Studies of the Core Conditions of the Earth and Super-Earths Using Intense Ion Beams at FAIR
Using detailed numerical simulations, we present the design of an experiment that will generate samples of iron under extreme conditions of density and pressure believed to exist in the interior of the Earth and interior of extrasolar Earth-like planets. In the proposed experiment design, an intense...
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description | Using detailed numerical simulations, we present the design of an experiment that will generate samples of iron under extreme conditions of density and pressure believed to exist in the interior of the Earth and interior of extrasolar Earth-like planets. In the proposed experiment design, an intense uranium beam is used to implode a multilayered cylindrical target that consists of a thin Fe cylinder enclosed in a thick massive W shell. Such intense uranium beams will be available at the heavy-ion synchrotron, SIS100, at the Facility for Antiprotons and Ion Research (FAIR), at Darmstadt, which is under construction and will become operational in the next few years. It is expected that the beam intensity will increase gradually over a couple of years to its maximum design value. Therefore, in our studies, we have considered a wide range of beam parameters, from the initial beam intensity ("Day One") to the maximum specified value. It is also worth noting that two different focal spot geometries have been used. In one case, a circular focal spot with a Gaussian transverse intensity distribution is considered, whereas in the other case, an annular focal spot is used. With these two beam geometries, one can access different parts of the Fe phase diagram. For example, heating the sample with a circular focal spot generates a hot liquid state, while an annular focal spot can produce a highly compressed liquid or a highly compressed solid phase depending on the beam intensity. |
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A. ; Lomonosov, I. V. ; Borm, B. ; Piriz, A. R. ; Shutov, A. ; Neumayer, P. ; Bagnoud, V. ; Piriz, S. A.</creator><creatorcontrib>Tahir, N. A. ; Lomonosov, I. V. ; Borm, B. ; Piriz, A. R. ; Shutov, A. ; Neumayer, P. ; Bagnoud, V. ; Piriz, S. A.</creatorcontrib><description>Using detailed numerical simulations, we present the design of an experiment that will generate samples of iron under extreme conditions of density and pressure believed to exist in the interior of the Earth and interior of extrasolar Earth-like planets. In the proposed experiment design, an intense uranium beam is used to implode a multilayered cylindrical target that consists of a thin Fe cylinder enclosed in a thick massive W shell. Such intense uranium beams will be available at the heavy-ion synchrotron, SIS100, at the Facility for Antiprotons and Ion Research (FAIR), at Darmstadt, which is under construction and will become operational in the next few years. It is expected that the beam intensity will increase gradually over a couple of years to its maximum design value. Therefore, in our studies, we have considered a wide range of beam parameters, from the initial beam intensity ("Day One") to the maximum specified value. It is also worth noting that two different focal spot geometries have been used. In one case, a circular focal spot with a Gaussian transverse intensity distribution is considered, whereas in the other case, an annular focal spot is used. With these two beam geometries, one can access different parts of the Fe phase diagram. For example, heating the sample with a circular focal spot generates a hot liquid state, while an annular focal spot can produce a highly compressed liquid or a highly compressed solid phase depending on the beam intensity.</description><identifier>ISSN: 0067-0049</identifier><identifier>EISSN: 1538-4365</identifier><identifier>DOI: 10.3847/1538-4365/aa813e</identifier><language>eng</language><publisher>Saskatoon: The American Astronomical Society</publisher><subject>Antiparticles ; ANTIPROTONS ; ASTROPHYSICS, COSMOLOGY AND ASTRONOMY ; Computer simulation ; COMPUTERIZED SIMULATION ; CONDENSED MATTER PHYSICS, SUPERCONDUCTIVITY AND SUPERFLUIDITY ; Cylinders ; dense matter ; Design ; Design of experiments ; Earth ; equation of state ; EQUATIONS OF STATE ; EXPERIMENT DESIGN ; EXPERIMENT PLANNING ; Extrasolar planets ; Gaussian distribution ; HEATING ; HEAVY IONS ; ION BEAMS ; IRON ; LAYERS ; LIQUIDS ; Nondestructive testing ; Numerical simulations ; PHASE DIAGRAMS ; PLANETS ; PLASMA ; plasmas ; SIS SYNCHROTRON ; Solid phases ; SOLIDS ; Stellar planets ; Terrestrial planets ; URANIUM</subject><ispartof>The Astrophysical journal. 