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| ¾®ÎÓ Þ« | ÅìµþÂç³Ø RESCEU | PD | °ìÈÌ | Non-Gaussianity from Curvatons Revisited |
| ¿ÜÆ£¡¡Ì÷ | ÅìµþÂç³ØÍý³ØÉô ±§ÃèÍýÏÀ¸¦µæ¼¼ | ¶µ¼ø | ¥×¥í | opening |
| Matthew Lake | RESCEU, University of Tokyo | PD | °ìÈÌ | Spinning Cosmic Strings |
| ÇðÌÚ¡¡½ÓºÈ | ÅìµþÂç³ØÍý³ØÉô ±§ÃèÍýÏÀ¸¦µæ¼¼ | Âç³Ø±¡À¸¡ÊM2¡Ë | x | - |
| ÃæÅç¡¡ÀµÍµ | ÅìµþÂç³Ø¥Ó¥Ã¥°¥Ð¥ó±§Ãè¹ñºÝ¸¦µæ¥»¥ó¥¿¡¼ | Âç³Ø±¡À¸¡ÊÇî»Î3ǯ¡Ë | °ìÈÌ | Sound Velocity and Features in the Primordial Power Spectrum |
| ËÒ±º¡¡¸²ÆóϺ | ÅìµþÂç³Ø RESCEU | Âç³Ø±¡À¸¡ÊM2¡Ë | x | - |
| Ëܶ¶ È»¿Í | ÅìµþÂç³ØÂç³Ø±¡Íý³Ø·Ï¸¦µæ²ÊÉí°¥Ó¥Ã¥°¥Ð¥ó±§Ãè¹ñºÝ¸¦µæ¥»¥ó¥¿¡¼ | Âç³Ø±¡À¸¡ÊD2¡Ë | °ìÈÌ | Constructing cosmological f(R) models for inflation and cosmic acceleration |
| ¿ÜÆ£¡¡ÂçÃÏ | ÅìµþÂç³ØÍý³ØÉô¡¡±§ÃèÍýÏÀ¸¦µæ¼¼ | Âç³Ø±¡À¸¡Ê½¤»Î1ǯ¡Ë | x | - |
| µÈÌî °ì·Ä | ÅìµþÂç³Ø ±§ÃèÀþ¸¦µæ½ê ÍýÏÀ¥°¥ë¡¼¥× | Âç³Ø±¡À¸¡ÊM1¡Ë | x | - |
| ²¬¥¢¥¥é | ÅìµþÂç³ØÍý³ØÉô ±§ÃèÍýÏÀ¸¦µæ¼¼ | Âç³Ø±¡À¸¡ÊM1¡Ë | x | - |
| XUE YUXIN | ÅìµþÂç³ØÍý³ØÉô ±§ÃèÍýÏÀ¸¦µæ¼¼ | Âç³Ø±¡À¸¡ÊM1¡Ë | x | - |
| ¾®ÎÓ¡¡ÅØ | µþÅÔÂç³Ø¡¡¼¡À¤Â带µæ¼Ô°éÀ®¥»¥ó¥¿¡¼ | ½õ¶µ | °ìÈÌ | Generalized Galileons and inflation |
| »³ÅÄ¡¡Õò¼ù | ÅìµþÂç³Ø¡¡±§ÃèÀþ¸¦µæ½ê¡¡ÍýÏÀ¥°¥ë¡¼¥× | Âç³Ø±¡À¸¡Ê½¤»Î£±Ç¯¡Ë | x | - |
| µÜËÜ¡¡ÍµÊ¿ | ÅìµþÂç³ØÂç³Ø±¡Íý³Ø·Ï¸¦µæ²ÊÉí°¥Ó¥Ã¥°¥Ð¥ó±§Ãè¹ñºÝ¸¦µæ¥»¥ó¥¿¡¼ | Âç³Ø±¡À¸¡ÊM2¡Ë | x | - |
| Ô¢¸÷ ÂÀϺ | ÅìµþÂç³ØÂç³Ø±¡Íý³Ø·Ï¸¦µæ²ÊÉí°¥Ó¥Ã¥°¥Ð¥ó±§Ãè¹ñºÝ¸¦µæ¥»¥ó¥¿¡¼ | Âç³Ø±¡À¸¡ÊM1¡Ë | x | - |
