＜＜＜「@」を「__AT__」に置き換えています＞＞＞ Date: Thu, 4 Dec 2014 14:31:08 +0900 From: Kazunori Kohri To: sg-l__AT__yukawa.kyoto-u.ac.jp, jgrg__AT__astro.sc.niigata-u.ac.jp, tennet__AT__asj.or.jp Subject: [Sg-l:789] Fwd: [rironkon:00583] Workshop on B-mode Cosmology : announcement 皆さま、 重複して受け取られる方々には、ご迷惑をおかけいたします。 ２月下旬にKEKで開かれる、インフレーション宇宙論に関する国際ワークショップの案内\ を転送いたします。 "B-mode Cosmology - Intermediate Scale Inflation and Hidden Sector -" 郡　和範 (KEK) ---------- Forwarded message ---------- From: Hideo Kodama 皆さま ２０１５年２月１９日（木）〜２１日（土）に，KEK理論センターにおいて下記のワークショップを開催します．ふるってご参加下さい． 参加登録および講演申し込みは，近日中に開設するホームページよりお願いします．準備ができ次第お知らせします． KEK理論センター 小玉英雄 ------------------------------------------------------------------------------- KEK-CPWS The 4th UTQuest Workshop B-mode Cosmology - Intermediate Scale Inflation and Hidden Sector - 19 - 21 February 2015 KEK, Tsukuba, Japan >Aim The recent unexpected result of BICEP2 has provoked tremendous interests in high scale inflation models, and lots of new ideas have been proposed within less than a year. This new development, however, rather seems to have made clear how difficult it is to construct a natural high scale model on the basis of a candidate of ultimate theory, such as superstring theory. This circumstance together with the issue on the foreground emission from dust strongly indicates the importance of thorough investigations of intermediate scale models that predict values of the tensor-scalar ratio in the range 0.01>r> 0.0001. In this workshop, we overview the present status of high and intermediate scale inflation models and discuss how to discriminate such models by various near future experiments including CMB B-mode measurements, taking account of the new results by Planck to be published in the form of paper by the end of January 2015. We particularly focus on the relevance of hidden sector physics such as string axions to intermediate scale inflation. The workshop will consist of invited review talks and contributed talks. Sufficient time will be spared for discussions. >Topics to be discussed CMB B-mode observation experiments Various sources of B-modes Inflation models Non-gaussianity Moduli problems Axions and hidden sector particles/fields Cosmological gravitational waves >Invited talks (* to be confirmed) *Adrian Lee (POLARBEAR/UC Berkeley) TBA (Present status of the ground-based CMB experiments) *An experimentalist on CMB TBA (Satellite CMB experiments) Kazunori Korhi (KEK) "New results of the Planck B-mode measurements - Report of the Planck2014 and the Paris conference" Fuminobu Takahashi (Tohoku U.) TBA (Overview of high and intermediate scale inflation models) Xingang Chen (Texas U, Dallas) TBA (Constraints on inflation models from CMB B-mode and non-gaussianity) Michele Cicoli (ICTP) TBA (String inspired inflation models and moduli problem) Masahiro Kawasaki (ICRR) TBA ( Axion constraints on inflation) Tatsuo Kobayashi (Hokkaido U) TBA (Inflation scale and string phenomenology) Jiro Soda (Kobe U) TBA (Inflation models with vector/form fields and observational consequences) Kazunori Nakayama (U. Tokyo) TBA (Probing inflation by GWs) >SOC Masashi Hazumi (KEK), Tetsutaro Higaki (KEK), Kunihito Ioka (KEK), Tatsuo Kobayashi (Hokkaido U.), Hideo Kodama (KEK, Chair), Kazunori Kohri (KEK), Shun'ya Mizoguchi (KEK), Kazunori Nakayama (U. Tokyo), Jiro Soda (Kobe U.), Yoske Sumitomo (KEK), Fuminobu Takahashi (Tohoku U.), Hirotaka Yoshino (KEK) >Sponsor This workshop is supported by the JSPS Grant-in-Aid for Scientific Research (A) 26247042　" Quest for the Ultimate Theory in terms of rich cosmophysical phenomena caused by fields and particles in the hidden sector"． *********************************************************** Hideo KODAMA http://cosmophysics.kek.jp/ Cosmophysics Group, Theory Center Institute of Particle and Nuclear Studies KEK (High Energy Accelerator Research Organization) 1-1 Oho, Tsukuba 305-0801, Japan Email: Hideo.Kodama__AT__kek.jp Phone: +81-29-864-5407 Fax: +81-29-864-5755 *********************************************************** %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% Date: Tue, 23 Dec 2014 20:02:53 +0900 From: Kazunori Kohri To: sg-l__AT__yukawa.kyoto-u.ac.jp, tennet__AT__asj.or.jp, jgrg__AT__astro.sc.niigata-u.ac.jp Subject: [Sg-l:828] Fwd: [rironkon:00606] Workshop on B-mode Cosmology: 1st Circular & homepage 皆さま、 重複して受け取られる方にはご迷惑をおかけいたします。 