00001 /* 00002 ------------------------------------------------------------------- 00003 00004 Copyright (C) 2006, 2007, 2008, Andrew W. Steiner 00005 00006 This file is part of O2scl. 00007 00008 O2scl is free software; you can redistribute it and/or modify 00009 it under the terms of the GNU General Public License as published by 00010 the Free Software Foundation; either version 3 of the License, or 00011 (at your option) any later version. 00012 00013 O2scl is distributed in the hope that it will be useful, 00014 but WITHOUT ANY WARRANTY; without even the implied warranty of 00015 MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the 00016 GNU General Public License for more details. 00017 00018 You should have received a copy of the GNU General Public License 00019 along with O2scl. If not, see <http://www.gnu.org/licenses/>. 00020 00021 ------------------------------------------------------------------- 00022 */ 00023 /** \mainpage 00024 00025 \htmlonly 00026 <a href="../latex/refman.pdf">PDF documentation</a> 00027 \endhtmlonly 00028 00029 \hline 00030 \section dcsect Quick Reference to User's Guide 00031 - \ref hadronic 00032 - \ref quark_matter 00033 - \ref tovtoc 00034 - \ref cnstar 00035 - \ref eossource_section 00036 - \ref eosref_section 00037 00038 \hline 00039 \section hadronic Hadronic equations of state 00040 00041 The hadronic equations of state are all inherited from 00042 hadronic_eos: schematic_eos, skyrme_eos, rmf_eos, apr_eos, and 00043 gen_potential_eos. 00044 00045 hadronic_eos includes several methods that can be used 00046 to calculate the saturation properties of nuclear matter. 00047 These methods are sometimes overloaded in descendants when 00048 exact formulas are available. 00049 00050 There is also a set of classes to modify the quartic term 00051 of the symmetry energy: rmf4_eos, apr4_eos, skyrme4_eos, and 00052 mdi4_eos all based on sym4_eos_base which can be used 00053 in sym4_eos. 00054 00055 \hline 00056 \section quark_matter Equations of state of quark matter 00057 00058 The equations of state of \quark matter are all inherited from 00059 quark_eos: bag_eos is a simple bag model, nambujl_eos is the 00060 Nambu-Jona-Lasinio model. The CFL and 2SC phases are described 00061 by \ref cfl_njl_eos, and \ref cfl6_eos adds the 00062 color-superconducting 't Hooft interaction. 00063 00064 \hline 00065 \section tovtoc Solution of the Tolman-Oppenheimer-Volkov equations 00066 00067 The class \ref tov_solve provide a solution to the 00068 Tolman-Oppenheimer-Volkov (TOV) equations given an equation of 00069 state. This is particularly useful for static neutron star 00070 structure: given any equation of state one can calculate the mass 00071 vs. radius curve and the properties of any star of a given 00072 mass. An adaptive integration is employed and calculates