| Ãæ´Ö ÃÒ¹° | ÅìµþÂç³ØÂç³Ø±¡Íý³Ø·Ï¸¦µæ²ÊÉí°¥Ó¥Ã¥°¥Ð¥ó±§Ãè¹ñºÝ¸¦µæ¥»¥ó¥¿¡¼ | Âç³Ø±¡À¸¡ÊM1¡Ë | x | - |
| ÅçÂÞÈ»»Î | ̾¸Å²°Âç³ØÍý³Ø¸¦µæ²Ê¡¡ÍýÏÀÅ·ÂÎʪÍý³Ø¶µ¼¼¡ÊAt¸¦¡Ë | Âç³Ø±¡À¸¡ÊM1¡Ë | x | - |
| °ÂÉð ¿½Ó | ÅìµþÂç³Ø¡¡RESCEU | PD | °ìÈÌ | Matter effects on thermal evolutions of compact stars |
| Àж¶¡¡²Â | Åìµþ¹©¶ÈÂç³ØÍý¹©³Ø¸¦µæ²Ê¡¡±§ÃèÍýÏÀ¸¦µæ¼¼ | Âç³Ø±¡À¸¡ÊM1¡Ë | x | - |
| Sungwook E. Hong | KAIST | PD | °ìÈÌ | Anthropic Likelihood for Lambda and Q using History of Milky Way and Local Group |
| ¾®ÎÓ¡¡ÎÌÊ¿ | ̾¸Å²°Âç³ØÍý³Ø¸¦µæ²Ê¡¡ÍýÏÀÅ·ÂÎʪÍý³Ø¸¦µæ¼¼ | Âç³Ø±¡À¸¡ÊM2¡Ë | x | - |
| ¹â¿å¡¡Íµ°ì | Áá°ðÅÄÂç³ØÍý¹©³Ø½Ñ±¡¡¡ | ½õ¶µ | °ìÈÌ | Beyond delta-N formalism for multi-scalar system |
| ¸ÍÊÕ¡¡¹°Î¼ | Åìµþ¹©¶ÈÂç³ØÍý¹©³Ø¸¦µæ²Ê¡¡±§ÃèÍýÏÀ¸¦µæ¼¼ | Âç³Ø±¡À¸¡ÊM1¡Ë | x | - |
| ʲϡ¡½ÓÌï | ÅìµþÂç³ØÍý³ØÉô ±§ÃèÍýÏÀ¸¦µæ¼¼ | Âç³Ø±¡À¸¡ÊD2¡Ë | °ìÈÌ | Reconstruction of Cosmic Magnification from Gravitational-Wave Standard Sirens |
| î²ÈÆÆ»Ë | ÅìµþÂç³ØÂç³Ø±¡Íý³Ø·Ï¸¦µæ²Ê Éí°¥Ó¥Ã¥°¥Ð¥ó±§Ãè¹ñºÝ¸¦µæ¥»¥ó¥¿¡¼ | ½õ¶µ | °ìÈÌ | RegPTfast: a fast computation of nonlinear power spectrum from perturbation theory |
| Ê¡±Ê¡¡·ò²ð | ÅìµþÂç³ØÍý³ØÉô ±§ÃèÍýÏÀ¸¦µæ¼¼ | Âç³Ø±¡À¸¡ÊD1¡Ë | x | - |
| ÌÚ¼¡¡ÍöÊ¿ | ¹ÅçÂç³ØÍý³Ø¸¦µæ²Ê¡¡±§ÃèʪÍý³Ø¸¦µæ¼¼ | Âç³Ø±¡À¸¡ÊD1¡Ë | °ìÈÌ | Large Scale Structures in Kinetic Gravity Braiding Model and Observational Implications |
| ·§ºê¡¡ÏËÊ¿ | ̾¸Å²°Âç³ØÍý³Ø¸¦µæ²Ê¡¡ÍýÏÀÅ·ÂÎʪÍý³Ø¸¦µæ¼¼ | Âç³Ø±¡À¸¡ÊM2¡Ë | x | - |
| µÜËÜ¡¡¹¬°ì | ÅìµþÂç³ØÍý³Ø·Ï¸¦µæ²ÊʪÍý³ØÀì¹¶¡¡±§ÃèÀþ¸¦µæ½ê | Âç³Ø±¡À¸¡ÊÇî»Î£²Ç¯¡Ë | °ìÈÌ | Cosmological effects of decaying cosmic string loops with TeV scale width |
