宇宙與粒子—物理科普講座

因疫情影響,本校停止辦理實體演講活動,
物理科普講座第2場次(5/27)、第3場次(6/17)延期辦理。
待擇定日期後再行公告。


時間:4/22 週四中午12:10~13:10  
地點:本校光復校區工程四館ED117
對象:對自然奧秘有興趣的大學部及研究所同學(不限科系)

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4/22
宇宙大霹靂的傳說—你和我的傳奇故事

高文芳 教授 /  國立陽明交通大學 物理研究所
時間:4/22 (四) 中午12:10~13:10
地點:本校光復校區工程四館ED117

Image courtesy of NASA


6/17  (延期辦理)
變身家族—微中子們的拿手好戲

林貴林 教授 /  國立陽明交通大學 物理研究所


5/27  (延期辦理)
從原子到夸克與膠子:量子色動力學的故事

林及仁 教授 /  國立陽明交通大學 物理研究所


可攜帶外食入場,歡迎邊用餐邊聽演講!!

12/24 The First Images of a Black Hole and General Relativistic Magnetohydrodynamical (GRMHD) Accretion/Jet : achievements and challenges

時間:12月24日(四) 13:20

題目: The First Images of a Black Hole and General Relativistic Magnetohydrodynamical (GRMHD) Accretion/Jet : achievements and challenges

講者:卜宏毅 教授

服務單位:國立臺灣師範大學 物理學系

地點:本校科學三館1樓 110室

對象:本所博士生及碩士生、或其他有興趣之師生

12/17 The emergence of collective modes, ecological collapse and directed percolation at the laminar-turbulent transition

時間:12月17日(四) 13:20

題目:The emergence of collective modes, ecological collapse and directed percolation at the laminar-turbulent transition
講者:施宏燕 研究員

服務單位:中央研究院 物理研究所

地點:本校科學三館1樓 110室

對象:本所博士生及碩士生、或其他有興趣之師生

摘要:

How a laminar flow becomes turbulence has been an unsolved problem for more than a century and is important in various industrial applications. Recently precise measurements in pipe flow experiments showed non-trivial spatiotemporal complexity at the onset of turbulence where lifetime and splitting time of metastable turbulence do not diverge asymptotically as would have been expected in a sharp transition.
Based on numerical evidence from the hydrodynamics equations, we discovered the surprising fact that the fluid behavior at the transition is governed by the emergent predator-prey dynamics of the important long-wavelength mode, leading to the mathematical prediction that the laminar-turbulent transition is analogous to an ecosystem on the edge of extinction. This prediction demonstrates that the laminar-turbulent transition is a non-equilibrium phase transition in the directed percolation universality class, and provides a unified picture of transition to turbulence emerging in systems ranging from turbulent convection to magnetohydrodynamics.

Reference:
[1] Hong-Yan Shih, Tsung-Lin Hsieh and Nigel Goldenfeld, Nature Physics 12, 245 (2016)
[2] https://www.nature.com/collections/rxsztdqblr

12/10 ANITA極高能微中子實驗中所發現的反常事例

時間:12月 10日(四) 13:20

題目:ANITA極高能微中子實驗中所發現的反常事例
講者:劉宗哲 老師

服務單位:國立交通大學 電子物理學系

地點:本校基礎科學教學研究大樓1樓 110室

對象:本所博士生及碩士生、或其他有興趣之師生

摘要:

We report on an upward traveling, radio-detected cosmic-ray-like impulsive event with characteristics closely matching an extensive air shower. This event,
observed in the third flight of the Antarctic Impulsive Transient Antenna (ANITA), a NASA-sponsored long-duration balloon payload, is consistent with a similar event reported in a previous flight.
These events may be produced by the atmospheric decay of an upward-propagating τ-lepton produced by a ντ interaction, although their relatively steep arrival angles create tension with the standard model (SM) neutrino cross section.
Each of the two events have a posteriori background estimates of <∼ 10^{−2} events.
If these are generated by τ-lepton decay, then either the charged-current ντ cross section is suppressed at EeV energies, or the events arise at moments
when the peak flux of a transient neutrino source was much larger than the typical expected cosmogenic background neutrinos.

https://arxiv.org/pdf/1803.05088.pdf