the 00073 gravitational mass, the baryonic mass (if the baryon density is 00074 supplied), and the gravitational potential. The remaining columns 00075 is the equation of state are also interpolated into the solution, 00076 e.g. if a chemical potential is given, then the radial dependence 00077 of the chemical potential for a 1.4 solar mass star can be 00078 automatically computed. The equation of state may be specified in 00079 arbitrary units so long as an appropriate conversion factor is 00080 supplied. An equation of state for low densities (baryon density < 00081 0.08 \f$ \mathrm{fm}^{-3} \f$ ) is provided and can be 00082 automatically appended to the user-defined equation of state. 00083 00084 This is still experimental. 00085 00086 \hline 00087 \section cnstar Naive Cold Neutron Stars 00088 00089 There is also a class to calculate zero-temperature neutron 00090 stars: \ref cold_nstar. It uses \ref tov_solve to compute 00091 the structure, given a hadronic equation of state (of type 00092 \ref hadronic_eos). It also computes the adiabatic index, the 00093 speed of sound, and determines the possibility of the 00094 direct Urca process as a function of density or radius. 00095 00096 This is still experimental. 00097 00098 \hline 00099 \section eossource_section Example source code 00100 00101 \subsection exlist_eos_subsect Example list 00102 00103 - \ref ex_cold_nstar_sect 00104 00105 \subsection ex_cold_nstar_sect Cold neutron star example 00106 00107 \dontinclude ex_cold_nstar.cpp 00108 \skip Example: 00109 \until End of example 00110 00111 \hline 00112 \section todo_section Other Todos 00113 00114 \future Right now, the equation of state classes depend on the 00115 user to input the correct value of \c non_interacting 00116 for the particle inputs. This is not very graceful... 00117 00118 \hline 00119 \section eosref_section Bibliography 00120 00121 Some of the references which contain links should direct you to 00122 the work referred to directly through dx.doi.org. 00123 00124 \anchor Akmal98 Akmal98: 00125 \htmlonly 00126 <a href="http://dx.doi.org/10.1103/PhysRevC.58.1805"> 00127 Akmal, Pandharipande, and Ravenhall</a>, 00128 \endhtmlonly 00129 \latexonly 00130 \href{http://dx.doi.org/10.1103/PhysRevC.58.1805}{ 00131 Akmal, Pandharipande, and Ravenhall}, 00132 \endlatexonly 00133 Phys. Rev. C \b 58, 1805 (1998). 00134 00135 \anchor Bartel79 Bartel79: 00136 \htmlonly 00137 <a href="http://dx.doi.org/10.1016/0375-9474(82)90403-1"> 00138 J. Bartel, P. Quentin, M. Brack, C. Guet, and Håkansson</a>, 00139 \endhtmlonly 00140 \latexonly 00141 \href{http://dx.doi.org/10.1016/0375-9474(82)90403-1}{ 00142 J. Bartel, P. Quentin, M. Brack, C. Guet, and H{\aa}kansson}, 00143 \endlatexonly 00144 Nucl. Phys. A \b 386 (1982) 79. 00145 00146 \anchor Baym71 Baym71: 00147 G. Baym, C. Pethick, and P. Sutherland, Astrophys. J. \b 170 (1971) 299. 