5/8 How to better measure seismic hazard: insights from earthquake kinematics and dynamics

Time: 1:20pm~3:10pm, May 8 (Thursday)

Title: How to better measure seismic hazard: insights from earthquake kinematics and dynamics

Speaker: Dr. Kuo-Fong Ma, Distinguished Research Fellow
(Institute of Earth Sciences, Academia Sinica)

Place: Science Building III SC162

5/1 Open Quantum Systems: Thermometry at the Extremes

Time: 1:20pm~3:10pm, May 1 (Thursday)

Title: Open Quantum Systems: Thermometry at the Extremes

Speaker: Prof. Alexander Karl Rothkopf
(Department of Physics, Korea University, South Korea)

Place: Science Building III SC162

Abstract: The study of quantum systems coupled to an environment plays a vital role in how we measure temperatures of the coldest and hottest matter in the universe. The strategy relies on introducing impurities into the system of interest and on observing how these probe particles evolve towards or in equilibrium with their surroundings, from which we may in turn deduce the thermal properties of that environment. Originally studied in the context of condensed matter physics, open quantum systems nowadays provide a common language to research spanning multiple orders of magnitude in temperature, ranging from Bose Einstein condensates made of ultracold atoms to the Quark-Gluon plasma created in ultra-relativistic collisions of heavy ions. This talk builds a bridge from polaron impurities in the former to quarkonium particles in the latter as two manifestations of quantum Brownian motion, a phenomenon ideally described by open quantum systems.

3/27 Amplitudes Meets Effective Field Theory: New Results for Gravitational Waves and Particle Physics

Time: 1:20pm~3:10pm, March 27 (Thursday)

Title: Amplitudes Meets Effective Field Theory: New Results for Gravitational Waves and Particle Physics

Speaker: Professor Chia-Hsien Shen
(Department of Physics, National Taiwan University)

Place: Science Building III SC162

3/20 Dark Matter Searches in Gravitational Wave Detectors

Time: 1:20pm~3:10pm, March 20 (Thursday)

Title: Dark Matter Searches in Gravitational Wave Detectors

Speaker: Professor Martin Spinrath
(Department of Physics, National Tsing Hua University)

Place: Science Building III SC162

Abstract: In my talk I will discuss our recent work in studying the prospects to look for Dark Mater in Gravitational Wave Detectors using KAGRA as example. Interestingly, these detectors can probe a parameter region inaccessible to conventional Dark Matter direct searches. If time allows I will also comment on some other peoples work looking for a different kind of dark matter in gravitational wave detectors.

3/6 Top quark entanglement 
at CMS experiment

Time: 1:20pm~3:10pm, March 6 (Thursday)

Title: Top quark entanglement 
at CMS experiment

Speaker: Professor Kai-Feng Chen
(Department of Physics, National Taiwan University)

Place: Science Building III SC162

2/27 Machine-learning enhanced quantum state tomography and its applications to the gravitational wave detectors

Time: 1:20pm~3:10pm, February 27 (Thursday)

Title: Machine-learning enhanced quantum state tomography and its applications to the gravitational wave detectors

Speaker: Professor Ray-Kuang Lee
(Institute of Photonics Technologies, National Tsing Hua University)

Place: Science Building III SC162

12/12 Multi-messenger signals from magnetized core-collapse supernovae

Time: 1:20pm~3:10pm, December 12 (Thursday)

Title: Multi-messenger signals from magnetized core-collapse supernovae

Speaker: Associate Professor Kuo-Chuan Pan
(Institute of Astronomy, National Tsing Hua University)

Place: Science Building III SC157

Abstract:

Core-collapse supernovae (CCSNe) are among the most explosive events in the universe and are the birthplaces of neutron stars and stellar-mass black holes under extreme conditions. CCSNe are also ideal multi-messenger sources, expected to be detected not only through electromagnetic waves but also via neutrinos and gravitational waves.
In this talk, I will present the latest results from our multi-dimensional supernova simulations with self-consistent neutrino transport. In particular, I will focus on how magnetic fields and stellar rotation affect the explosion engine and multi-messenger signals. I will also comment on further searches for gravitational waves from core-collapse supernovae.

11/28 Probing entanglement dynamics on NISQ computers

Time: 1:20pm~3:10pm, November 28 (Thursday)

Title: Probing entanglement dynamics on NISQ computers

Speaker: Associate Professor Hsiu-Chuan Hsu
(Graduate Institute of Applied Physics, National Chengchi University)

Place: Science Building III SC157

Abstract:

The quench dynamics of the Su-Schierffer-Heeger (SSH) chain is simulated on IBM Quantum computers. The second-order Rényi entanglement entropy, the twist order parameter and the Berry phase are calculated and shown persistent oscillations. Through error mitigation techniques, including global depolarizing error ansatz and postselection based on symmetry constraints, the simulation results match closely to the exact solution. Along with this research, a software tool is developed for effective simulation of entanglement entropy and a patent for monitoring quantum computers is granted.

10/17 Cosmic Ray Feedback in the Universe: Fermi Bubbles and Odd Radio Circles

Time: 1:20pm~3:10pm, October 17 (Thursday)

Title: Cosmic Ray Feedback in the Universe: Fermi Bubbles and Odd Radio Circles

Speaker: Associate Professor Hsiang-Yi Karen Yang
(Institute of Astronomy, National Tsing Hua University)

Place: Science Building III SC157

Abstract:

Relativistic jets from supermassive black holes (SMBHs) are vital drivers of massive galaxy properties, and cosmic rays (CRs) within SMBH jets have shown to be a key ingredient in the process. It is therefore crucial to model the effects of CRs self-consistently in numerical simulations. In this talk, I will present how we could apply 3D CR-magnetohydrodynamic (MHD) simulations to understand enigmatic phenomena in the Universe, including the Fermi bubbles within the Milky Way Galaxy, as well as the newly discovered odd radio circles (ORCs). Our investigations suggest that both phenomena could be explained by powerful jet activity of SMBHs.

5/30 Toward a better understanding of galaxy formation in ΛCDM: part II

Time: 1:20pm~3:10pm, May 30 (Thursday)
Title: Toward a better understanding of galaxy formation in ΛCDM: part II
Speaker: Dr. Yen-Ting Lin (Research Fellow)
(Institute of Astronomy and Astrophysics, Academia Sinica)
Place: Science Building III SC157
Abstract:
I will continue my unfinished talk from last year(!) and provide a general overview of our current understanding of how galaxies form in the framework of the standard model of cosmology. I will review the success and potential problems ΛCDM faces in producing the galaxy population we observe, and finish with our recent validation of ΛCDM using the most massive galaxies in the universe.