candles, and as no counterparts have been found at low redshift, future cosmology studies will have to consider possible contamination from such events. |
|---|---|
| AbstractList | The accelerating expansion of the Universe, and the need for dark energy, were inferred from observations of type Ia supernovae. There is a consensus that type Ia supernovae are thermonuclear explosions that destroy carbon-oxygen white dwarf stars that have accreted matter from a companion star, although the nature of this companion remains uncertain. These supernovae are thought to be reliable distance indicators because they have a standard amount of fuel and a uniform trigger: they are predicted to explode when the mass of the white dwarf nears the Chandrasekhar mass of 1.4 solar masses (M(o)). Here we show that the high-redshift supernova SNLS-03D3bb has an exceptionally high luminosity and low kinetic energy that both imply a super-Chandrasekhar-mass progenitor. Super-Chandrasekhar-mass supernovae should occur preferentially in a young stellar population, so this may provide an explanation for the observed trend that overluminous type Ia supernovae occur only in 'young' environments. As this supernova does not obey the relations that allow type Ia supernovae to be calibrated as standard candles, and as no counterparts have been found at low redshift, future cosmology studies will have to consider possible contamination from such events. Candle in the wind Type Ia supernovae are used as cosmological distance indicators. It is through them that the accelerating expansion of the Universe was detected, and with it the implied existence of dark energy. Their presumed reliability as 'standard candles' stems from the fact they have a fixed amount of fuel and a uniform trigger: they are predicted to explode when the mass of the white dwarf nears 1.4 solar masses, the 'Chandrasekhar' mass. Howell et al . now show that the high-redshift supernova SNLS-03D3bb does not play by these rules: its exceptionally high luminosity and low kinetic energy imply a super-Chandrasekhar mass progenitor. So future cosmological studies may need to consider possible contamination from such events when calculating distances. The high-redshift supernova SNLS-03D3bb has an exceptionally high luminosity and low kinetic energy, which both imply a super-Chandrasekhar mass progenitor. The accelerating expansion of the Universe, and the need for dark energy, were inferred from observations 1 , 2 of type Ia supernovae. There is a consensus that type Ia supernovae are thermonuclear explosions that destroy carbon–oxygen white dwarf stars that have accreted matter from a companion star 3 , although the nature of this companion remains uncertain. These supernovae are thought to be reliable distance indicators because they have a standard amount of fuel and a uniform trigger: they are predicted to explode when the mass of the white dwarf nears the Chandrasekhar mass 4 of 1.4 solar masses ( M ⊙ ). Here we show that the high-redshift supernova SNLS-03D3bb has an exceptionally high luminosity and low kinetic energy that both imply a super-Chandrasekhar-mass progenitor. Super-Chandrasekhar-mass supernovae should occur preferentially in a young stellar population, so this may provide an explanation for the observed trend that overluminous type Ia supernovae occur only in ‘young’ environments 5 , 6 . As this supernova does not obey the relations that allow type Ia supernovae to be calibrated as standard candles, and as no counterparts have been found at low redshift, future cosmology studies will have to consider possible contamination from such events. The acceleration of the expansion of the universe, and the need for Dark Energy, were inferred from the observations of Type Ia supernovae (SNe Ia). There is consensus that SNe Ia are thermonuclear explosions that destroy carbon-oxygen white dwarf stars that accrete matter from a companion star, although the nature of this companion remains uncertain. SNe Ia are thought to be reliable distance indicators because they have a standard amount of fuel and a uniform trigger -- they are predicted to explode when the mass of the white dwarf nears the Chandrasekhar mass -- 1.4 solar masses. Here we show that the high redshift supernova SNLS-03D3bb has an exceptionally high luminosity and low kinetic energy that both imply a super-Chandrasekhar mass progenitor. Super-Chandrasekhar mass SNe Ia should preferentially occur in a young stellar population, so this may provide an explanation for the observed trend that overluminous SNe Ia only occur in young environments. Since this supernova does not obey the relations that allow them to be calibrated as standard candles, and since no counterparts have been found at low redshift, future cosmology studies will have to consider contamination from such events. The accelerating expansion of the Universe, and the need for dark energy, were inferred from observations super(1, ) super(2) of type Ia supernovae. There is a consensus that type Ia supernovae are thermonuclear explosions that destroy carbon-oxygen white dwarf stars that have accreted matter from a companion star super(3), although the nature of this companion remains uncertain. These supernovae are thought to be reliable distance indicators because they have a standard