00148 00149 \anchor Beiner75 Beiner75: 00150 \htmlonly 00151 <a href="http://dx.doi.org/10.1016/0375-9474(75)90338-3"> 00152 M. Beiner, H. Flocard, Nguyen van Giai, and P. Quentin</a>, 00153 \endhtmlonly 00154 \latexonly 00155 \href{http://dx.doi.org/10.1016/0375-9474(75)90338-3}{ 00156 M. Beiner, H. Flocard, Nguyen van Giai, and P. Quentin}, 00157 \endlatexonly 00158 Nucl. Phys. A \b 238 (1975) 29. 00159 00160 \anchor Bernard88 Bernard88: 00161 \htmlonly 00162 <a href="http://dx.doi.org/10.1016/0550-3213(88)90127-7"> 00163 V. Bernard, R.L. Jaffe, and U.-G. Meissner</a>, 00164 \endhtmlonly 00165 \latexonly 00166 \href{http://dx.doi.org/10.1016/0550-3213(88)90127-7}{ 00167 V. Bernard, R.~L. Jaffe, and U.-G. Meissner}, 00168 \endlatexonly 00169 Nucl. Phys. B \b 308 (1988) 753. 00170 00171 \anchor Bombaci01 Bombaci01: 00172 I. Bombaci, "Equation of State for Dense Isospin Asymmetric 00173 Nuclear Matter for Astrophysical Applications Equation of 00174 State for Isospin-Asymmetric Nuclear Matter and Neutron Star 00175 Properties", in "Isospin physics in heavy-ion collisions at 00176 intermediate energies" 00177 \htmlonly 00178 ed. by B-A. Li and W. U. Schröder (2001) Nova Science, New York. 00179 \endhtmlonly 00180 \latexonly 00181 ed. by B-A. Li and W. U. Schr\"{o}der (2001) Nova Science, New York. 00182 \endlatexonly 00183 00184 \anchor Brack85 Brack85: 00185 \htmlonly 00186 <a href="http://dx.doi.org/10.1016/0370-1573(86)90078-5"> 00187 M. Brack, C. Guet, and H.-B. Håkansson</a> 00188 \endhtmlonly 00189 \latexonly 00190 \href{http://dx.doi.org/10.1016/0370-1573(86)90078-5}{ 00191 M. Brack, C. Guet, and H.-B. H{\aa}kansson}, 00192 \endlatexonly 00193 Phys. Rep. \b 123 (1985) 275. 00194 00195 \anchor Buballa99 Buballa99: 00196 \htmlonly 00197 <a href="http://dx.doi.org/10.1016/S0370-2693(99)00533-X"> 00198 M. Buballa and M. Oertel</a>, 00199 \endhtmlonly 00200 \latexonly 00201 \href{http://dx.doi.org/10.1016/S0370-2693(99)00533-X}{ 00202 M. Buballa and M. Oertel}, 00203 \endlatexonly 00204 Phys. Lett. B \b 457 (1999) 261. 00205 00206 \anchor Buballa04 Buballa04: 00207 \htmlonly 00208 <a href="http://dx.doi.org/10.1016/j.physrep.2004.11.004"> 00209 M. Buballa</a>, 00210 \endhtmlonly 00211 \latexonly 00212 \href{http://dx.doi.org/10.1016/j.physrep.2004.11.004}{ 00213 M. Buballa}, 00214 \endlatexonly 00215 Phys. Rep. \b 407 (2005) 205-376. 00216 00217 \anchor Chabanat95 Chabanat95: 00218 E. Chabanat, Ph. D. Thesis 1995 00219 00220 \anchor Chabanat97 Chabanat97: 00221 \htmlonly 00222 <a href="http://dx.doi.org/10.1016/S0375-9474(97)00596-4"> 00223 E. Chabanat, J. Meyer, P. Bonche, R. Schaeffer, and P. Haensel</a>, 00224 \endhtmlonly 00225 \latexonly 00226 \href{http://dx.doi.org/10.1016/S0375-9474(97)00596-4}{ 00227 E. Chabanat, J. Meyer, P. Bonche, R. Schaeffer, and P. Haensel}, 00228 \endlatexonly 00229 Nucl. Phys. A \b 627 (1997) 710. 