| »³Æâ¡¡Âç²ð | ÅìµþÂç³Ø¡¡±§ÃèÀþ¸¦µæ½ê | PD | °ìÈÌ | Weak lensing of CMB from cosmic (super-)strings |
| À¾Æ» ·¼Çî | ÅìµþÂç³Ø¿ôʪϢ·È±§Ã踦µæµ¡¹½ | PD | °ìÈÌ | accurate modeling of the redshift-space distortions of biased tracers |
| ã·Àî ¸°ì | ÅìµþÂç³Ø±§ÃèÀþ¸¦µæ½ê¡¡ÍýÏÀ¥°¥ë¡¼¥× | Âç³Ø±¡À¸¡ÊD2¡Ë | °ìÈÌ | Axion cosmology and domain walls |
| ¹õúË ¹¬»Ò | ÅìµþÂç³Ø¡¡±§ÃèÀþ¸¦µæ½ê | PD | °ìÈÌ | Higher order corrections to the power-law form of the primordial tensor spectrum |
| Vennin | Institut d'Astrophysique de Paris | Graduate Student¡Ê1st year of PhD¡Ë | °ìÈÌ | Numerical approach to the inflationary Langevin equation |
| ¾®ÎÓ¡¡ÌÀÈþ | ̾¸Å²°Âç³ØÍý³Ø¸¦µæ²Ê¡¡ÍýÏÀÅ·ÂÎʪÍý³Ø¸¦µæ¼¼ | Âç³Ø±¡À¸¡ÊM£±¡Ë | x | - |
| ¾¾ÅÄ¡¡¹¯ | ̾¸Å²°Âç³ØÍý³ØÉô¡¡±§ÃèÍýÏÀ¸¦µæ¼¼ | Âç³Ø±¡À¸¡ÊM1¡Ë | x | - |
| Æ£ÅÄ¡¡ÃÒ¹° | ¿ôʪϢ·È±§Ã踦µæµ¡¹½ | Âç³Ø±¡À¸¡Ê½¤»Î£²Ç¯¡Ë | x | - |
| ËÌÅ衡ľÌï | ÅìµþÂç³ØÍý³Ø·Ï¸¦µæ²Ê¡¡±§ÃèÀþ¸¦µæ½ê | Âç³Ø±¡À¸¡ÊÇî»Î²ÝÄø£±Ç¯¡Ë | °ìÈÌ | Inflation in a supersymmetric axion model |
| ËÒÅç°ìÉ× | ÅìµþÂç³ØÍý³Ø·Ï¸¦µæ²ÊʪÍý³ØÀì¹¶ | ¶µ¼ø | ¥×¥í | ¡Ö¤¹¤¶¤¯¡×¡¢MAXI¡¢ASTRO-H |
| ÄÚÌî ¸øÉ× | ÅìµþÂç³ØÍý³Ø·Ï¸¦µæ²Ê | ¶µ¼ø | ¥×¥í | LCGT,DECIGO,DPF |
| ²£»³½ç°ì | ÅìµþÂç³Ø¥Ó¥Ã¥°¥Ð¥ó±§Ãè¹ñºÝ¸¦µæ¥»¥ó¥¿¡¼ | ¶µ¼ø | ¥×¥í | Temporal enhancement and decay of superhorizon curvature fluctuations |
| Ê¿¾¾ ¾°»Ö | µþÅÔÂç³Ø¡¡´ðÁÃʪÍý³Ø¸¦µæ½ê | ½õ¶µ | °ìÈÌ | A head-on approach to structure formation |
| Âçëͧ¹áÍý | ÅìµþÂç³ØÂç³Ø±¡Íý³Ø·Ï¸¦µæ²ÊÉÕ°¥Ó¥Ã¥°¥Ð¥ó±§Ãè¹ñºÝ¸¦µæ¥»¥ó¥¿¡¼ | Âç³Ø±¡À¸¡ÊM2¡Ë | x | - |