amount of fuel and a uniform trigger: they are predicted to explode when the mass of the white dwarf nears the Chandrasekhar mass super(4) of 1.4 solar masses (M sub([circle])). Here we show that the high-redshift supernova SNLS-03D3bb has an exceptionally high luminosity and low kinetic energy that both imply a super-Chandrasekhar-mass progenitor. Super- Chandrasekhar-mass supernovae should occur preferentially in a young stellar population, so this may provide an explanation for the observed trend that overluminous type Ia supernovae occur only in 'young' environments super(5, ) super(6). As this supernova does not obey the relations that allow type Ia supernovae to be calibrated as standard candles, and as no counterparts have been found at low redshift, future cosmology studies will have to consider possible contamination from such events. The accelerating expansion of the Universe, and the need for dark energy, were inferred from observations of type Ia supernovae. There is a consensus that type Ia supernovae are thermonuclear explosions that destroy carbon-oxygen white dwarf stars that have accreted matter from a companion star, although the nature of this companion remains uncertain. These supernovae are thought to be reliable distance indicators because they have a standard amount of fuel and a uniform trigger: they are predicted to explode when the mass of the white dwarf nears the Chandrasekhar mass of 1.4 solar masses (M(o)). Here we show that the high-redshift supernova SNLS-03D3bb has an exceptionally high luminosity and low kinetic energy that both imply a super-Chandrasekhar-mass progenitor. Super-Chandrasekhar-mass supernovae should occur preferentially in a young stellar population, so this may provide an explanation for the observed trend that overluminous type Ia supernovae occur only in 'young' environments. As this supernova does not obey the relations that allow type Ia supernovae to be calibrated as standard candles, and as no counterparts have been found at low redshift, future cosmology studies will have to consider possible contamination from such events.The accelerating expansion of the Universe, and the need for dark energy, were inferred from observations of type Ia supernovae. There is a consensus that type Ia supernovae are thermonuclear explosions that destroy carbon-oxygen white dwarf stars that have accreted matter from a companion star, although the nature of this companion remains uncertain. These supernovae are thought to be reliable distance indicators because they have a standard amount of fuel and a uniform trigger: they are predicted to explode when the mass of the white dwarf nears the Chandrasekhar mass of 1.4 solar masses (M(o)). Here we show that the high-redshift supernova SNLS-03D3bb has an exceptionally high luminosity and low kinetic energy that both imply a super-Chandrasekhar-mass progenitor. Super-Chandrasekhar-mass supernovae should occur preferentially in a young stellar population, so this may provide an explanation for the observed trend that overluminous type Ia supernovae occur only in 'young' environments. As this supernova does not obey the relations that allow type Ia supernovae to be calibrated as standard candles, and as no counterparts have been found at low redshift, future cosmology studies will have to consider possible contamination from such events. The accelerating expansion of the Universe, and the need for dark energy, were inferred from observations of type Ia supernovae. There is a consensus that type Ia supernovae are thermonuclear explosions that destroy carbon-oxygen white dwarf stars that have accreted matter from a companion star, although the nature of this companion remains uncertain. These supernovae are thought to be reliable distance indicators because they have a standard amount of fuel and a uniform trigger: they are predicted to explode when the mass of the white dwarf nears the Chandrasekhar mass of 1.4 solar masses (M[symbol omitted]). Here we show that the high-redshift supernova SNLS-03D3bb has an exceptionally high luminosity and low kinetic energy that both imply a super-Chandrasekhar-mass progenitor. Super-Chandrasekhar-mass supernovae should occur preferentially in a young stellar population, so this may provide an explanation for the observed trend that overluminous type Ia supernovae occur only in 'young' environments. As this supernova does not obey the relations that allow type Ia supernovae to be calibrated as standard candles, and as no counterparts have been found at low redshift, future cosmology studies will have to consider possible contamination from such events. [PUBLICATION ABSTRACT] The acceleration of the expansion of the universe, and the need for Dark Energy, were inferred from the observations of Type Ia supernovae (SNe Ia). There is consensus that SNe Ia are thermonuclear explosions that destroy carbon-oxygen white dwarf stars that accrete matter from a companion star, although the nature of this companion remains uncertain. SNe Ia are thought to be reliable distance indicators because they have a standard amount of fuel and a uniform trigger they are predicted to explode when the mass of the white dwarf nears the Chandrasekhar mass of 1.4 solar masses. Here we show that the high-redshift supernova SNLS-03D3bb has an exceptionally high luminosity and low kinetic energy that both imply a super-Chandrasekhar mass progenitor. Super-Chandrasekhar mass SNe Ia should preferentially occur in a young stellar population, so this may provide an explanation for the observed trend that overluminous SNe Ia only occur in young environments. Since this supernova does not obey the relations that allow them to be calibrated as standard candles, and since no counterparts have been found at low redshift, future cosmology studies will have to consider contamination from such events. |