00230 00231 \anchor Danielewicz08 Danielewicz08: 00232 \htmlonly 00233 <a href="http://arxiv.org/abs/0807.3743"> 00234 P. Danielewicz, J. Lee</a>, 00235 \endhtmlonly 00236 \latexonly 00237 \href{http://arxiv.org/abs/0807.3743}{ 00238 P. Danielewicz, J. Lee}, 00239 \endlatexonly 00240 arXiv.org:0807.3743. 00241 00242 \anchor Das03 Das03: 00243 \htmlonly 00244 <a href="http://dx.doi.org/10.1103/PhysRevC.67.034611"> 00245 C.B. Das, S. Das Gupta, C. Gale, and B.-A. Li</a>, 00246 \endhtmlonly 00247 \latexonly 00248 \href{http://dx.doi.org/10.1103/PhysRevC.67.034611}{ 00249 C.B. Das, S. Das Gupta, C. Gale, and B.-A. Li}, 00250 \endlatexonly 00251 Phys. Rev. C \b 67 (2003) 034611. 00252 00253 \anchor Dobaczewski94 Dobaczewski94: 00254 \htmlonly 00255 <a href="http://dx.doi.org/10.1016/0375-9474(84)90433-0"> 00256 J. Dobaczewski, H. Flocard, and J. Treiner</a>, 00257 \endhtmlonly 00258 \latexonly 00259 \href{http://dx.doi.org/10.1016/0375-9474(84)90433-0}{ 00260 J. Dobaczewski, H. Flocard, and J. Treiner}, 00261 \endlatexonly 00262 Nucl. Phys. A \b 422 (1984) 103. 00263 00264 \anchor Dutta86 Dutta86: 00265 \htmlonly 00266 <a href="http://dx.doi.org/10.1016/0375-9474(86)90283-6"> 00267 A.K.Dutta, J.-P.Arcoragi, J.M.Pearson, R.Behrman, F.Tondeur</a>, 00268 \endhtmlonly 00269 \latexonly 00270 \href{http://dx.doi.org/10.1016/0375-9474(86)90283-6}{ 00271 A.K.Dutta, J.-P.Arcoragi, J.M.Pearson, R.Behrman, F.Tondeur}, 00272 \endlatexonly 00273 Nucl. Phys. A \b 458 (1986) 77. 00274 00275 \anchor Friedrich86 Friedrich86: 00276 \htmlonly 00277 <a href="http://dx.doi.org/10.1103/PhysRevC.33.335"> 00278 J. Friedrich, and P.-G. Reinhard</a>, 00279 \endhtmlonly 00280 \latexonly 00281 \href{http://dx.doi.org/10.1103/PhysRevC.33.335}{ 00282 J. Friedrich, and P.-G. Reinhard}, 00283 \endlatexonly 00284 Phys. Rev. C \b 33 (1986) 335. 00285 00286 \anchor Gaitanos04 Gaitanos04: 00287 \htmlonly 00288 <a href="http://dx.doi.org/10.1016/j.nuclphysa.2003.12.001"> 00289 T. Gaitanos, M. Di Toro, S. Typel, V. Barana, C. Fuchs, 00290 V. Greco, and d H. H. Wolter</a>, 00291 \endhtmlonly 00292 \latexonly 00293 \href{http://dx.doi.org/10.1016/j.nuclphysa.2003.12.001}{ 00294 T. Gaitanos, M. Di Toro, S. Typel, V. Barana, C. Fuchs, 00295 V. Greco, and d H. H. Wolter}, 00296 \endlatexonly 00297 Nucl. Phys. A \b 732 (2004) 24. 00298 00299 \anchor Gale87 Gale87: 00300 \htmlonly 00301 <a href="http://dx.doi.org/10.1103/PhysRevC.35.1666"> 00302 C. Gale, G. Bertsch, and S. Das Gupta</a>, 00303 \endhtmlonly 00304 \latexonly 00305 \href{http://dx.doi.org/10.1103/PhysRevC.35.1666}{ 00306 C. Gale, G. Bertsch, and S. Das Gupta}, 00307 \endlatexonly 00308 Phys. Rev. C \b 35 (1986) 1666. 