Espectroscopia

A set of three physical laws forming the basis of classical mechanics. The first law (inertia) states an object remains at rest or in uniform motion unless acted upon by a net external force. The second law quantifies force as mass times acceleration, [latex]\vec{F} = m\vec{a}[/latex]. The third law states that for every action, there is an equal and opposite reaction.

A Newtonian fluid's shear stress is directly proportional to the rate of shear strain. This linear relationship is defined by Newton's law of viscosity: [latex]\tau = \mu \frac{du}{dy}[/latex], where [latex]\tau[/latex] is the shear stress, [latex]\mu[/latex] is the dynamic viscosity (a constant of proportionality), and [latex]\frac{du}{dy}[/latex] is the shear rate or velocity gradient.

Bernoulli's principle states that for an inviscid flow, an increase in a fluid's speed occurs simultaneously with a decrease in pressure or a decrease in its potential energy. It is a statement of the conservation of energy for a moving fluid, commonly expressed as [latex]p + \frac{1}{2}\rho v^2 + \rho gh = \text{constant}[/latex] along a streamline.

La mecánica de fluidos es la rama de la mecánica aplicada que estudia la estática (fluidos en reposo) y la dinámica (fluidos en movimiento) de líquidos y gases. Aplica los principios fundamentales de conservación de la masa, el momento y la energía para analizar y predecir el comportamiento de los fluidos. Sus aplicaciones son amplias, abarcando desde la aerodinámica y la hidráulica hasta la meteorología y la oceanografía.

La fuerza centrífuga es una fuerza inercial o ficticia que parece actuar sobre una masa cuando se observa en un sistema de referencia giratorio. Se dirige radialmente hacia afuera desde el eje de rotación. Esta fuerza no es una interacción fundamental, sino que surge de la inercia del objeto, su tendencia a mantener el movimiento en línea recta en un sistema inercial.

Generalized Hooke's Law is the constitutive equation for linear elastic materials, stating that the stress tensor is linearly proportional to the strain tensor. The relationship is expressed as [latex]\sigma = C : \varepsilon[/latex], where [latex]\sigma[/latex] is the stress tensor, [latex]\varepsilon[/latex] is the strain tensor, and [latex]C[/latex] is the fourth-order stiffness tensor containing the material's elastic constants.

This law states that every particle attracts every other particle in the universe with a force directly proportional to the product of their masses and inversely proportional to the square of the distance between their centers. The formula is [latex]F = G \frac{m_1 m_2}{r^2}[/latex], where [latex]G[/latex] is the gravitational constant. It unified terrestrial and celestial mechanics.

In an isolated system, the total momentum remains constant. An isolated system is one not subject to external forces. This principle follows from Newton's laws of motion. For a system of particles, the total momentum [latex]\vec{p}_{\text{total}} = \sum_{i} m_i \vec{v}_i[/latex] is conserved if the net external force is zero. This is fundamental to analyzing collisions.

In a reference frame rotating with an angular velocity [latex]\boldsymbol{\omega}[/latex], the centrifugal force [latex]\mathbf{F}_{\mathrm{cf}}[/latex] acting on an object of mass [latex]m[/latex] at a position vector [latex]\mathbf{r}[/latex] from the origin is given by the vector formula: [latex]\mathbf{F}_{\mathrm{cf}} = -m \boldsymbol{\omega} \times (\boldsymbol{\omega} \times \mathbf{r})[/latex]. This formula shows the force is directed perpendicular to the axis of rotation and outwards.