31![Heavy Element Production and Neutrino-Driven Jets in Neutron-Star Merger Oliver Just Max-Planck-Institut für Astrophysik, Garching, Germany Heavy Element Production and Neutrino-Driven Jets in Neutron-Star Merger Oliver Just Max-Planck-Institut für Astrophysik, Garching, Germany](https://www.pdfsearch.io/img/17a61e334855bde70b693c61b7b0f0cd.jpg) | Add to Reading ListSource URL: www.resceu.s.u-tokyo.ac.jpLanguage: English - Date: 2016-07-26 22:16:08
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32![Measurement of the Gerasimov-Drell-Hearn Integral at low Q2 on the Deuteron and Neutron A. Deur (Co-spokesperson and contact), P. Bosted, V. Burkert, V. Dharmawardane, Thomas Jefferson National Accelerator Facility Measurement of the Gerasimov-Drell-Hearn Integral at low Q2 on the Deuteron and Neutron A. Deur (Co-spokesperson and contact), P. Bosted, V. Burkert, V. Dharmawardane, Thomas Jefferson National Accelerator Facility](https://www.pdfsearch.io/img/0b9ea2b4a7254e1ccb7da3184af547b9.jpg) | Add to Reading ListSource URL: www.jlab.orgLanguage: English - Date: 2005-12-12 10:50:23
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33![Flash Report on the first outcome from RIKEN RI beam factory commissioned on March 27, 2007 Discovery of a very neutron-rich new isotope Pd 125 (N (N=79, Flash Report on the first outcome from RIKEN RI beam factory commissioned on March 27, 2007 Discovery of a very neutron-rich new isotope Pd 125 (N (N=79,](https://www.pdfsearch.io/img/2659ff394e7b36ae39e5c41f1a03d035.jpg) | Add to Reading ListSource URL: inpc2007.riken.jpLanguage: English - Date: 2007-06-07 04:04:28
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34![THE MEASUREMENT OF THE NEUTRON STAR RADIUS THE MEASUREMENT OF THE NEUTRON STAR RADIUS](https://www.pdfsearch.io/img/e939fd15dd7752fd523127494c814d01.jpg) | Add to Reading ListSource URL: www.nucl.phys.tohoku.ac.jpLanguage: English - Date: 2013-07-22 22:22:54
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35![Press release – October 17th, 2017 Observation of gravitational waves from binary neutron stars opens the way to new science IHES congratulates the LIGO/Virgo project team which announced, on October 16th, the first o Press release – October 17th, 2017 Observation of gravitational waves from binary neutron stars opens the way to new science IHES congratulates the LIGO/Virgo project team which announced, on October 16th, the first o](https://www.pdfsearch.io/img/df9e329ff4a646afce4419b881219cdb.jpg) | Add to Reading ListSource URL: www.ihes.frLanguage: English - Date: 2017-11-30 04:33:07
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36![New Maxwellian Average Neutron Capture Cross Sections for 35 37Cl ; 1 K. H. Guber,1 R. O. Sayer,1, T. E. Valentine,1 L. C. Leal,1 R. New Maxwellian Average Neutron Capture Cross Sections for 35 37Cl ; 1 K. H. Guber,1 R. O. Sayer,1, T. E. Valentine,1 L. C. Leal,1 R.](https://www.pdfsearch.io/img/50709df7ab2ad2f3e8affee38c075299.jpg) | Add to Reading ListSource URL: thomasrauscher.chLanguage: English - Date: 2002-03-07 05:19:26
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37![Neutron diffraction study of SnO2-CeO2-SbOx system K. Nomura (A), H. Kageyama (A), C. Minagoshi (B), Y. Kawabata (B), T. Maekawa (B), and K. Kanda (B) (A) National Institute of Advanced Industrial Science and Technology Neutron diffraction study of SnO2-CeO2-SbOx system K. Nomura (A), H. Kageyama (A), C. Minagoshi (B), Y. Kawabata (B), T. Maekawa (B), and K. Kanda (B) (A) National Institute of Advanced Industrial Science and Technology](https://www.pdfsearch.io/img/a9b202eee47aebeb3f03918a231b6479.jpg) | Add to Reading ListSource URL: quasi.issp.u-tokyo.ac.jpLanguage: English - Date: 2010-12-31 00:10:30
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38![Synthesis and neutron diffraction of iron-based high-T c superconductor 154 SmFeAsO 1−x D x Soshi Iimura, Hideo Hosono:Tokyo Tech Electron-doped SmFeAsO shows the highest critical temperature (T c ) among all iron-ba Synthesis and neutron diffraction of iron-based high-T c superconductor 154 SmFeAsO 1−x D x Soshi Iimura, Hideo Hosono:Tokyo Tech Electron-doped SmFeAsO shows the highest critical temperature (T c ) among all iron-ba](https://www.pdfsearch.io/img/9a1d82ba747912729a691b273a55a4a4.jpg) | Add to Reading ListSource URL: elements-strategy.jpLanguage: English - Date: 2018-02-01 00:01:11
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39![Nuclear Waffles in Neutron Star Crust Objectives Use large scale GPU computing to perform detailed MD simulations of dense neutron rich matter. Explore complex nuclear pasta phases in the crust of neutron stars. Nuclear Waffles in Neutron Star Crust Objectives Use large scale GPU computing to perform detailed MD simulations of dense neutron rich matter. Explore complex nuclear pasta phases in the crust of neutron stars.](https://www.pdfsearch.io/img/182b3a762b4c926980cdb93ed7546a1a.jpg) | Add to Reading ListSource URL: nuclei.mps.ohio-state.edu- Date: 2014-10-30 21:41:12
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40![International Symposium on Physics and Astronomy of Neutron Stars and Supernovae Symposium will be held in the Lecture Room in Main Building (North). 22nd, JuneMonday) T. Kajino : Opening International Symposium on Physics and Astronomy of Neutron Stars and Supernovae Symposium will be held in the Lecture Room in Main Building (North). 22nd, JuneMonday) T. Kajino : Opening](https://www.pdfsearch.io/img/59117f1c11d06395065add6b6058a770.jpg) | Add to Reading ListSource URL: th.nao.ac.jpLanguage: English - Date: 2015-06-16 21:57:57
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