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A.</creatorcontrib><creatorcontrib>Lomonosov, I. V.</creatorcontrib><creatorcontrib>Borm, B.</creatorcontrib><creatorcontrib>Piriz, A. R.</creatorcontrib><creatorcontrib>Shutov, A.</creatorcontrib><creatorcontrib>Neumayer, P.</creatorcontrib><creatorcontrib>Bagnoud, V.</creatorcontrib><creatorcontrib>Piriz, S. A.</creatorcontrib><title>Studies of the Core Conditions of the Earth and Super-Earths Using Intense Ion Beams at FAIR</title><title>The Astrophysical journal. Supplement series</title><addtitle>APJS</addtitle><addtitle>Astrophys. J. Suppl</addtitle><description>Using detailed numerical simulations, we present the design of an experiment that will generate samples of iron under extreme conditions of density and pressure believed to exist in the interior of the Earth and interior of extrasolar Earth-like planets. In the proposed experiment design, an intense uranium beam is used to implode a multilayered cylindrical target that consists of a thin Fe cylinder enclosed in a thick massive W shell. Such intense uranium beams will be available at the heavy-ion synchrotron, SIS100, at the Facility for Antiprotons and Ion Research (FAIR), at Darmstadt, which is under construction and will become operational in the next few years. It is expected that the beam intensity will increase gradually over a couple of years to its maximum design value. Therefore, in our studies, we have considered a wide range of beam parameters, from the initial beam intensity ("Day One") to the maximum specified value. It is also worth noting that two different focal spot geometries have been used. In one case, a circular focal spot with a Gaussian transverse intensity distribution is considered, whereas in the other case, an annular focal spot is used. With these two beam geometries, one can access different parts of the Fe phase diagram. For example, heating the sample with a circular focal spot generates a hot liquid state, while an annular focal spot can produce a highly compressed liquid or a highly compressed solid phase depending on the beam intensity.</description><subject>Antiparticles</subject><subject>ANTIPROTONS</subject><subject>ASTROPHYSICS, COSMOLOGY AND ASTRONOMY</subject><subject>Computer simulation</subject><subject>COMPUTERIZED SIMULATION</subject><subject>CONDENSED MATTER PHYSICS, SUPERCONDUCTIVITY AND SUPERFLUIDITY</subject><subject>Cylinders</subject><subject>dense matter</subject><subject>Design</subject><subject>Design of experiments</subject><subject>Earth</subject><subject>equation of state</subject><subject>EQUATIONS OF STATE</subject><subject>EXPERIMENT DESIGN</subject><subject>EXPERIMENT PLANNING</subject><subject>Extrasolar planets</subject><subject>Gaussian distribution</subject><subject>HEATING</subject><subject>HEAVY IONS</subject><subject>ION BEAMS</subject><subject>IRON</subject><subject>LAYERS</subject><subject>LIQUIDS</subject><subject>Nondestructive testing</subject><subject>Numerical simulations</subject><subject>PHASE DIAGRAMS</subject><subject>PLANETS</subject><subject>PLASMA</subject><subject>plasmas</subject><subject>SIS SYNCHROTRON</subject><subject>Solid phases</subject><subject>SOLIDS</subject><subject>Stellar planets</subject><subject>Terrestrial planets</subject><subject>URANIUM</subject><issn>0067-0049</issn><issn>1538-4365</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2017</creationdate><recordtype>article</recordtype><recordid>eNp9kE1LxDAQhoMouH7cPQb0aDVp0iQ96uLqgiC47k0IaTJ1u2hSk-zBf2_ril5EBuaL5x2GF6ETSi6Y4vKSVkwVnInq0hhFGeygyc9qF00IEbIghNf76CClNSFEVqyeoOdF3rgOEg4tzivA0xDH5F2Xu-B_1jcm5hU23uHFpodYfM0JL1PnX_DcZ_AJ8Dx4fA3mLWGT8exq_niE9lrzmuD4ux6i5ezmaXpX3D_czqdX94XlROZCQcOccMrWrrQNbQx1vBWOla2ypASwDeOS8UbyoVNSWsGpqpTjHGwrgLNDdLq9G1LudLJdBruywXuwWZelEJTU9S_Vx_C-gZT1OmyiHx7TJaukoCUnZKDIlrIxpBSh1X3s3kz80JTo0Wk92qpHW_XW6UFyvpV0of-9-Q9-9gdu-vX4R6npEL1r2SfFTIoq</recordid><startdate>20170901</startdate><enddate>20170901</enddate><creator>Tahir, N. A.