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¾®ÎÓ Þ« | ÅìµþÂç³Ø RESCEU | PD | °ìÈÌ | Non-Gaussianity from Curvatons Revisited |
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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 |
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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 |