9/17 A Search for Planet Nine with IRAS and AKARI Data

時間:9月17日(四) 13:20 ~ 15:10

題目:A Search for Planet Nine with IRAS and AKARI Data

講者:後藤友嗣 教授

服務單位:國立清華大學 物理學系

地點:本校科學三館1樓 SC157

摘要:The outer solar system is theoretically predicted to harbour an undiscovered planet, often referred to as P9. Simulations suggest that its gravitational influence could explain the unusual clustering of minor bodies in the Kuiper Belt. However, no observational evidence for P9 has been found so far, as its predicted orbit lies far beyond Neptune, where it reflects only a faint amount of Sunlight. This work aims to find P9 candidates by taking advantage of two far-infrared all-sky surveys, which are IRAS and AKARI. The epochs of these two surveys were separated by 23 years, which is large enough to detect the ~3’/year orbital motion of P9. We use a dedicated AKARI Far-Infrared point source list for our P9 search – AKARI Monthly Unconfirmed Source List, which includes sources detected repeatedly only in hours timescale, but not after months. We search for objects that moved slowly between IRAS and AKARI detections given in the catalogues. First, we estimated the expected flux and orbital motion of P9 by assuming its mass, distance, and effective temperature to ensure it can be detected by IRAS and AKARI, then applied the positional and flux selection criteria to narrow down the number of sources from the catalogues. Next, we produced all possible candidate pairs whose angular separations were limited between 42′ and 69.6′, corresponding to the heliocentric distance range of 500 – 700 AU and the mass range of 7 – 17 Earth masses. There are 13 pairs obtained after the selection criteria. After image inspection, we found one good candidate, of which the IRAS source is absent from the same coordinate in the AKARI image after 23 years and vice versa. However, AKARI and IRAS detections are not enough to determine the full orbit of this candidate. This issue leads to the need for follow-up observations, which will determine the Keplerian motion of our candidate.

 

6/24【Special Colloquium】Experimental and Computational Physics for Several Nuclear and Radiation Applications

Experimental and Computational Physics for Several Nuclear and Radiation Applications [Part I] :
Radiation Protection, Shielding Materials, and Monte Carlo Simulations

時間:6月24日(四) 10:10 ~ 11:00 / Time:  Tuesday the 24th of June 2026, 10:10 ~ 11:00

講者:Main Speaker: Dr. Tung Hoang Nguyen
Co- Speaker: Dr. Mohamed Mitwalli

服務單位:IRC for Industrial Nuclear Energy (IRC-INE)
King Fahd University of Petroleum & Minerals (KFUPM), Saudi Arabia

地點:本校科學三館4樓 SC427會議室 / Venue: SC427, Science Building 3, NYCU

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Experimental and Computational Physics for Several Nuclear and Radiation Applications [Part II] :
Environmental Sustainability, Rare Element Mining, and Heritage Dating

時間:6月24日(四) 11:10 ~ 12:00 / Time:  Tuesday the 24th of June 2026, 11:10 ~ 12:00

講者:Main Speaker: Dr. Mohamed Mitwalli
Co- Speaker: Dr. Tung Hoang Nguyen

服務單位:IRC for Industrial Nuclear Energy (IRC-INE)
King Fahd University of Petroleum & Minerals (KFUPM), Saudi Arabia

地點:本校科學三館4樓 SC427會議室 / Venue: SC427, Science Building 3, NYCU

6/4 Probing Magnetar Science in the NICER Era

時間:6月4日(四) 13:20 ~ 15:10

題目:Probing Magnetar Science in the NICER Era

講者:胡欽評 副教授

服務單位:國立彰化師範大學 物理學系

地點:本校科學三館1樓 SC157

5/28 A Decade of Progress and Future Prospects in Rare Kaon Decays

時間:5月28日(四) 13:20 ~ 15:10

題目:A Decade of Progress and Future Prospects in Rare Kaon Decays

講者:林杰 助理教授

服務單位:國立彰化師範大學 物理學系

地點:本校科學三館1樓 SC157

 

4/30 New Frontiers in Characterizing Exoplanet Atmospheres

時間:4月30日(四) 13:20 ~ 15:10

題目:New Frontiers in Characterizing Exoplanet Atmospheres

講者:蔡尚旻 助研究員

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

摘要:

Exoplanet science has made remarkable progress. With advancements in high-resolution spectroscopy and the launch of JWST, the field has transitioned from detection to detailed atmospheric characterization.
The diversity of exoplanets presents intriguing puzzles that challenge our theoretical understanding.
In this talk, I will review progress in exoplanet research, with an emphasis on atmospheric characterization. I will highlight some recent JWST observations, including the first evidence of photochemistry on an exoplanet. I will present the enigmatic nature of intermediate-sized planets and share insights from our recent study on temperate sub-Neptunes. I will conclude with key open questions in exoplanet characterization that are within reach of upcoming capabilities.