| Audience | Academic |
| Author | Fouchez, Dominique Hook, Isobel M. Sullivan, Mark Ellis, Richard S. Basa, Stephane Hsiao, Eric Y. Neill, James D. Guy, Julien Andrew Howell, D. Nugent, Peter E. Balam, David Conley, Alexander J. Perrett, Kathryn M. Le Borgne, Damien Pritchet, Christopher J. Carlberg, Raymond G. Pain, Reynald |
| Author_xml | – sequence: 1 givenname: D. surname: Andrew Howell fullname: Andrew Howell, D. email: howell@astro.utoronto.ca organization: Department of Astronomy and Astrophysics, University of Toronto – sequence: 2 givenname: Mark surname: Sullivan fullname: Sullivan, Mark organization: Department of Astronomy and Astrophysics, University of Toronto – sequence: 3 givenname: Peter E. surname: Nugent fullname: Nugent, Peter E. organization: Lawrence Berkeley National Laboratory – sequence: 4 givenname: Richard S. surname: Ellis fullname: Ellis, Richard S. organization: California Institute of Technology – sequence: 5 givenname: Alexander J. surname: Conley fullname: Conley, Alexander J. organization: Department of Astronomy and Astrophysics, University of Toronto – sequence: 6 givenname: Damien surname: Le Borgne fullname: Le Borgne, Damien organization: DAPNIA/Service d'Astrophysique, CEA/Saclay – sequence: 7 givenname: Raymond G. surname: Carlberg fullname: Carlberg, Raymond G. organization: Department of Astronomy and Astrophysics, University of Toronto – sequence: 8 givenname: Julien surname: Guy fullname: Guy, Julien organization: LPNHE, CNRS-IN2P3 and University of Paris VI and VII – sequence: 9 givenname: David surname: Balam fullname: Balam, David organization: Department of Physics and Astronomy, University of Victoria – sequence: 10 givenname: Stephane surname: Basa fullname: Basa, Stephane organization: LAM CNRS, BP8, Traverse du Siphon – sequence: 11 givenname: Dominique surname: Fouchez fullname: Fouchez, Dominique organization: CPPM, CNRS-IN2P3 and University Aix Marseille II, Case 907 – sequence: 12 givenname: Isobel M. surname: Hook fullname: Hook, Isobel M. organization: University of Oxford Astrophysics, Denys Wilkinson Building – sequence: 13 givenname: Eric Y. surname: Hsiao fullname: Hsiao, Eric Y. organization: Department of Physics and Astronomy, University of Victoria – sequence: 14 givenname: James D. surname: Neill fullname: Neill, James D. organization: Department of Physics and Astronomy, University of Victoria – sequence: 15 givenname: Reynald surname: Pain fullname: Pain, Reynald organization: LPNHE, CNRS-IN2P3 and University of Paris VI and VII – sequence: 16 givenname: Kathryn M. surname: Perrett fullname: Perrett, Kathryn M. organization: Department of Astronomy and Astrophysics, University of Toronto – sequence: 17 givenname: Christopher J. surname: Pritchet fullname: Pritchet, Christopher J. organization: Department of Physics and Astronomy, University of Victoria |
| BackLink | https://www.ncbi.nlm.nih.gov/pubmed/16988705$$D View this record in MEDLINE/PubMed https://in2p3.hal.science/in2p3-00103975$$DView record in HAL https://www.osti.gov/servlets/purl/927329$$D View this record in Osti.gov |
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| Copyright | Springer Nature Limited 2006 COPYRIGHT 2006 Nature Publishing Group Copyright Nature Publishing Group Sep 21, 2006 Distributed under a Creative Commons Attribution 4.0 International License |
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| Snippet | Candle in the wind
Type Ia supernovae are used as cosmological distance indicators. It is through them that the accelerating expansion of the Universe was... The accelerating expansion of the Universe, and the need for dark energy, were inferred from observations of type Ia supernovae. There is a consensus that type... The accelerating expansion of the Universe, and the need for dark energy, were inferred from observations super(1, ) super(2) of type Ia supernovae. There is a... The acceleration of the expansion of the universe, and the need for Dark Energy, were inferred from the observations of Type Ia supernovae (SNe Ia). There is... |
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| SubjectTerms | ACCELERATION Astronomy Astrophysics CONTAMINATION COSMOLOGY Cosmology and Extra-Galactic Astrophysics Explosions Humanities and Social Sciences Indicators KINETIC ENERGY letter LUMINOSITY multidisciplinary NUCLEAR PHYSICS AND RADIATION PHYSICS Physics PHYSICS OF ELEMENTARY PARTICLES AND FIELDS Red shift Science Science (multidisciplinary) Sciences of the Universe Stars supernova type Ia thermonuclear super-chandrasekhar SUPERNOVAE Supernovas THERMONUCLEAR EXPLOSIONS UNIVERSE WHITE DWARF STARS |
| Title | The type Ia supernova SNLS-03D3bb from a super-Chandrasekhar-mass white dwarf star |
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