00309 00310 \anchor Hatsuda94 Hatsuda94: 00311 \htmlonly 00312 <a href="http://dx.doi.org/10.1016/0370-1573(94)90022-1"> 00313 T. Hatsuda and T. Kunihiro</a>, 00314 \endhtmlonly 00315 \latexonly 00316 \href{http://dx.doi.org/10.1016/0370-1573(94)90022-1}{ 00317 T. Hatsuda and T. Kunihiro}, 00318 \endlatexonly 00319 Phys. Rep. \b 247 (1994) 221. 00320 00321 \anchor Horowitz01 Horowitz01: 00322 \htmlonly 00323 <a href="http://dx.doi.org/10.1103/PhysRevLett.86.5647"> 00324 C.J. Horowitz and J. Piekarewicz</a>, 00325 \endhtmlonly 00326 \latexonly 00327 \href{http://dx.doi.org/10.1103/PhysRevLett.86.5647}{ 00328 C.~J. Horowitz and J. Piekarewicz}, 00329 \endlatexonly 00330 Phys. Rev. Lett. \b 86 (2001) 5647. 00331 00332 \anchor Kubis97 Kubis97: 00333 \htmlonly 00334 <a href="http://dx.doi.org/10.1016/S0370-2693(97)00306-7"> 00335 S. Kubis and M. Kutschera</a>, 00336 \endhtmlonly 00337 \latexonly 00338 \href{http://dx.doi.org/10.1016/S0370-2693(97)00306-7}{ 00339 S. Kubis and M. Kutschera}, 00340 \endlatexonly 00341 Phys. Lett. B \b 399 (1997) 191. 00342 00343 \anchor Lattimer01 Lattimer01: 00344 \htmlonly 00345 <a href="http://dx.doi.org/10.1086/319702"> 00346 J. M. Lattimer and M. Prakash</a>, 00347 \endhtmlonly 00348 \latexonly 00349 \href{http://dx.doi.org/10.1086/319702}{ 00350 J. M. Lattimer and M. Prakash}, 00351 \endlatexonly 00352 Astrophys. J. \b 550 (2001) 426. 00353 00354 \anchor Margueron02 Margueron02: 00355 \htmlonly 00356 <a href="http://dx.doi.org/10.1103/PhysRevC.66.014303"> 00357 J. Margueron, J. Navarro, and N.V. Giai</a>, 00358 \endhtmlonly 00359 \latexonly 00360 \href{http://dx.doi.org/10.1103/PhysRevC.66.014303}{ 00361 J. Margueron, J. Navarro, and N.~V. Giai}, 00362 \endlatexonly 00363 Phys. Rev. C \b 66 (2002) 014303. 00364 00365 \anchor Muller96 Muller96: 00366 \htmlonly 00367 <a href="http://dx.doi.org/10.1016/0375-9474(96)00187-X"> 00368 H. Muller and B. D. Serot</a>, 00369 \endhtmlonly 00370 \latexonly 00371 \href{http://dx.doi.org/10.1016/0375-9474(96)00187-X}{ 00372 H. Muller and B.~D. Serot}, 00373 \endlatexonly 00374 Nucl. Phys. A \b 606 (1996), 508. 00375 00376 \anchor Onsi94 Onsi94: 00377 \htmlonly 00378 <a href="http://dx.doi.org/10.1103/PhysRevC.50.460"> 00379 M. Onsi, H. Przysiezniak, J.M. Pearson</a>, 00380 \endhtmlonly 00381 \latexonly 00382 \href{http://dx.doi.org/10.1103/PhysRevC.50.460}{ 00383 M. Onsi, H. Przysiezniak, J.M. Pearson}, 00384 \endlatexonly 00385 Phys. Rev. C \b 50 (1994) 460. 00386 00387 \anchor Pethick95 Pethick95: 00388 \htmlonly 00389 <a href="http://dx.doi.org/10.1016/0375-9474(94)00506-I"> 00390 C.J. Pethick, D.G. Ravenhall, and C.P. Lorenz</a>, 00391 \endhtmlonly 00392 \latexonly 00393 \href{http://dx.doi.org/10.1016/0375-9474(94)00506-I}{ 00394 C.~J. Pethick, D.~G. Ravenhall, and C.~P. Lorenz}, 00395 \endlatexonly 00396 Nucl. Phys. A \b 584 (1995) 675. 