4/16 Biophysics of cyclic stretch-induced cell columnarization

時間:4月16日(四) 13:20 ~ 15:10

題目:Biophysics of cyclic stretch-induced cell columnarization (循環拉伸誘導細胞柱狀化的生物物理學)

講者:温福來 助理教授

服務單位:國立中央大學 物理學系

地點:本校科學三館1樓 SC157

4/9 Device-Independent Quantum Rigidity for Secure Global Positioning

時間:4月9日(四) 13:20 ~ 15:10

題目:Device-Independent Quantum Rigidity for Secure Global Positioning

講者:郭恩瑞 助理教授

服務單位:國立陽明交通大學 電子物理系

地點:本校科學三館1樓 SC157

摘要:

Device-independent (DI) protocols provide the strongest form of security by removing trust assumptions on quantum devices and relying solely on observed nonlocal correlations and quantum rigidity. In this talk, I will discuss how multipartite Bell nonlocality and self-testing can be leveraged to secure distributed positioning tasks, using a quantum-secured global positioning system (GPS) as a concrete case study.

We consider a protocol based on a five-qubit entangled state shared among four satellites and one ground station, where correct state preparation and measurement behavior are certified solely from Bell inequality violations. I will explain how rigidity guarantees enable device-independent authentication against spoofing and cyberattacks, and discuss practical considerations in the NISQ era, including implementation trade-offs between superconducting and trapped-ion platforms, as well as constraints arising from long-distance photonic distribution.

The emphasis of the talk will be on conveying the core ideas of device-independence and self-testing, with sufficient background to make the discussion accessible to a broad quantum information audience.

For reference, the related paper of mine is available here:
https://link.springer.com/article/10.1140/epjqt/s40507-026-00470-6

3/19 New High-Tc Charge-Transfer Multiferroicity in the Quasi-2D Antiferromagnet CrSbS3

時間:3月19日(四) 13:20 ~ 15:10

題目:New High-Tc Charge-Transfer Multiferroicity in the Quasi-2D Antiferromagnet CrSbS3

講者:吳紘丞 助理教授

服務單位:國立中山大學 物理學系

地點:本校科學三館1樓 SC157

3/12 Taiwan’s Time-Domain Framework at Lulin Observatory

時間:3月12日(四) 13:20 ~ 15:10

題目:Taiwan’s Time-Domain Framework at Lulin Observatory

講者:陳婷琬 助理教授

服務單位:國立中央大學 天文研究所

地點:本校科學三館1樓 SC157

物理研究所2026春季通俗演講系列

  • 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)

3/5
天文學嘛會使用台語講

    • 蔡安理博士 / 國立中央大學 天文研究所

蔡安理老師曾在臺師大地球科學系教授臺語天文學,還將NASA APOD (Astronomy Picture of the Day) 英文天文文章翻譯成台語,張貼在「逐工一幅天文圖」的部落格,更特地建立「台語科學學術詞彙庫」,在Facebook、Podcast等社群媒體上向大眾推廣以台語認識天文學,讓我們看見母語的更多可能性。本次演講她將帶領我們打破語言框架,用親切的台語探索浩瀚宇宙。


4/23
質子內部的反物質

    • 彭仁傑教授 / 美國伊利諾大學香檳分校 物理系
      【中央研究院院士】

原子核是由質子和中子組成的。質子和中子並非基本粒子,而是由其他基本粒子組成的。這些基本粒子包括夸克,反夸克,及膠子。我們知道質子是「物質」,然而反夸克是「反物質」。為何在物質中會含有反物質?如何在實驗室探測到質子中的反物質?這些反物質有何特性?這是我們嘗試探討的問題。


5/14
球形牛可以有皺紋嗎?——超重力五十週年展望

    • 黃宇廷教授 / 國立臺灣大學 物理學系