Topics (206k) Articles (211k) Users (302) Discussions (237) Comments (383) Files (715) New article
In physics, the term "residual property" can refer to various concepts depending on the context, but it is most commonly associated with materials science, thermodynamics, and fluid mechanics. Here are a couple of common interpretations: 1. **Residual Stress**: This refers to internal forces that remain in a material after the original cause of the stresses has been removed. Residual stresses can significantly affect the material's strength, durability, and overall performance.
"Reduced properties" typically refer to a set of thermodynamic properties that are used to characterize the behavior of substances in relation to their critical points. These properties are particularly useful in the study of gases and other substances in various thermodynamic processes. The reduced properties are defined as follows: 1. **Reduced Temperature (\( T_r \))**: This is defined as the ratio of the temperature of the substance to its critical temperature (\( T_c \)).
Recalescence is a phenomenon observed in materials, particularly in metallurgy, during the phase transformation from a liquid to a solid state, specifically during solidification. It refers to the rise in temperature that can occur in a material as it transitions from a supercooled liquid to a solid phase. When a metal or alloy is cooled past its freezing point, it may continue to cool below its equilibrium solidification temperature, entering a metastable state.
The rate of heat flow, often referred to as heat transfer rate, is a measure of the amount of thermal energy being transferred from one system or body to another over a specific period of time. It is typically expressed in units such as watts (W), where one watt is equivalent to one joule per second (J/s). Heat flow occurs through three primary mechanisms: 1. **Conduction**: The transfer of heat through a material without the movement of the material itself.
Pressure is defined as the force exerted per unit area on a surface. It is a scalar quantity, meaning it has magnitude but no direction. The formula to calculate pressure (P) is: \[ P = \frac{F}{A} \] where: - \( P \) is the pressure, - \( F \) is the force applied, - \( A \) is the area over which the force is distributed.
A partial molar property is a thermodynamic property of a component in a mixture that describes how that property changes when the number of moles of that component is varied while keeping the temperature, pressure, and the amounts of all other components constant. In essence, it provides insight into how the behavior of one component affects the overall properties of the mixture.
Molar heat capacity (often represented as \( C_m \)) is a physical property of a substance that indicates the amount of heat required to raise the temperature of one mole of that substance by one degree Celsius (or one Kelvin). It reflects how much heat energy is absorbed or released when a substance undergoes a temperature change.
In the context of thermodynamics, material properties refer to the characteristics of a material that define its behavior in response to changes in temperature, pressure, and other environmental conditions. These properties are critical for understanding how materials will perform in various applications, particularly in areas such as engineering, materials science, and physics.
Latent internal energy refers to the energy stored within a substance that is associated with changes in its phase or state, such as during melting, freezing, vaporization, or condensation. This type of energy is not immediately observable as a change in temperature since it is involved in breaking or forming intermolecular bonds rather than increasing the kinetic energy of the particles.
Internal pressure refers to the pressure that exists within a confined space, such as a container, vessel, or any system that holds a fluid (liquid or gas). This pressure is caused by the molecules of the substance interacting with each other and the walls of the container. Key points about internal pressure include: 1. **Definition**: Internal pressure is the force exerted by the molecules of a fluid on the walls of its container.
Intensive and extensive properties are classifications of physical properties of matter that help in understanding the behavior and characteristics of different substances. Here's a brief overview of each: ### Intensive Properties Intensive properties are those that do not depend on the amount of substance present. These properties are intrinsic to the material and are characteristic of the substance itself. Some common examples include: - **Temperature**: The temperature of a substance does not change regardless of the size of the sample.
The heat of vaporization (also known as enthalpy of vaporization) is the amount of energy required to convert a unit mass of a substance from a liquid into a vapor at a constant temperature and pressure. For elements, this value varies significantly and is typically measured in joules per gram (J/g) or kilojoules per mole (kJ/mol).
The heat of fusion, also known as the enthalpy of fusion, is the amount of energy required to change a substance from a solid to a liquid at its melting point. This property varies among different elements and compounds. Here’s a general overview of the heats of fusion for some common elements (values are approximate and can vary based on the source): 1. **Hydrogen (H)**: 0.117 kJ/mol 2.