KEKで開かれるワークショップ"B-mode Cosmology" の案内を転送いたします。 郡 和範 (KEK) ---------- Forwarded message ---------- From: Hideo Kodama Date: 2014-12-23 18:49 GMT+09:00 Subject: [rironkon:00606] Workshop on B-mode Cosmology: 1st Circular & homepage To: rironkon__AT__rironkon.jp 皆さま すでにアナウンスしましたように，2015年2月19日〜21日にKEK小林ホールで国際ワークショップ B-\ mode Cosmologyを開催します．ワークショップの概要については，以下の1st Circularをご覧下さい． 参加を希望される方は，ワークショップホームページ http://research.kek.jp/people/hkodama/UTQuestWS4/ のRegistrationページより参加登録をお願いします．また，一般講演・ポスター発表を受け付けま\\ すので，希望される方は参加登録の際に発表に関する情報を登録して下さい． ＊重要な締め切り＊ 　　旅費補助申し込み: January 23 (Fri), 2015 (銀行口座振り込みのみ) 　　参加登録:　　　　　　 January 31 (Sat), 2015 　　講演・発表申し込み: January 31 (Sat), 2015 　　バンケット申し込み: January 31 (Sat), 2015 小玉英雄 ==================================================================== 1st Circular KEK-CPWS The 4th UTQuest Workshop B-mode Cosmology — Intermediate Scale Inflation and Hidden Sector — 19 — 21 February 2015 KEK, Tsukuba, Japan http://research.kek.jp/people/hkodama/UTQuestWS4/ Please register through the above web page immediately!! Important Deadlines ・Financial Support: January 23, 2015 (post remittance to a domestic bank account only) ・Registration: January 31, 2015 ・Abstract Submission: January 31, 2015 ・Banquet application: January 31, 2015 Aim 　The recent unexpected result of BICEP2 has provoked tremendous interests in high scale inflation models, and lots of new ideas have been proposed within less than a year. This new development, however, rather seems to have made clear how difficult it is to construct a natural high scale model on the basis of a candidate of ultimate theory, such as superstring theory. This circumstance together with the issue on the foreground emission from dust strongly indicates the importance of thorough investigations of intermediate scale models that predict values of the tensor-scalar ratio in the range 0.01>r> 0.0001. 　 In this workshop, we overview the present status of high and intermediate scale inflation models and discuss how to discriminate such models by various near future experiments including CMB B-mode measurements, taking account of the new results by Planck to be published in the form of paper by the end of January 2015. We particularly focus on the relevance of hidden sector physics such as string axions to intermediate scale inflation. The workshop will consist of invited review talks and contributed talks. Sufficient time will be spared for discussions. Topics to be discussed ・CMB B-mode observation experiments ・Various sources of B-modes ・Inflation models ・Non-gaussianity ・Moduli problems ・Axions and hidden sector particles/fields ・Cosmological gravitational waves Invited speakers ・Adrian Lee (POLARBEAR/UC Berkeley) 　　 TBA (Present status of the ground-based CMB experiments) ・Carlo Baccigalupi (Planck/SISSA) 　　 TBA (Foreground subtraction, bispectrum) ・Kazunori Korhi (KEK) 　　 “Large and small field conformal inflation models, including reports 　　　of the Planck2014 and the Paris conference” ・Fuminobu Takahashi (Tohoku U.) 　　 