The influence of chemical composition on models of Type Ia supernovae
Type Ia supernovae are bright stellar explosions distinguished by standardizable light curves that allow for their use as distance indicators for cosmological studies. Despite the highly successful use of these events in this capacity, many fundamental questions remain. Contemporary research investi...
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| Veröffentlicht in: | Frontiers of physics 2013-04, Vol.8 (2), p.168-188 |
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| creator | Calder, Alan C. Krueger, Brendan K. Jackson, Aaron P. Townsley, Dean M. |
| description | Type Ia supernovae are bright stellar explosions distinguished by standardizable light curves that allow for their use as distance indicators for cosmological studies. Despite the highly successful use of these events in this capacity, many fundamental questions remain. Contemporary research investigates how properties of the progenitor system that follow from the host galaxy such as composition and age influence the brightness of an event with the goal of better understanding and assessing the intrinsic scatter in the brightness. We provide an overview of these supernovae and proposed progenitor systems, all of which involve one or more compact stars known as white dwarfs. We describe contemporary research investigating how the composition and structure of the progenitor white dwarf systematically influences the explosion outcome assuming the progenitor is a single white dwarf that has gained mass from a companion. We present results illustrating some of these systematic effects from our research. |
| doi_str_mv | 10.1007/s11467-013-0301-4 |
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Phys</addtitle><addtitle>Frontiers of Physics in China</addtitle><description>Type Ia supernovae are bright stellar explosions distinguished by standardizable light curves that allow for their use as distance indicators for cosmological studies. Despite the highly successful use of these events in this capacity, many fundamental questions remain. Contemporary research investigates how properties of the progenitor system that follow from the host galaxy such as composition and age influence the brightness of an event with the goal of better understanding and assessing the intrinsic scatter in the brightness. We provide an overview of these supernovae and proposed progenitor systems, all of which involve one or more compact stars known as white dwarfs. We describe contemporary research investigating how the composition and structure of the progenitor white dwarf systematically influences the explosion outcome assuming the progenitor is a single white dwarf that has gained mass from a companion. We present results illustrating some of these systematic effects from our research.</description><subject>abundances</subject><subject>Astronomical models</subject><subject>Astronomy</subject><subject>Astrophysics and Cosmology</subject><subject>Atomic</subject><subject>Brightness</subject><subject>Chemical composition</subject><subject>Condensed Matter Physics</subject><subject>Explosions</subject><subject>hydrodynamics</subject><subject>Ia型超新星</subject><subject>Light curve</subject><subject>Molecular</subject><subject>nuclear reactions</subject><subject>nucleosynthesis</subject><subject>Optical and Plasma Physics</subject><subject>Particle and Nuclear Physics</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Review Article</subject><subject>stars: supernovae: general</subject><subject>stars: white dwarfs</subject><subject>Supernovae</subject><subject>White dwarf stars</subject><subject>光变曲线</subject><subject>化学成分</subject><subject>宇宙学</subject><subject>恒星爆炸</subject><subject>模型</subject><subject>白矮星</subject><subject>系统</subject><issn>2095-0462</issn><issn>2095-0470</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2013</creationdate><recordtype>article</recordtype><sourceid>BENPR</sourceid><recordid>eNp9kNFLwzAQxosoOHR_gG8Vn6u5NmmaRxlTBwNf5nNok8va0TZdsgr7783omG-DcLmD73f38UXRE5BXIIS_eQCa84RAlpCMQEJvollKBEsI5eT20ufpfTT3fkcIAeA0zLNouakxbnrTjtgrjK2JVY1do8o2VrYbrG8Oje3j8DqrsfUnxeY4YLwqYz8O6Hr7W-JjdGfK1uP8_D9EPx_LzeIrWX9_rhbv60RlAg6JDjZLU-Wp5pzrLC0ZFJprYJwKWlFuRK5RU66M4BgqNZkpGCsIF5VKK8geopdp7-DsfkR_kDs7uj6clKmAghWMAAsqmFTKWe8dGjm4pivdUQKRp8DkFJgMgclTYJIGJp0YH7T9Ft3_5mtQMUF1s63RoR4cei-Ns_2hQXcdfT57rG2_3YeTF5OUcaAERPYHl4eJtA</recordid><startdate>20130401</startdate><enddate>20130401</enddate><creator>Calder, Alan C.</creator><creator>Krueger, Brendan K.</creator><creator>Jackson, Aaron P.</creator><creator>Townsley, Dean M.</creator><general>Higher Education Press</general><general>SP Higher Education Press</general><general>Springer Nature B.V</general><scope>2RA</scope><scope>92L</scope><scope>CQIGP</scope><scope>~WA</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>3V.</scope><scope>7XB</scope><scope>88I</scope><scope>8FE</scope><scope>8FG</scope><scope>8FK</scope><scope>ABUWG</scope><scope>AEUYN</scope><scope>AFKRA</scope><scope>ARAPS</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>BHPHI</scope><scope>BKSAR</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>GNUQQ</scope><scope>HCIFZ</scope><scope>M2P</scope><scope>P5Z</scope><scope>P62</scope><scope>PCBAR</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>Q9U</scope></search><sort><creationdate>20130401</creationdate><title>The influence of chemical composition on models of Type Ia supernovae</title><author>Calder, Alan C. ; 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| subjects | abundances Astronomical models Astronomy Astrophysics and Cosmology Atomic Brightness Chemical composition Condensed Matter Physics Explosions hydrodynamics Ia型超新星 Light curve Molecular nuclear reactions nucleosynthesis Optical and Plasma Physics Particle and Nuclear Physics Physics Physics and Astronomy Review Article stars: supernovae: general stars: white dwarfs Supernovae White dwarf stars 光变曲线 化学成分 宇宙学 恒星爆炸 模型 白矮星 系统 |
| title | The influence of chemical composition on models of Type Ia supernovae |
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