00397 00398 \anchor Prakash87 Prakash87: 00399 \htmlonly 00400 M. Prakash, T.L. Ainsworth, J.P. Blaizot, and H. Wolter, 00401 in Windsurfing the Fermi Sea, Volume II 00402 edited by T.T.S. Kuo and J. Speth, Elsevier 1987, pg. 357. 00403 \endhtmlonly 00404 \latexonly 00405 M. Prakash, T.~L. Ainsworth, J.~P. Blaizot, and H. Wolter, 00406 in Windsurfing the Fermi Sea, Volume II 00407 edited by T.~T.~S. Kuo and J. Speth, Elsevier 1987, pg. 357. 00408 \endlatexonly 00409 00410 \anchor Prakash88 Prakash88: 00411 \htmlonly 00412 <a href="http://dx.doi.org/10.1103/PhysRevLett.61.2518"> 00413 M. Prakash, T. L. Ainsworth, and J. M. Lattimer</a>, 00414 \endhtmlonly 00415 \latexonly 00416 \href{http://dx.doi.org/10.1103/PhysRevLett.61.2518}{ 00417 M. Prakash, T.~L. Ainsworth, and J.~M. Lattimer}, 00418 \endlatexonly 00419 Phys. Rev. Lett. \b 61 (1988) 2518. 00420 00421 \anchor Prakash97 Prakash97: 00422 \htmlonly 00423 <a href="http://dx.doi.org/10.1016/S0370-1573(96)00023-3"> 00424 Madappa Prakash, I. Bombaci, Manju Prakash, P.J. Ellis, J.M. Lattimer, 00425 and R. Knorren</a>, 00426 \endhtmlonly 00427 \latexonly 00428 \href{http://dx.doi.org/10.1016/S0370-1573(96)00023-3}{ 00429 Madappa Prakash, I. Bombaci, Manju Prakash, P.~J. Ellis, J.~M. Lattimer, 00430 and R. Knorren}, 00431 \endlatexonly 00432 Phys. Rep. \b 280 (1997) 1. 00433 00434 \anchor Reinhard95 Reinhard95: 00435 \htmlonly 00436 <a href="http://dx.doi.org/10.1016/0375-9474(94)00770-N"> 00437 P.-G. Reinhard and H. Flocard</a>, 00438 \endhtmlonly 00439 \latexonly 00440 \href{http://dx.doi.org/10.1016/0375-9474(94)00770-N}{ 00441 P.-G. Reinhard and H. Flocard}, 00442 \endlatexonly 00443 Nucl. Phys. A \b 584 (1995) 467. 00444 00445 \anchor Reinhard99 Reinhard99: 00446 \htmlonly 00447 <a href="http://dx.doi.org/10.1103/PhysRevC.60.014316"> 00448 P.-G. Reinhard, D.J. Dean, W. Nazarewicz, J. Dobaczewski, 00449 J.A. Maruhn, M.R. Strayer</a>, 00450 \endhtmlonly 00451 \latexonly 00452 \href{http://dx.doi.org/10.1103/PhysRevC.60.014316}{ 00453 P.-G. Reinhard, D.J. Dean, W. Nazarewicz, J. Dobaczewski, 00454 J.A. Maruhn, M.R. Strayer}, 00455 \endlatexonly 00456 Phys. Rev. C \b 60, (1999) 014316. 00457 00458 \anchor Shapiro83 Shapiro83: 00459 S. L. Shapiro and S. A. Teukolsky, "Black Holes, White Dwarfs, 00460 and Neutron Stars: The Physics of Compact Objects", John 00461 Wiley and Sons, New York, 1983. 00462 00463 \anchor Skyrme59 Skyrme59: 00464 \htmlonly 00465 <a href=""> 00466 T. H. R. Skyrme</a>, 00467 \endhtmlonly 00468 \latexonly 00469 \href{}{ 00470 T. H. R. Skyrme}, 00471 \endlatexonly 00472 Nucl. Phys. \b 9 (1959) 615. 00473 00474 \anchor Steiner00 Steiner00: 00475 \htmlonly 00476 <a href="http://dx.doi.org/10.1016/S0370-2693(00)00780-2"> 00477 A. W. Steiner, M. Prakash, and J. M. Lattimer</a>, 00478 \endhtmlonly 00479 \latexonly 00480 \href{http://dx.doi.org/10.1016/S0370-2693(00)00780-2}{ 00481 A. W. Steiner, M. Prakash, and J.M. Lattimer}, 00482 \endlatexonly 00483 Phys. Lett. B, \b 486 (2000) 239. 