TBA (Overview of high and intermediate scale inflation models) ・Xingang Chen (Texas U, Dallas) 　　 TBA (Constraints on inflation models from CMB B-mode and non-gaussianity) ・Michele Cicoli (ICTP) 　　 TBA (String inspired inflation models and moduli problem) ・Masahiro Kawasaki (ICRR) 　　 TBA ( Axion constraints on inflation) ・Tatsuo Kobayashi (Hokkaido U) 　　 TBA (Inflation scale and string phenomenology) ・Gary Shiu (Wisconsin U/HKUST) 　　 TBA ・Jiro Soda (Kobe U) 　　 TBA (Inflation models with vector/form fields and observational consequences) ・Kazunori Nakayama (U. Tokyo) 　　 TBA (Probing inflation by GWs) Registration Fee 　 The registration fee is 5,000 yen. It will be collected at the registration desk. Financial Supports 　 We will be able to support the expenses of the domestic travel and the accommodation in the KEK dormitory for all participants. Note that we can only provide the dormitory-rate-equivalent even if you stay at a hotel, except for invited participants. You can apply for the financial support when you make the online registration. The financial support will be remitted to your domestic bank account after the workshop. Reception and Banquet 　 A reception and a banquet will be held on the 1st and 2nd nights, respectively. All participants are invited to the reception party on 2/19 at the salon in front of the Kobayashi Hall. 　 If you would like to participate in the banquet on 2/20, please apply at the online registration. The banquet fee is 5,000 yen and will be collected at the registration desk. The banquet will be held at a restaurant outside the KEK SOC Masashi Hazumi (KEK), Tetsutaro Higaki (KEK), Kunihito Ioka (KEK), Tatsuo Kobayashi (Hokkaido U.), Hideo Kodama (KEK, Chair), Kazunori Kohri (KEK), Shun'ya Mizoguchi (KEK), Kazunori Nakayama (U. Tokyo), Jiro Soda (Kobe U.), Yoske Sumitomo (KEK), Fuminobu Takahashi (Tohoku U.), Hirotaka Yoshino (KEK) Sponsor 　 This workshop is supported by the Theory Centre of KEK and the JSPS Grant-in-Aid for Scientific Research (A) 26247042　” Quest for the Ultimate Theory in terms of rich cosmophysical phenomena caused by fields and particles in the hidden sector”． ================================================================= *********************************************************** Hideo KODAMA http://cosmophysics.kek.jp/ Cosmophysics Group, Theory Center Institute of Particle and Nuclear Studies KEK (High Energy Accelerator Research Organization) 1-1 Oho, Tsukuba 305-0801, Japan Email: Hideo.Kodama__AT__kek.jp Phone: +81-29-864-5407 Fax: +81-29-864-5755 *********************************************************** %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% Date: Thu, 15 Jan 2015 15:46:34 +0900 From: Kazunori Kohri To: tennet__AT__asj.or.jp, sg-l__AT__yukawa.kyoto-u.ac.jp, jgrg__AT__astro.sc.niigata-u.ac.jp Subject: [Sg-l:866] Reminder: Workshop on B-mode Cosmology 皆さま 国際ワークショップ "B-mode Cosmology"の案内を転送いたします。 郡 (KEK) ---------- Forwarded message ---------- From: Hideo Kodama Date: 2015-01-15 14:19 GMT+09:00 皆さま 2015年2月19日〜21日にKEK小林ホールで国際ワークショップ B-mode Cosmologyを開催します． http://research.kek.jp/people/hkodama/UTQuestWS4/ 旅費補助の申し込み期限があと一週間程度に迫ってきました．旅費補助を希望される方はできるだけ早い時期に参加登録をお願いします． 一般講演の枠もまだ十分ありますので，ふるっての参加・講演の申し込みをお待ちしています． ＊重要な締め切り＊ 　　旅費補助申し込み: January 23 (Fri), 2015 (銀行口座振り込みのみ) 　　参加登録:　　　　　　 January 31 (Sat), 2015 　　講演・発表申し込み: January 31 (Sat), 2015 　　バンケット申し込み: January 31 (Sat), 2015 小玉英雄 ==================================================================== KEK-CPWS The 4th UTQuest Workshop B-mode Cosmology — Intermediate Scale Inflation and Hidden Sector — 19 — 21 February 2015 KEK, Tsukuba, Japan http://research.kek.jp/people/hkodama/UTQuestWS4/ Please register through the above web page immediately!! Aim 　The recent unexpected result of BICEP2 has provoked tremendous interests in high scale inflation models, and lots of new ideas have been proposed within less than a year. This new development, however, rather seems to have made clear how difficult it is to construct a natural high scale model on the basis of a candidate of ultimate theory, such as superstring theory. This circumstance together with the issue on the foreground emission from dust strongly indicates the importance of thorough investigations of intermediate scale models that predict values of the tensor-scalar ratio in the range 0.01>r> 0.0001. 　 