Changeset 8037f4b in sasview
- Timestamp:
- Jul 31, 2012 3:26:25 PM (12 years ago)
- Branches:
- master, ESS_GUI, ESS_GUI_Docs, ESS_GUI_batch_fitting, ESS_GUI_bumps_abstraction, ESS_GUI_iss1116, ESS_GUI_iss879, ESS_GUI_iss959, ESS_GUI_opencl, ESS_GUI_ordering, ESS_GUI_sync_sascalc, costrafo411, magnetic_scatt, release-4.1.1, release-4.1.2, release-4.2.2, release_4.0.1, ticket-1009, ticket-1094-headless, ticket-1242-2d-resolution, ticket-1243, ticket-1249, ticket885, unittest-saveload
- Children:
- 1d3a2e7
- Parents:
- fa3f081
- File:
-
- 1 edited
Legend:
- Unmodified
- Added
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sansmodels/src/sans/models/media/model_functions.html
r082c565 r8037f4b 8218 8218 <p ><b><span style="font-size: 14pt;"></span></b><b><span style="font-size: 14pt;"></span></b> </p> 8219 8219 <p ></p> 8220 <p style="margin-left: 0.55in; text-indent: -0.3in;"><b><span style="font-size: 14pt;">3.10.</span></b>8221 <b>8222 <span style="font-size: 7pt;"> 8223 </span>8224 </b>8225 <b>8226 <span style="font-size: 14pt;"><a name="StarPolymer"></a><a name="StarPolymerModel">Star Polymer with Gaussian Statistics</a></span>8227 </b>8228 </p>8229 <p style="margin-left: 0.25in;">For a star with <i>f</i> arms: </p>8230 <p style="text-align: center;" align="center"><span style="font-size: 12pt; font-family: "Times New Roman","serif"; position: relative; top: 4.5pt;"><img src="star1.png"></span>8231 </p>8232 <p style="text-align: center;" align="center">8233 <span style="font-size: 12pt; font-family: "Times New Roman","serif"; position: relative; top: 4.5pt;"><img src="star2.png" /></span>8234 </p>8235 <p style="text-align: center;" align="center">8236 <span style="font-size: 12pt; font-family: "Times New Roman","serif"; position: relative; top: 4.5pt;"><img src="star3.png" /></span>8237 </p>8238 <p style="margin-left: 0.25in; float: top">where <R<sub>g</sub><sup>2</sup>> is the ensemble average radius of gyration squared of an arm. </p>8239 <p style="margin-left: 0.25in; text-align: center;" align="center"> </p>8240 <p style="margin-left: 0.25in;">References:8241 </p>8242 <p style="margin-left: 0.25in; text-indent: 0.25in;">H. Benoit, J. Polymer Science., 11,8243 596-599 (1953)</p>8244 <p> </p>8245 8246 8220 8247 8221 <p style="margin-left: 0.55in; text-indent: -0.3in;"><b><span style="font-size: 14pt;">3.10.</span></b><b><span style="font-size: 7pt;"> … … 10619 10593 Simon Mallam, Ferenc Horkay, Anne-Marie Hecht, Adrian R. Rennie, Erik Geissler, Macromolecules 1991, 24, 543-548.</p> 10620 10594 10621 10622 10623 10624 10625 <p class="MsoListParagraph" style="margin-left: 0.55in; text-indent: -0.3in;"><b><span style="font-size: 14pt;">3.28.</span></b><b><span style="font-size: 7pt;"> 10595 <p/> 10596 <p style="margin-left: 0.55in; text-indent: -0.3in;"><b><span style="font-size: 14pt;">3.29.</span></b> 10597 <b> 10598 <span style="font-size: 7pt;"> 10599 </span> 10600 </b> 10601 <b> 10602 <span style="font-size: 14pt;"><a name="StarPolymer"></a><a name="StarPolymerModel">Star Polymer with Gaussian Statistics</a></span> 10603 </b> 10604 </p> 10605 <p style="margin-left: 0.25in;">For a star with <i>f</i> arms: </p> 10606 <p style="text-align: center;" align="center"><span style="font-size: 12pt; font-family: "Times New Roman","serif"; position: relative; top: 4.5pt;"><img src="star1.png"></span> 10607 </p> 10608 <p style="text-align: center;" align="center"> 10609 <span style="font-size: 12pt; font-family: "Times New Roman","serif"; position: relative; top: 4.5pt;"><img src="star2.png" /></span> 10610 </p> 10611 <p style="text-align: center;" align="center"> 10612 <span style="font-size: 12pt; font-family: "Times New Roman","serif"; position: relative; top: 4.5pt;"><img src="star3.png" /></span> 10613 </p> 10614 <p style="margin-left: 0.25in; float: top">where <R<sub>g</sub><sup>2</sup>> is the ensemble average radius of gyration squared of an arm. </p> 10615 <p style="margin-left: 0.25in; text-align: center;" align="center"> </p> 10616 <p style="margin-left: 0.25in;">References: 10617 </p> 10618 <p style="margin-left: 0.25in; text-indent: 0.25in;">H. Benoit, J. Polymer Science., 11, 10619 596-599 (1953)</p> 10620 <p> </p> 10621 10622 10623 10624 10625 10626 <p class="MsoListParagraph" style="margin-left: 0.55in; text-indent: -0.3in;"><b><span style="font-size: 14pt;">3.30.</span></b><b><span style="font-size: 7pt;"> 10626 10627 </span></b><a name="FractalO_Z"><b><span style="font-size: 14pt;">FractalO_Z</span></b></a></p> 10627 10628
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