Previous Schedule: 1998 1999 2000 2001 2002 2003 2004 2005 2006 2007 2008 2009 2010 2011 2012 2013 2014 2015 2016 2017 2018 2019 2020 2021 2022
2023
2024
2025
2025
October 27?–31?
Zhejiang University, Hangzhou, China
October 23,24
Sektionssitzung, Harnack-Haus, Berlin
August 28–September 26
Nagoya University for the secondment of CMB-INFLATE
- 8/28-29: MUC(11:15)-HND(6:55); Move to Nagoya
- Inauguration of the Max Planck Center at the National Taiwan University
- 8/31: NGO(10:40)-TPE(12:45)
- 9/3: TPE(14:05)-NGO(17:50)
- 9/4-24: Nagoya University (9/19: APCTP Colloquium on Parity violation in cosmology [online])
- 9/25: Move to HND
- 9/26: HND(9:30)-MUC(16:45)
June 30–July 4
- 6/30: MUC(8:50)-ARN(11:00)
- 7/4: ARN(18:10)-MUC(20:30)
June 24–26
Jahresversammlung, Magdeburg
- 6/23: München Hbf(12:51, Gl.20)-Halle Hbf-Magdeburg Hbf(16:55)
- 6/25: Magdeburg Hbf(11:04, Gl.7)-Halle Hbf-München Hbf(15:08)
May 28–31
CMB@60, the Academy of Science of Turin
- 5/28: MUC(8:10)-TRN(9:25)
- 5/30: Give a 15-min presentation on "A tantalizing hint of cosmological parity violation in the polarized light of the cosmic microwave background" in the Panel 9 - Fundamental physics and anomalies
- 5/31: TRN(10:05)-MUC(11:15)
May 23
HEP/Astro Results Forum. Give a talk on "A tantalizing hint of cosmological parity violation in the polarized light of the cosmic microwave background"
May 12–17
UT Austin. Excited to be back in Austin!
- 5/12: MUC(7:00)-FRA-AUS(14:20)
- 5/13: Visiting Weinberg Institute
- 5/14-16: HETDEX Collaboration Meeting
- 5/16-17: AUS(16:05)-FRA-MUC(13:10)
May 5–9
Hamburg
- 5/5: MUC(13:15)-HAM(14:30)
- 5/6: Quantum Universe Colloquium, DESY on "A tantalizing hint of cosmological parity violation in the polarized light of the cosmic microwave background" [video]
- Abstract: The polarized light of the cosmic microwave background is sensitive to new physics that violates parity symmetry. In this presentation, we present a tantalizing hint of parity violation from the polarization data of two satellite missions, WMAP and Planck, with a statistical significance of 3 sigma. This signal has also been observed in recent data from the Atacama Cosmology Telescope. Taken together, there is evidence for a cosmological parity violation with a statistical significance of 4 sigma. If confirmed in the future with higher statistical significance, this finding would have profound implications for the elusive nature of dark matter and dark energy.
- 5/7: Kolloquium, Hamburger Sternwarte, on the same topic.
- 5/9: HAM(10:45)-MUC(12:05)