In this workshop, we overview the present status of high and intermediate scale inflation models and discuss how to discriminate such models by various near future experiments including CMB B-mode measurements, taking account of the new results by Planck to be published in the form of paper by the end of January 2015. We particularly focus on the relevance of hidden sector physics such as string axions to intermediate scale inflation. The workshop will consist of invited review talks and contributed talks. Sufficient time will be spared for discussions. Topics to be discussed ・CMB B-mode observation experiments ・Various sources of B-modes ・Inflation models ・Non-gaussianity ・Moduli problems ・Axions and hidden sector particles/fields ・Cosmological gravitational waves Invited speakers ・Adrian Lee (POLARBEAR/UC Berkeley) 　　 TBA (Ground-based CMB experiments) ・Carlo Baccigalupi (Planck/SISSA) 　　 TBA (Foreground subtraction, bispectrum) ・Kazunori Korhi (KEK) 　　 “Large and small field conformal inflation models, including reports 　　　of the Planck2014 and the Paris conference” ・Fuminobu Takahashi (Tohoku U.) 　　 ”High and intermediate-scale inflation” ・Xingang Chen (Texas U, Dallas) 　　 TBA (Non-gaussianity) ・Michele Cicoli (U Bologna) 　　 "Pre- and Post-inflationary string cosmology" ・Masahiro Kawasaki (ICRR) 　　TBA (Axion cosmology) ・Tatsuo Kobayashi (Hokkaido U) 　　 TBA (Inflation scale and string phenomenology) ・Gary Shiu (Wisconsin U/HKUST) 　　 TBA ・Jiro Soda (Kobe U) 　　 "Impact of form fields on primordial gravitational waves" ・Kazunori Nakayama (U. Tokyo) 　　 "Inflationary gravitational waves as a probe of the early universe" Registration Fee 　 The registration fee is 5,000 yen. It will be collected at the registration desk. Financial Supports 　 We will be able to support the expenses of the domestic travel and the accommodation in the KEK dormitory for all participants. Note that we can only provide the dormitory-rate-equivalent even if you stay at a hotel, except for invited participants. You can apply for the financial support when you make the online registration. The financial support will be remitted to your domestic bank account after the workshop. Reception and Banquet 　 A reception and a banquet will be held on the 1st and 2nd nights, respectively. All participants are invited to the reception party on 2/19 at the salon in front of the Kobayashi Hall. 　 If you would like to participate in the banquet on 2/20, please apply at the online registration. The banquet fee is 5,000 yen and will be collected at the registration desk. The banquet will be held at a restaurant outside the KEK SOC Masashi Hazumi (KEK), Tetsutaro Higaki (KEK), Kunihito Ioka (KEK), Tatsuo Kobayashi (Hokkaido U.), Hideo Kodama (KEK, Chair), Kazunori Kohri (KEK), Shun'ya Mizoguchi (KEK), Kazunori Nakayama (U. Tokyo), Jiro Soda (Kobe U.), Yoske Sumitomo (KEK), Fuminobu Takahashi (Tohoku U.), Hirotaka Yoshino (KEK) Sponsor 　 This workshop is supported by the Theory Centre of KEK and the JSPS Grant-in-Aid for Scientific Research (A) 26247042　” Quest for the Ultimate Theory in terms of rich cosmophysical phenomena caused by fields and particles in the hidden sector”． ================================================================= *********************************************************** Hideo KODAMA http://cosmophysics.kek.jp/ Cosmophysics Group, Theory Center Institute of Particle and Nuclear Studies KEK (High Energy Accelerator Research Organization) 1-1 Oho, Tsukuba 305-0801, Japan Email: Hideo.Kodama__AT__kek.jp Phone: +81-29-864-5407 Fax: +81-29-864-5755 ***********************************************************