00484 00485 \anchor Steiner02 Steiner02: 00486 \htmlonly 00487 <a href="http://dx.doi.org/10.1103/PhysRevD.66.094007"> 00488 A. W. Steiner, S. Reddy, and M. Prakash</a>, 00489 \endhtmlonly 00490 \latexonly 00491 \href{http://dx.doi.org/10.1103/PhysRevD.66.094007}{ 00492 A. W. Steiner, S. Reddy, and M. Prakash}, 00493 \endlatexonly 00494 Phys. Rev. D, \b 66 (2002) 094007. 00495 00496 \anchor Steiner05 Steiner05: 00497 \htmlonly 00498 <a href="http://dx.doi.org/10.1103/PhysRevD.72.054024"> 00499 A. W. Steiner</a>, 00500 \endhtmlonly 00501 \latexonly 00502 \href{http://dx.doi.org/10.1103/PhysRevD.72.054024}{ 00503 A. W. Steiner}, 00504 \endlatexonly 00505 Phys. Rev. D, \b 72 (2005) 054024. 00506 00507 \anchor Steiner06 Steiner06: 00508 \htmlonly 00509 <a href="http://dx.doi.org/10.1103/PhysRevC.74.045808"> 00510 A. W. Steiner</a>, 00511 \endhtmlonly 00512 \latexonly 00513 \href{http://dx.doi.org/10.1103/PhysRevC.74.045808}{ 00514 A. W. Steiner}, 00515 \endlatexonly 00516 Phys. Rev. C, \b 74 (2006) 045808. 00517 00518 \anchor Tondeur84 Tondeur84: 00519 \htmlonly 00520 <a href="http://dx.doi.org/10.1016/0375-9474(84)90444-5"> 00521 F. Tondeur, M. Brack, M. Farine, and J.M. Pearson</a>, 00522 \endhtmlonly 00523 \latexonly 00524 \href{http://dx.doi.org/10.1016/0375-9474(84)90444-5}{ 00525 F. Tondeur, M. Brack, M. Farine, and J.M. Pearson}, 00526 \endlatexonly 00527 Nucl. Phys. A \b 420 (1984) 297. 00528 00529 \anchor Typel99 Typel99: 00530 \htmlonly 00531 <a href="http://dx.doi.org/10.1016/S0375-9474(99)00310-3"> 00532 S. Typel and H. H. Wolter</a>, 00533 \endhtmlonly 00534 \latexonly 00535 \href{http://dx.doi.org/10.1016/S0375-9474(99)00310-3} 00536 {S. Typel and H. H. Wolter}, 00537 \endlatexonly 00538 Nucl. Phys. A \b 656 (1999) 331. 00539 00540 \anchor VanGiai81 VanGiai81: 00541 \htmlonly 00542 <a href="http://dx.doi.org/10.1016/0370-2693(81)90646-8"> 00543 Nguyen van Giai and H. Sagawa</a>, 00544 \endhtmlonly 00545 \latexonly 00546 \href{http://dx.doi.org/10.1016/0370-2693(81)90646-8}{ 00547 Nguyen van Giai and H. Sagawa}, 00548 \endlatexonly 00549 Phys. Lett. B \b 106 (1981) 379. 00550 00551 \anchor Zimanyi90 Zimanyi90: 00552 \htmlonly 00553 <a href="http://dx.doi.org/10.1103/PhysRevC.42.1416"> 00554 Zimanyi and Moszkowski</a>, 00555 \endhtmlonly 00556 \latexonly 00557 \href{http://dx.doi.org/10.1103/PhysRevC.42.1416}{ 00558 Zimanyi and Moszkowski}, 00559 \endlatexonly 00560 Phys. Rev. C \b 42 (1990) 1416. 00561 00562 \comment 00563 A blank reference 00564 00565 \anchor : 00566 \htmlonly 00567 <a href=""> 00568 </a>, 00569 \endhtmlonly 00570 \latexonly 00571 \href{}{ 00572 }, 00573 \endlatexonly 00574 00575 \endcomment 00576 00577 */
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