RESCEU/DENET ¥µ¥Þ¡¼¥¹¥¯¡¼¥ë »²²Ã¼Ô¥ê¥¹¥È

Notice: Undefined variable: totnum in /var/www/vhosts/resceu.s.u-tokyo.ac.jp/httpdocs/workshops/resceu11s/list.php on line 64

Notice: Undefined variable: accnum in /var/www/vhosts/resceu.s.u-tokyo.ac.jp/httpdocs/workshops/resceu11s/list.php on line 93
¸½ºß¡¢69̾¤ÎÊý¤¬ÅÐÏ¿¤µ¤ì¤Æ¤¤¤Þ¤¹¡£
»á̾ ½ê° ¿Èʬ ¹Ö±é¿½¹þ ¥¿¥¤¥È¥ë
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¸¦µæ²ÊʪÍý³ØÀ칶¡¡±§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¸¦µæ²ÊʪÍý³ØÀ칶 ¶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±§ÃèʪÍý³ØÀ칶ÍýÏÀÅ·ÂÎʪÍý³Ø¸¦µæ¼¼[AT¸¦] Âç³Ø±¡À¸¡Ê½¤»Î2ǯ¡Ë °ìÈÌ Decaying dark matter models with finite 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
²ÏÌ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