12/18 【Special lecture】Unraveling AGN Jets and Black Hole Accretion Across Multiple Scales

時間:12月18日(三) 12:00 ~ 13:20

題目:Unraveling AGN Jets and Black Hole Accretion Across Multiple Scales

講者:蘇恭毅 博士後研究員 Dr. Kung-Yi Su, BHI Fellow

服務單位: Black Hole Initiative, Harvard University

地點:本校科學三館3樓 SC353-2會議室

摘要:

AGN feedback poses a multiscale challenge, intertwined with significant disparities across the diverse length and time scales inherent in galaxy physics and the dynamics of black hole accretion disks. In this presentation, we explore our comprehensive investigation of AGN jets and black hole accretion, spanning from the galaxy scale to the black hole event horizon, with the ultimate goal of unifying the underlying physics across these scales.
At the galactic scale, we conduct an in-depth study of the physical variations of AGN jets using isolated galaxy simulations, ranging from L* galaxies to massive cluster ellipticals. We identify the conditions under which jet models effectively quench massive galaxies and their corresponding observational signatures. Notably, we reveal the critical role of cosmic rays in jets and highlight significant variations arising from different cosmic ray launching models.
At the intermediate scale, we employ a suite of idealized simulations centered on the black hole vicinity. By resolving the gravitational capture of gas by the black hole, we examine the detailed interplay between AGN jets and black hole accretion, deriving an analytical model to describe jet propagation and the self-regulation of black hole growth as functions of black hole mass, feedback models, and gas properties. This model points to a low feedback efficiency upper limit required for the formation of supermassive black holes at high redshift, as uncovered by JWST observations.

Finally, we outline our ongoing efforts to integrate the galaxy scale and black hole horizon scale into a unified simulation framework that leverages a novel multi-zone method to track bidirectional gas flows.

12/11【Special lecture】Manipulating elementary excitations in functional quantum materials using resonant X-ray techniques

時間:12月11日(三) 12:00 ~ 13:20

題目:Manipulating elementary excitations in functional quantum materials using resonant X-ray techniques

講者:曾奕 博士後研究員 Dr. Tseng Yi

服務單位:Deutsches Elektronen Synchrotron, Free-Electron Laser Hamburg

地點:本校科學三館3樓 SC353-2會議室

摘要:
The increasing demand and interests of quantum materials, as well as their intriguing macroscopic manifestation of collective phenomena and exotic properties, have led to unprecedented opportunities for materializing these emergent properties into functional devices, e.g. high-temperature superconductivity, quantum Hall effect, ferroelectricity, etc. In this vein, characterizing the underlying physics highlights a hallmark and unique realization in condensed matter physics, both from a fundamental as well from an applied perspective. In this talk, I will present studies using resonant X-ray spectroscopy techniques on elementary excitations in a number of quantum materials, specifically low-dimensional transition-metal magnets. Such experimental probes are sensitive to all electron degrees of freedom, i.e. lattice, spin, orbital and charge, capable of revealing unique information about the microscopic electronic interactions that are vital to the low-energy Hamiltonian. In addition to the aforementioned research achievements and present focus, future prospect including the ultrafast time control of electronic dynamics will be discussed.

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

時間:12月12日(四) 13:20 ~ 15:10

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

講者:潘國全 副教授

服務單位:國立清華大學 天文研究所

地點:本校科學三館1樓 SC157

摘要:
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

時間:11月28日(四) 13:20 ~ 15:10

題目:Probing entanglement dynamics on NISQ computers

講者:許琇娟 副教授

服務單位:國立政治大學 應用物理研究所

地點:本校科學三館1樓 SC157

摘要:
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

時間:10月17日(四) 13:20 ~ 15:10

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

講者:楊湘怡 副教授

服務單位:國立清華大學 天文研究所

地點:本校科學三館1樓 SC157

摘要:
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.

物理研究所2024秋季通俗演講系列

  • 地點:本校光復校區科學三館1樓SC106教室
  • 時間:週四中午12:10~13:20
  • 對象:全校大學部及研究所同學(不限科系)

11/14
我們為什麼需要DEI (diversity, equality and inclusion)? 從文化談起

王俐容 教授 / 國立中央大學通識教育中心‧客家語文暨社會科學學系


11/21
從「不正經的」動漫畫、科幻電影到「正經的」科學傳播

From ‘Playful’ Anime, Comics, and Sci-Fi Movies to ‘Serious’ Science Communication

許經夌 教授 / 中原大學物理學系


12/5
揭開自然界最強作用力的奧秘

Uncover the mysteries of the strongest force in nature

郭家銘教授 / 國立中央大學物理學系


9/26 Toward a Deeper Understanding of the Proton

時間:9月26日(四) 13:20 ~ 15:10

題目:Toward a Deeper Understanding of the Proton

講者:章文箴 研究員兼副所長

服務單位:中央研究院 物理研究所

地點:本校科學三館1樓 SC157

9/19 Searching for Extra Higgs Boson Effects in General 2HDM

時間:9月19日(四) 13:20 ~ 15:10

題目:Searching for Extra Higgs Boson Effects in General 2HDM

講者:侯維恕 講座教授

服務單位:國立臺灣大學 物理學系

地點:本校科學三館1樓 SC157

9/12 Using gravitational lensing to study dark matter and cosmology

時間:9月12日(四) 13:20 ~ 15:10
題目:Using gravitational lensing to study dark matter and cosmology
講者:譚雪瑩 老師
服務單位:國立陽明交通大學 物理研究所
地點:本校科學三館1樓 SC157

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

時間:5月30日(四) 13:20 ~ 15:10
題目:Toward a better understanding of galaxy formation in ΛCDM: part II
講者:林彥廷 研究員
服務單位:中央研究院 天文及天文物理研究所
地點:本校科學三館1樓 SC157