全國中小學科展

物理與天文學

液滴撞擊平板耗散能量之變因

本研究探討液滴碰撞時各種變因對撞擊前後耗散能量的影響,主要以直徑、速度、黏度作為變因進行實驗。實驗前,先完成接觸角、表面張力、黏度與密度等基本量測,再利用高速攝影機測量出液滴直徑、最大擴張直徑與液滴撞擊速度,將其數值代入能量守恆式,計算出耗散能量後,發現它受到直徑的二分之一次方、速度的二分之三次方、黏度的二分之一影響,其中黏度也會造成能量與韋伯數關係圖的斜率些微變化。

扁平長方容器中顆粒體之轉動現象探討

顆粒體(細沙、塑膠珠與鋼珠)於扁平長方容器內近二維堆積在高速轉動時,其自由面有要成為拋物線的趨勢,但因有摩擦力的存在易導致自由面出現中央尖錐區與兩側線性堆積區之分布,因而呈現類似W之外型。近二維堆積顆粒體高速轉動下,摩擦力大者(如細沙、塑膠珠)易在近轉軸處出現中央尖錐;而摩擦力小者(如鋼珠)在近轉軸處則易出現較平坦之分布。另近二維堆積顆粒體在轉動過程達穩定後之自由面分布,會受經過的歷程所影響,不具可再現性。 相同數量(1000顆)與尺寸(3 mm)的鋼珠與塑膠珠混合後以高速(>500 rpm)轉動,其堆積分布與同轉速下的鋼珠一致,代表混合態高速轉動後穩定堆積的自由面分布是由慣性大的顆粒體所決定。 顆粒體和液體轉動時類似卻又不同的現象讓值得進一步的探討。

從吹不動螞蟻到吹出層流特質

為觀察氣流流經物體表面不易流動的現象,我們設計製造風洞實驗裝置。將筆芯墊在金屬片上,測量筆芯被吹動時的驅動速率,繼而變更筆芯的高度與水平位置,測量筆芯被吹動之驅動速率。由數據作圖可看出在風洞管下半部,筆芯驅動速率會隨著高度以乘冪減少,也就是從底層往上的流速是乘冪函數增加,與文獻之圖形類似。同時從數據作圖分析中也可看出筆芯越細,隨高度增加時,驅動速率較快變小。而筆芯超過風洞管一半鉛直高度後,數據曲線不如預期,故又繼續研究金屬塊破壞層流之效應。在底層放平行條狀物(簡稱肋條),用筆芯來看出氣流的擾動,測出驅動速率有些區域大有些區域小,表示障礙物引起二次流的紊流並不是流速變快,是屬於擾動式的。

Measuring the large nonlinear refractive index of pigment from avocado leaves by a laser pointer

本研究報告,從酪梨葉利用柱層分析技術萃取出葉綠素-a、葉綠素-b以及類胡蘿蔔素,用來研究其物理性質以及測量非線性折射率(n2)。 當雷射光束照射在置於比色管中的樣本時,中央軸上的強度最高,導致溶液產生了溫度梯度和折射率梯度。雷射光束穿過溶液後,在屏幕上產生了遠場繞射圖樣。這些繞射圖樣的最大半徑(Rm)和暗條紋的數目(N)隨雷射光的功率(P)、光徑長度 (𝓵)、溶液的熱吸收係數(μ)和溶劑的熱光係數(dn/dT)變化。從N對𝓵和N對P的關係圖中,可以計算出溶液的n2。 在本研究中,從酪梨葉中萃取的色素濃度分別是從菠菜和朱槿葉中萃取色素濃度的4.0倍和3.1倍。更令人驚訝的是測得的n₂ 值比石墨烯大100倍。結果顯示,該樣品具有顯著的非線性折射率,使其成為各種光學開關應用的理想材料。

旋轉鏈條張力分析及擾動波速研究

此實驗在研究一條環狀鏈條被吊起並開始旋轉時,在不同轉速下敲擊後所產生擾動波的現象。其中主要分析鏈條上波速和鏈條旋轉速度之間的關係。首先我們利用雷射切割機自製轉盤,並觀察到旋轉鏈條在不同轉速、敲擊不同位置時,在鏈條上所產生的波。我們接著用手機拍下此現象並用Tracker標記波的位置變化,放入Excel用回歸分析作圖之後,推測波速和鏈條轉速之間的關係。我們接著研究金屬鏈條碰觸地面受到摩擦力作用產生的週期性振盪,我們提出理論模型並估算週期,計算的結果與實驗數據吻合。最後研究旋轉鏈條被挑出圓盤後在地面移動的情形,分析移動距離、移動時間與轉速之間的關係。

Can Quantum Mechanical Two-State Theory model Coulomb’s Force?

