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Density Of Ice
Density Of Ice
The density of solid water, unlike most molecules, is less than that of its liquid form. Its precise value is of use in many applications. Freezing a spherical droplet of water and analyzing the changed shape from a sphere to a sphere with a slight peak in order to find the density of ice. We find the density of ice to be at 0.90 ± 1.66 · 106 g/mL. The precision of our measurement was limited by uncertainty in the angle measurements of the peak of the droplet.
Ashley
Homework 3
Homework 3
MATH 108 - Introduction to Formal Mathematics
Brennan Gilmore
Compte rendu Thermo
Compte rendu Thermo
TP thermodynamique
Remini Loucif
Assignment 0
Assignment 0
First 2 problems as a tester.
Jacob Vella
مسألة  دالة اللوغاريامية مع المساحات
مسألة دالة اللوغاريامية مع المساحات
مسالة للدالة اللوعالاتمية مع المساحات و قابلية الإشتقاق
bouanad
Why it's good that Soulstealer Vayne is so hard to get - a statistical Analysis
Why it's good that Soulstealer Vayne is so hard to get - a statistical Analysis
I analyzed the Hextech-Crafting in a Stochastic Simulation with 10 Million Players and found that you're going to make more Riot Points than you spend (in value) and thats without counting Champs. I've made some assumptions, which can be found down in the paper itself for those interested. For everyone else: If you're trying to maximize your RP-Net-Worth stack up on Hextech Chests.
WORST BRUISER EU
Lane's Test Template
Lane's Test Template
A template for instructors to create exams for Mathematics/Statistics classes.
Lane Tait
Geometría del Espacio
Geometría del Espacio
Solucionario de dos interesantes problemas propuestos
William Arcaya C.
Oscilaciones del Neutrino
Oscilaciones del Neutrino
Las observaciones han mostrado que el numero de neutrinos electrónicos νe que llegan a la tierra desde el sol es aproximadamente la mitad del número esperado de nuestro conocimiento de las reacciones nucleares que ocurren al interior del sol. Estas observaciones se explican como el resultado de que algunos neutrinos electrónicos νe se convierten en neutrinos muónicos νμ y neutrinos tauónicos ντ durante su recorrido entre su creación al interior del sol y su observación en la tierra. Este cambio de un sabor a otro se conoce como oscilaciónes del neutrino. Se introduce un término de masa para el neutrino que es invariante de Lorentz en la densidad lagrangiana del modelo estándar (SM), y se describe el estado del neutrino |να⟩(α = e, μ, τ) como una combinación lineal de autoestados de masa |νi⟩ (i=1,2,3), lo cual conduce a las oscilaciones del neutrino.
Daniel Ocampo Henao

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