| ÎëÌÚ Î´Ç· | »³¸ýÂç³ØÂç³Ø±¡Íý¹©³Ø¸¦µæ²Ê(Íý³Ø·Ï)¡¡ÁÇγ»ÒÍýÏÀ±§ÃèÏÀÇòÀи¦µæ¼¼ | Âç³Ø±¡À¸¡ÊÇî»Î¸å´ü²ÝÄø3ǯ¡Ë | °ìÈÌ | ½¤Àµ½ÅÎϱ§Ãè¥â¥Ç¥ë¤Ë±÷¤±¤ë±§Ãè¤Î¹½Â¤·ÁÀ®¥·¥ß¥å¥ì¡¼¥·¥ç¥ó |
| ÀÄ»³¡¡¾°Ê¿ | ̾¸Å²°Âç³ØÂç³Ø±¡Íý³Ø¸¦µæ²ÊÁÇγ»Ò±§ÃèʪÍý³ØÀì¹¶ÍýÏÀÅ·ÂÎʪÍý³Ø¸¦µæ¼¼[AT¸¦] | Âç³Ø±¡À¸¡Ê½¤»Î2ǯ¡Ë | °ìÈÌ | Decaying dark matter models withfinite mass daughter particles |
| Michael Kotson | ÅìµþÂç³ØÍý³ØÉô ±§ÃèÍýÏÀ¸¦µæ¼¼ / MIT | ¤½¤Î¾¡Ê³ØÉôÀ¸¡Ë | x | - |
| ã·Æ£¡¡Î¼ | ̾¸Å²°Âç³ØÍý³Ø¸¦µæ²Ê¡¡ÁÇγ»ÒÏÀŪ±§ÃèÏÀ¸¦µæ¼¼ | Âç³Ø±¡À¸¡ÊD1¡Ë | °ìÈÌ | The unification of inflation and late-time acceleration in the frame of k-essence |
| ÌÚëÂÀ°ì | ¥Ý¡¼¥Ä¥Þ¥¹Âç³Ø¡¢±§ÃèÏÀ½ÅÎÏÍýÏÀ¸¦µæ½ê | Âç³Ø±¡À¸¡Ê£Ä£±¡Ë | x | - |
| Ìл³ ½ÓÏ | ÅìµþÂç³ØÍý³Ø·Ï¸¦µæ²ÊÉí°¥Ó¥Ã¥°¥Ð¥ó±§Ãè¹ñºÝ¸¦µæ¥»¥ó¥¿¡¼ | ½Ú¶µ¼ø | ¥×¥í | ÌÀ¤ë¤¤Ia·¿Ä¶¿·À±¤Îµ¯¸» |
| À¥¸Í ľ¼ù | µþÅÔÂç³Ø Íý³ØÉô ʪÍý | ½õ¶µ | x | - |
| Chung-Chi Lee | National Tsing Hua University, Taiwan | Graduate Student¡Ê2nd year¡Ë | °ìÈÌ | Phantom Crossing in Modified Gravity Theories |
| Yi-Peng Wu | Dept. of Phys, National Tsing Hua University | Graduate Student¡Ê1 st¡Ë | x | - |
| Ling-Wei Luo | Department of Physics, National Tsing Hua University | Graduate Student¡Ê2nd year of PhD¡Ë | °ìÈÌ | Observational Constraints on Exponential Gravity |
| º´Æ£¡¡ÀµÅµ | ̾¸Å²°Âç³Ø¡¡ÍýÏÀÅ·ÂÎʪÍý³Ø¸¦µæ¼¼ | Âç³Ø±¡À¸¡ÊD2¡Ë | °ìÈÌ | Nonlinear Biasing and Redshift-Space Distortions in Lagrangian Resummation Theory and N-body Simulations |
