Previous Schedule: 1998 1999 2000 2001 2002 2003 2004 2005 2006 2007 2008 2009 2010 2011 2012 2013 2014 2015 2016 2017 2018
2019
December 16–19
International conference on “B-mode from Space” at MPA
December 12
Perspektivenkommission, Berlin-Dahlem
December 6
Universität Bonn
November 12–14
Fachbeirat, MPA
October 24,25
Sektionssitzung, Berlin-Dahlem
October 9–12
Universität Bonn
- 10/9: MUC()-CGN()
- 10/11: Plücker-Lecture
- 10/12: CGN()-MUC()
September 24
Astrophysics Seminar at Département d’Astrophysique, CEA Saclay
September 20
Perspektivenkommission, Berlin-Dahlem
September 13
Barcelona
September 6
Universität zu Köln for 「第4回ドイツ物理学・応用物理学セミナー」
September 2–6
COSMO-19, RWTH Aachen
July 26–August 11
Urlaub! No laptop, no email
- 7/26: MUC(11:05)-HEL(14:35)
- 8/1: HEL(15:20)-MUC(16:50)
July 23
Perspektivenkommission, München
June 11–July 19
SISSA, Trieste
May 27
Cambridge [unless Brexit goes wild]
May 23,24
MPIfR
- 5/23: MUC()-CGN()
- 5/24: Give a colloquium on “Finding Cosmic Inflation”
- Abstract: The cosmic microwave background (CMB) research told us a remarkable story: the structure we see in our Universe such as galaxies, stars, planets, and eventually ourselves originated from tiny quantum fluctuations generated in the early Universe. With the WMAP we have confirmed many of the key predictions of inflation including flatness and statistical homogeneity of our Universe, Gaussianity and adiabaticity of primordial density fluctuations, and a small but non-zero deviation from the scale-invariant spectrum of density fluctuations. Yet, the extraordinary claim requires extraordinary evidence. The last prediction of inflation that is yet to be confirmed is the existence of primordial gravitational waves whose wavelength can be as big as billions of light years. To this end we have proposed to JAXA a new satellite mission called LiteBIRD, whose primary scientific goal is to find signatures of gravitational waves in the polarisation of the CMB. In this presentation we describe the current state of affairs regarding our understanding of the early Universe, physics of polarisation of CMB, the LiteBIRD proposal, as well as a sub-mm telescope in Chile called CCAT-p that we are currently building.
- CGN()-MUC()
May 20
Astro-NFDI discussion, AIP, Potsdam [10:00-17:00]
May 15,16
Editorial Board Meeting of AARv, Heidelberg
May 14
Perspektivenkommission, Berlin-Dahlem
May 10
“Working Culture and Working Atmosphere in the Max Planck Society” Task Force meeting at Harnack Haus, Berlin-Dahlem [10:00-13:00]
May 8
Friedrich-Alexander-Universität Erlangen-Nürnberg
March 26–April 24
Kavli IPMU, Kashiwa, Japan
- 3/26-27: MUC(20:00)-HND(15:40)
- 3/30: 講演会「宇宙の始まり、そして終わり〜HORIZON 宇宙の果てにあるもの〜」, 多摩六都科学館 [17:10-19:40]
- 4/17: 講演会, 日本建築家協会(JIA)トーク [18:30-20:30]
- 4/18: Colloquium on “Non-Gaussian Gravitational Waves from Inflation” [16:00-17:00] at RESCEU, the Univ. of Tokyo
- 4/20: 科学ライブショー「ユニバース」, 科学技術館
- [1回目, 特別番組] 13:30-15:00; [2回目, 通常ライブショー] 15:30-16:10
- 4/23: APEC Seminar, Kavli IPMU [12:00-13:00]
- 4/23: キャリアパス・セミナー, Kavli IPMU [13:15-15:00]
- 4/24: HND(12:30)-MUC(17:20)
March 21,22
LiteBIRD Europe Collaboration Meeting (9:00 March 21 to 17:00 March 22)
March 20
Perspektivenkommission, Berlin-Dahlem
- 3/20: MUC(8:00)-TXL(9:10); TXL(18:30)-MUC(19:40)
March 1-9
Kyoto
- 3/1-2: MUC(15:30)-HND-ITM(14:05)
- 3/3-4: 新学術領域シンポジウム, Yukawa Institute, Kyoto University
- 3/4: D01 Update (10:45-11:15)
- 3/4-8: Symposium on “Accelerating Universe in the Dark”, Yukawa Institute, Kyoto University
- 3/9: ITM(10:00)-HND-MUC(16:45)
February 21,22
Sektionssitzung, Berlin-Dahlem
- 2/21: MUC(7:45)-TXL(8:55)
- 2/22: TXL(14:30)-MUC(15:40)
February 11
ESO Knowledge Exchange on CMB [10:45-11:45]
February 9
ミュンヘン日本語補習校で講演「僕は天文学者」（14:00-15:30）
January 31
Colloquium at Institute of Cosmology and Gravitation (ICG), Univ. of Portsmouth
- 1/30: MUC(9:40)-LGW(10:45); Gatwick Airport(11:39)-Portsmouth&Southsea(13:01)
- 1/31: Give a colloquium on “Non-Gaussian gravitational waves from inflation” [14:30-15:30]
- Abstract: It has been widely assumed that detection of primordial gravitational waves from inflation in, for example, B-mode polarisation of the cosmic microwave background, immediately implies discovery of the quantum nature of spacetime. While this statement is true for the vacuum solution, it does not apply if the gravitational waves originate from the matter fields. How can we distinguish between these two origins? The answer is non-Gaussinaity. We show that the gravitational waves from SU(2) gauge fields coupled to a spectator axion field during inflation are highly non-Gaussian with a characteristic shape, whereas those from the vacuum are only weakly non-Gaussian.
- 2/1: Portsmouth&Southsea(10:15)-Gatwick Airport(11:38); LGW(13:35)-MUC(16:30)
Canceled due to illness. Not a great start of the new year...
January 25
Physikalisches Kolloquium at Universität Bonn on “Critical Tests of Theory of the Early Universe using the Cosmic Microwave Background” [15:15-17:00]
1/25: MUC(11:30)-CGN(12:35)1/26: CGN(10:15)-MUC(11:20)
January 23,24
Perspektivenkommission, Zugspitze
1/23: München Hbf(9:32)-Garmisch-Partenkirchen(10:54); Zugspitzbahn(11:15)-SonnAlpin(12:28)1/24: SonnAlpin(15:30)-Zugspitzbahn(16:50); Garmisch-Partenkirchen(17:05)-München Hbf(18:26)
January 21,22
ESTEC, for the kick-off meeting of ESA Cosmic Vision 2050 Senior Committee
1/21: MUC(14:35)-AMS(16:10)1/22: AMS(19:55)-MUC(21:15)
January 10
Back to normal life...