Heat loss due to linear thermal bridging refers to the additional heat loss that occurs at junctions and around openings in building elements—such as walls, roofs, and floors—where two materials meet. This phenomenon occurs because the thermal resistance of the junctions is often lower than that of the surrounding materials, leading to increased heat transfer. **Key Points about Linear Thermal Bridging:** 1.
Heat flux, often denoted as \( q \), is the rate of heat transfer per unit area through a surface. It quantifies the amount of thermal energy that flows through a given surface area in a specific direction, typically expressed in units of watts per square meter (W/m²). Heat flux can occur through conduction, convection, and radiation: 1. **Conduction:** Involves heat transfer through materials due to temperature gradients.
Heat capacity is a physical property of a substance that measures the amount of heat energy required to change its temperature by a certain amount. It quantifies how much heat is needed to raise the temperature of a material based on its mass and specific heat capacity. There are two key concepts related to heat capacity: 1. **Specific Heat Capacity**: This is the amount of heat required to raise the temperature of one unit mass of a substance by one degree Celsius (or one Kelvin).
Heat capacity is a property that indicates the amount of heat energy required to change the temperature of a substance by a certain amount. For elements, heat capacity can be expressed in different forms, commonly as molar heat capacity (the heat capacity per mole of an element) and specific heat capacity (the heat capacity per unit mass).
Fugacity is a concept in thermodynamics and physical chemistry used to describe the "effective pressure" of a real gas. It accounts for deviations from ideal gas behavior, particularly under conditions of high pressure or low temperature, where interactions between gas molecules become significant. In essence, fugacity (\( f \)) represents how a gas behaves in a system relative to an ideal gas.
The entropy of vaporization, often denoted as \( \Delta S_{vap} \), is a thermodynamic quantity that describes the change in entropy when one mole of a substance transitions from the liquid phase to the vapor phase at a given temperature and pressure. It reflects the degree of disorder or randomness in the system. When a liquid evaporates, its molecules gain sufficient energy to overcome intermolecular forces and enter the gas phase, which is characterized by greater molecular movement and spacing.
Pinned article: Introduction to the OurBigBook Project
Welcome to the OurBigBook Project! Our goal is to create the perfect publishing platform for STEM subjects, and get university-level students to write the best free STEM tutorials ever.
Everyone is welcome to create an account and play with the site: ourbigbook.com/go/register. We belive that students themselves can write amazing tutorials, but teachers are welcome too. You can write about anything you want, it doesn't have to be STEM or even educational. Silly test content is very welcome and you won't be penalized in any way. Just keep it legal!
Intro to OurBigBook
. Source. We have two killer features:
- topics: topics group articles by different users with the same title, e.g. here is the topic for the "Fundamental Theorem of Calculus" ourbigbook.com/go/topic/fundamental-theorem-of-calculusArticles of different users are sorted by upvote within each article page. This feature is a bit like:
- a Wikipedia where each user can have their own version of each article
- a Q&A website like Stack Overflow, where multiple people can give their views on a given topic, and the best ones are sorted by upvote. Except you don't need to wait for someone to ask first, and any topic goes, no matter how narrow or broad
This feature makes it possible for readers to find better explanations of any topic created by other writers. And it allows writers to create an explanation in a place that readers might actually find it.Figure 1. Screenshot of the "Derivative" topic page. View it live at: ourbigbook.com/go/topic/derivativeVideo 2. OurBigBook Web topics demo. Source. - local editing: you can store all your personal knowledge base content locally in a plaintext markup format that can be edited locally and published either:This way you can be sure that even if OurBigBook.com were to go down one day (which we have no plans to do as it is quite cheap to host!), your content will still be perfectly readable as a static site.
- to OurBigBook.com to get awesome multi-user features like topics and likes
- as HTML files to a static website, which you can host yourself for free on many external providers like GitHub Pages, and remain in full control
Figure 2. You can publish local OurBigBook lightweight markup files to either OurBigBook.com or as a static website.Figure 3. Visual Studio Code extension installation.Figure 5. . You can also edit articles on the Web editor without installing anything locally. Video 3. Edit locally and publish demo. Source. This shows editing OurBigBook Markup and publishing it using the Visual Studio Code extension. - Infinitely deep tables of contents:
All our software is open source and hosted at: github.com/ourbigbook/ourbigbook
Further documentation can be found at: docs.ourbigbook.com
Feel free to reach our to us for any help or suggestions: docs.ourbigbook.com/#contact