| ²ÏÌî¹§ÂÀϺ | ÅìµþÂç³ØÂç³Ø±¡Íý³Ø·Ï¸¦µæ²ÊÉí°ŷʸ³Ø¶µ°é¸¦µæ¥»¥ó¥¿¡¼ | ¶µ¼ø | ¥×¥í | ¥µ¥Ö¥ß¥êÇȡʶä²Ï¡Ë |
| À¾ß· ÆÆ»Ö | µþÅÔÂç³Ø´ðÁÃʪÍý³Ø¸¦µæ½ê | PD | °ìÈÌ | Gravitational-wave standard siren |
| Nikolai Meures | ICG, University of Portsmouth | Graduate Student¡Ê2nd year¡Ë | °ìÈÌ | Light Propagation through exact non-linear inhomogeneities in LCDM cosmology |
| Nicolas Van de Rijt | CEA/Saclay | Graduate Student¡Ê2nd year¡Ë | °ìÈÌ | Multi-fluid renormalized perturbation theory and massive neutrinos |
| µÈ¼ ¹À»Ê | ¹â¥¨¥Í¥ë¥®¡¼²Ã®´ï¸¦µæµ¡¹½¡¦ÁÇγ»Ò¸¶»Ò³Ë¸¦µæ½ê | ½Ú¶µ¼ø | ¥×¥í | BESS-Polar¼Â¸³¡¦À®²ÌÊó¹ð |
| Borchers, Florian Wolfgang | Lecospa, NTU, Taiwan | Graduate Student¡Ê1st year¡Ë | x | - |
| ±ÊÌî¡¡ÁáÉ´¹ç | RESCEU | ¤½¤Î¾¡Ê¡Ë | x | - |
| LEE YOJU | µþÅÔÂç³ØÍý³Ø¸¦µæ²ÊʪÍýÂè°ì¶µ¼¼ÈóÀþ·ÁÈóÊ¿¹Õ¸¦µæ¼¼ | Âç³Ø±¡À¸¡Ê½¤»Î£²Ç¯¡Ë | x | - |
| ¾¾ËÜ Ï©Ï¯ | ̾¸Å²°Âç³ØÂç³Ø±¡Íý³Ø¸¦µæ²Ê Q¸¦ | Âç³Ø±¡À¸¡ÊD2¡Ë | °ìÈÌ | Necessity of revisions for the cosmological matter perturbations from general relativity |
| °æ¾å ·Ä½ã | ÅìµþÂç³ØÁÇγ»ÒʪÍý¹ñºÝ¸¦µæ¥»¥ó¥¿¡¼ | ½õ¶µ | ¥×¥í | Tokyo axion helioscope |
| Åèºî°ìÂç | ÅìµþÂç³ØÍý³ØÉôŷʸ³Ø¶µ¼¼ | ½Ú¶µ¼ø | ¥×¥í | ¥×¥í¥¸¥§¥¯¥ÈÊó¹ð |
| »³Åĵü | ÅìËÌÂç³Ø¡¡Âç³Ø±¡Íý³Ø¸¦µæ²Ê | ¶µ¼ø | °ìÈÌ | ¹âÀÖÊýÊаܱ§Ãè¤Ç¤Ë¤ª¤±¤ë¶ä²Ï´Ñ¬ |
| Roy Maartens | University of Portsmouth | ¶µ¼ø | °ìÈÌ | Theoretical models for the accelerating universe |
| Shirley Ho | UC Berkeley | °ìÈÌ | Large scale structure of the Universe | |
| Alexei Starobinsky | Landau Institute | ¶µ¼ø | °ìÈÌ | TBA |