The quantum mechanical description of the four fundamental forces of nature is very important for the decryption of the rules which underlie our world. While Quantum Electrodynamics (QED) describes the electromagnetic force in great detail, it also uses complex mathematical techniques and advanced physical concepts. In the following, I will analyze to what extent a quantum mechanical two-state model can be used to describe the Coulomb interaction between two charged particles. To do so, I will exclusively focus on the electrostatic interaction, leaving dynamics aside. Furthermore, the analysis is nonrelativistic and does not consider the spin of the particles. Finally, using discrete state theory allows to explore the strength of the basic concepts of early quantum mechanics. In this sense, I will try to develop a simpli ed model for the quantum mechanical description of the electrostatic force. However, the analysis is not simplistic, since the traditional formalism of quantum mechanics will be used, including Dirac's Bra-ket notation, probability amplitudes, the Hamiltonian matrix as well as the Schrödinger equation. To understand the framework of my project, it may be helpful to take a look at the source of inspiration for my analysis: In Chapter 10 of the third volume of the well-known textbook series The Feynman Lectures on Physics[4], the force holding the hydrogen molecular ion together is explained in terms of a two-state system. The electron of the molecular ion can be either at the rst proton or at the second one. The exchange of the electron between both protons leads to an attractive force between them. It is known from QED that the electrostatic interaction between two charged particles is due to the exchange of a virtual photon which acts as force carrier. The idea of my work is to explore whether the electrostatic force can be described by a very similar model, replacing the electron acting as force carrier in the molecular ion by a virtual photon for the description of the electrostatic force between two charged particles. To describe a system consisting of charged particles, I will make the assumption that a charged particle can appear in two states. Either it is in state e where it can emit a photon or it is in state a which enables it to absorb a photon. Upon emission or absorption of a photon the charged particle transitions to the respective other state. This makes the approach analyzed in my work an element of discrete state theory, since two di erent states of the particle are used to store information about it. Of course such a model cannot be compared to the sophisticated theory of Quantum Electrodynamics. The point is, however, that it is interesting to explore the power of the most fundamental concepts of quantum mechanics and to show that such an analysis can lead to inspiring results.

旋轉鏈條張力分析及擾動波速研究

此實驗在研究一條環狀鏈條被吊起並開始旋轉時,在不同轉速下敲擊後所產生擾動波的現象。其中主要分析鏈條上波速和鏈條旋轉速度之間的關係。首先我們利用雷射切割機自製轉盤,並觀察到旋轉鏈條在不同轉速、敲擊不同位置時,在鏈條上所產生的波。我們接著用手機拍下此現象並用Tracker標記波的位置變化,放入Excel用回歸分析作圖之後,推測波速和鏈條轉速之間的關係。我們接著研究金屬鏈條碰觸地面受到摩擦力作用產生的週期性振盪,我們提出理論模型並估算週期,計算的結果與實驗數據吻合。最後研究旋轉鏈條被挑出圓盤後在地面移動的情形,分析移動距離、移動時間與轉速之間的關係。

運用機器學習強化探測重力波訊號

本研究欲利用機器學習演算法,透過觀察重力波訊號來判斷黑洞融合訊號的時間。本研究 的數據來源於雷射干涉引力波天文台的開放資料庫,我從中獲取最被廣為認定的64筆原始數據,並生成具有不同黑洞質量與不同訊噪比的模擬信號。我將模擬信號與不同噪聲混合 後,進行強度調整、Q轉換和資料白化等數據處理,並提取資料的統計量,將其用於訓練三種決策樹演算法和兩種迴歸演算法中。最終研究結果顯示,決策樹演算法的判斷能力優於迴歸演算法,以及指出強度差值的標準差是最關鍵的特徵,重要性達全體特徵的27%。 我們的模型在重力波訊號判斷上表現出較高的效率,並成功降低了模型的複雜度,使其更適合實際應用。

磁星短x射線爆發特徵分析:以1E2259+586為例

我們是探討磁星的短X射線爆發(Short X-ray burst)。利用RXTE太空望遠鏡觀測磁星1E2259+586的數據,經由Bayesian block方法對光變曲線篩選找出爆發,並配合「波松分佈」與「虛無假設」找出50筆爆發事件(爆發的正確性有5σ的信心水準)。再利用HDBSCAN非監督式學習演算法來對短X射線爆發進行分群,找出此磁星有「短暫且高能爆發、中等持續與能量爆發、較長持續且溫和爆發、快速且低能爆發」現象,暗示了磁星爆發的多樣性並有不同的爆發機制。此外我們也發現磁星可能有「週期性」的現象,也許是自轉週期、地殼受的應力或磁場變化經過同樣時間累積(有週期性)而爆發。我們也比對有快速電波爆發 (Fast radio burst, FRB)的磁星SGR 1935+2154,看是否1E2259+586有FRB現象,結果暗示1E2259+586可能沒有FRB現象。

Efficient Modelling of Aeroacoustic Phenomena in Seebeck Sirens: A Simplified Approach for Real-World Applications

This paper presents a simplified but mostly accurate model for the acoustic mechanism of Seebeck sirens. We investigate the impact of key parameters, including the number and size of holes, as well as the angular speed of the disk, on the characteristics of the produced sound. The disk is fabricated using fused deposition modelling 3D printing, and we used a brushless motor, an air compressor, and a shotgun microphone to capture the generated sound. An order of magnitude analysis was conducted on the Navier-Stokes equation to formulate a simplified version. These simplifications allowed for a low computational intensity model relating volume flow rate to sound pressure level, which is used to predict the waveform of sound produced. Our findings reveal that the fundamental frequency of the sound can be precisely predicted by only the rotational frequency of the disk and the number of holes, a relationship validated experimentally. Notably, observed asymmetry in the waveform was attributed to skin drag effects, and this hypothesis was experimentally verified. Our model computes a solution in less than half a second on average: far less than the 21h 47min needed for a k−ω turbulent model to compute the same phenomenon. The research presents and verifies a simplified model of acoustic mechanics for the sound generated by rotating systems that require little computational resources, which can prove useful in situations where absolute precision is not required, in exchange for ease of computation. For more precise systems, this model serves as a foundation for quickly generating an initial design, paving the way for subsequent iterations using more comprehensive models. The developed model not only serves as a foundation for efficient preliminary designs but also contributes valuable insights into the intersection of fluid dynamics and sound production.