</creator><creator>Lomonosov, I. V.</creator><creator>Borm, B.</creator><creator>Piriz, A. R.</creator><creator>Shutov, A.</creator><creator>Neumayer, P.</creator><creator>Bagnoud, V.</creator><creator>Piriz, S. A.</creator><general>The American Astronomical Society</general><general>IOP Publishing</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>8FD</scope><scope>H8D</scope><scope>KL.</scope><scope>L7M</scope><scope>OTOTI</scope></search><sort><creationdate>20170901</creationdate><title>Studies of the Core Conditions of the Earth and Super-Earths Using Intense Ion Beams at FAIR</title><author>Tahir, N. A. ; Lomonosov, I. V. ; Borm, B. ; Piriz, A. R. ; Shutov, A. ; Neumayer, P. ; Bagnoud, V. ; Piriz, S. 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A.</creatorcontrib><creatorcontrib>Lomonosov, I. V.</creatorcontrib><creatorcontrib>Borm, B.</creatorcontrib><creatorcontrib>Piriz, A. R.</creatorcontrib><creatorcontrib>Shutov, A.</creatorcontrib><creatorcontrib>Neumayer, P.</creatorcontrib><creatorcontrib>Bagnoud, V.</creatorcontrib><creatorcontrib>Piriz, S. A.</creatorcontrib><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>OSTI.GOV</collection><jtitle>The Astrophysical journal. Supplement series</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Tahir, N. A.</au><au>Lomonosov, I. V.</au><au>Borm, B.</au><au>Piriz, A. R.</au><au>Shutov, A.</au><au>Neumayer, P.</au><au>Bagnoud, V.</au><au>Piriz, S. A.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Studies of the Core Conditions of the Earth and Super-Earths Using Intense Ion Beams at FAIR</atitle><jtitle>The Astrophysical journal. Supplement series</jtitle><stitle>APJS</stitle><addtitle>Astrophys. J. Suppl</addtitle><date>2017-09-01</date><risdate>2017</risdate><volume>232</volume><issue>1</issue><spage>1</spage><pages>1-</pages><issn>0067-0049</issn><eissn>1538-4365</eissn><abstract>Using detailed numerical simulations, we present the design of an experiment that will generate samples of iron under extreme conditions of density and pressure believed to exist in the interior of the Earth and interior of extrasolar Earth-like planets. In the proposed experiment design, an intense uranium beam is used to implode a multilayered cylindrical target that consists of a thin Fe cylinder enclosed in a thick massive W shell. Such intense uranium beams will be available at the heavy-ion synchrotron, SIS100, at the Facility for Antiprotons and Ion Research (FAIR), at Darmstadt, which is under construction and will become operational in the next few years. It is expected that the beam intensity will increase gradually over a couple of years to its maximum design value. Therefore, in our studies, we have considered a wide range of beam parameters, from the initial beam intensity ("Day One") to the maximum specified value. It is also worth noting that two different focal spot geometries have been used. In one case, a circular focal spot with a Gaussian transverse intensity distribution is considered, whereas in the other case, an annular focal spot is used. With these two beam geometries, one can access different parts of the Fe phase diagram. For example, heating the sample with a circular focal spot generates a hot liquid state, while an annular focal spot can produce a highly compressed liquid or a highly compressed solid phase depending on the beam intensity.</abstract><cop>Saskatoon</cop><pub>The American Astronomical Society</pub><doi>10.3847/1538-4365/aa813e</doi><tpages>15</tpages><oa>free_for_read</oa></addata></record> |
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subjects | Antiparticles ANTIPROTONS ASTROPHYSICS, COSMOLOGY AND ASTRONOMY Computer simulation COMPUTERIZED SIMULATION CONDENSED MATTER PHYSICS, SUPERCONDUCTIVITY AND SUPERFLUIDITY Cylinders dense matter Design Design of experiments Earth equation of state EQUATIONS OF STATE EXPERIMENT DESIGN EXPERIMENT PLANNING Extrasolar planets Gaussian distribution HEATING HEAVY IONS ION BEAMS IRON LAYERS LIQUIDS Nondestructive testing Numerical simulations PHASE DIAGRAMS PLANETS PLASMA plasmas SIS SYNCHROTRON Solid phases SOLIDS Stellar planets Terrestrial planets URANIUM |
title | Studies of the Core Conditions of the Earth and Super-Earths Using Intense Ion Beams at FAIR |
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