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| Fältnamn | Indikatorer | Metadata |
|---|---|---|
| 000 | 02875naa a2200337 4500 | |
| 001 | oai:DiVA.org:liu-47631 | |
| 003 | SwePub | |
| 008 | 091011s2000 | |||||||||||000 ||eng| | |
| 024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:liu:diva-476312 URI |
| 024 | 7 | a https://doi.org/10.1126/science.288.5473.20182 DOI |
| 040 | a (SwePub)liu | |
| 041 | a engb eng | |
| 042 | 9 SwePub | |
| 072 | 7 | a ref2 swepub-contenttype |
| 072 | 7 | a art2 swepub-publicationtype |
| 100 | 1 | a Baughman, R.H.u Honeywell International, Honeywell Technology Center, Morristown, NJ 07962-1021, United States4 aut |
| 245 | 1 0 | a Negative Poisson's ratios for extreme states of matter |
| 264 | 1 | b American Association for the Advancement of Science (AAAS),c 2000 |
| 338 | a print2 rdacarrier | |
| 520 | a Negative Poisson's ratios are predicted for body-centered-cubic phases that likely exist in white dwarf cores and neutron star outer crusts, as well as those found for vacuumlike ion crystals, plasma dust crystals, and colloidal crystals (including certain virus crystals). The existence of this counterintuitive property, which means that a material laterally expands when stretched, is experimentally demonstrated for very low density crystals of trapped ions. At very high densities, the large predicted negative and positive Poisson's ratios might be important for understanding the asteroseismology of neutron stars and white dwarfs and the effect of stellar stresses on nuclear reaction rates. Giant Poisson's ratios are both predicted and observed for highly strained coulombic photonic crystals, suggesting possible applications of large, tunable Poisson's ratios for photonic crystal devices. | |
| 653 | a TECHNOLOGY | |
| 653 | a TEKNIKVETENSKAP | |
| 700 | 1 | a Dantas, S.O.u Departamento de Física, Universidade Federal de Juiz de Fora, Juiz de Fora, 36036-330, Mina Gerais, Brazil4 aut |
| 700 | 1 | a Stafström, Svenu Linköpings universitet,Tekniska högskolan,Beräkningsfysik4 aut0 (Swepub:liu)svest87 |
| 700 | 1 | a Zakhidov, A.A.u Honeywell International, Honeywell Technology Center, Morristown, NJ 07962-1021, United States4 aut |
| 700 | 1 | a Mitchell, T.B.u Natl. Inst. of Std. and Technology, Boulder, CO 80303, United States4 aut |
| 700 | 1 | a Dubin, D.H.E.u Department of Physics, Univ. of California at San Diego, San Diego, CA 92093, United States4 aut |
| 710 | 2 | a Honeywell International, Honeywell Technology Center, Morristown, NJ 07962-1021, United Statesb Departamento de Física, Universidade Federal de Juiz de Fora, Juiz de Fora, 36036-330, Mina Gerais, Brazil4 org |
| 773 | 0 | t Scienced : American Association for the Advancement of Science (AAAS)g 288:5473, s. 2018-2022q 288:5473<2018-2022x 0036-8075x 1095-9203 |
| 856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:liu:diva-47631 |
| 856 | 4 8 | u https://doi.org/10.1126/science.288.5473.2018 |
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- Baughman, R.H.
- Dantas, S.O.
- Stafström, Sven
- Zakhidov, A.A.
- Mitchell, T.B.
- Dubin, D.H.E.
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