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Elastic modulus
Elastic modulus
from Wikipedia

An elastic modulus (also known as modulus of elasticity (MOE)) is a quantity that describes an object's or substance's resistance to being deformed elastically (i.e., non-permanently) when a stress is applied to it.

Definition

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The elastic modulus of an object is defined as the slope of its stress–strain curve in the elastic deformation region:[1] A stiffer material will have a higher elastic modulus. An elastic modulus has the form:

where stress is the force causing the deformation divided by the area to which the force is applied and strain is the ratio of the change in some parameter caused by the deformation to the original value of the parameter.

Since strain is a dimensionless quantity, the units of will be the same as the units of stress.[2]

Elastic constants and moduli

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Elastic constants are specific parameters that quantify the stiffness of a material in response to applied stresses and are fundamental in defining the elastic properties of materials. These constants form the elements of the stiffness matrix in tensor notation, which relates stress to strain through linear equations in anisotropic materials. Commonly denoted as Cijkl, where i,j,k, and l are the coordinate directions, these constants are essential for understanding how materials deform under various loads.[3]

Types of elastic modulus

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Specifying how stress and strain are to be measured, including directions, allows for many types of elastic moduli to be defined. The four primary ones are:

  1. Young's modulus (E) describes tensile and compressive elasticity, or the tendency of an object to deform along an axis when opposing forces are applied along that axis; it is defined as the ratio of tensile stress to tensile strain. It is often referred to simply as the elastic modulus.
  2. The shear modulus or modulus of rigidity (G or Lamé second parameter) describes an object's tendency to shear (the deformation of shape at constant volume) when acted upon by opposing forces; it is defined as shear stress over shear strain. The shear modulus is part of the derivation of viscosity.
  3. The bulk modulus (K) describes volumetric elasticity, or the tendency of an object to deform in all directions when uniformly loaded in all directions; it is defined as volumetric stress over volumetric strain, and is the inverse of compressibility. The bulk modulus is an extension of Young's modulus to three dimensions.
  4. Flexural modulus (Eflex) describes the object's tendency to flex when acted upon by a moment.

Two other elastic moduli are Lamé's first parameter, λ, and P-wave modulus, M, as used in table of modulus comparisons given below references. Homogeneous and isotropic (similar in all directions) materials (solids) have their (linear) elastic properties fully described by two elastic moduli, and one may choose any pair. Given a pair of elastic moduli, all other elastic moduli can be calculated according to formulas in the table below at the end of page.

Fluids at rest are special in that they cannot support shear stress, meaning that the shear modulus is always zero. This also implies that Young's modulus for this group is always zero. When moving relative to a solid surface a fluid will experience shear stresses adjacent to the surface, giving rise to the phenomenon of viscosity.

In some texts, the modulus of elasticity is referred to as the elastic constant, while the inverse quantity is referred to as elastic modulus.

Density functional theory calculation

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Density functional theory (DFT) provides reliable methods for determining several forms of elastic moduli that characterise distinct features of a material's reaction to mechanical stresses. Utilize DFT software such as VASP, Quantum ESPRESSO, or ABINIT. Overall, conduct tests to ensure that results are independent of computational parameters such as the density of the k-point mesh, the plane-wave cutoff energy, and the size of the simulation cell.

  1. Young's modulus (E) - apply small, incremental changes in the lattice parameter along a specific axis and compute the corresponding stress response using DFT. Young's modulus is then calculated as E=σ/ϵ, where σ is the stress and ϵ is the strain.[4]
    1. Initial structure: Start with a relaxed structure of the material. All atoms should be in a state of minimum energy (i.e., minimum energy state with zero forces on atoms) before any deformations are applied.[5]
    2. Incremental uniaxial strain: Apply small, incremental strains to the crystal lattice along a particular axis. This strain is usually uniaxial, meaning it stretches or compresses the lattice in one direction while keeping other dimensions constant or periodic.
    3. Calculate stresses: For each strained configuration, run a DFT calculation to compute the resulting stress tensor. This involves solving the Kohn-Sham equations to find the ground state electron density and energy under the strained conditions
    4. Stress-strain curve: Plot the calculated stress versus the applied strain to create a stress-strain curve. The slope of the initial, linear portion of this curve gives Young's modulus. Mathematically, Young's modulus E is calculated using the formula E=σ/ϵ, where σ is the stress and ϵ is the strain.
  2. Shear modulus (G)
    1. Initial structure: Start with a relaxed structure of the material. All atoms should be in a state of minimum energy with no residual forces. (i.e., minimum energy state with zero forces on atoms) before any deformations are applied.
    2. Shear strain application: Apply small increments of shear strain to the material. Shear strains are typically off-diagonal components in the strain tensor, affecting the shape but not the volume of the crystal cell.[6]
    3. Stress calculation: For each configuration with applied shear strain, perform a DFT calculation to determine the resulting stress tensor.
    4. Shear stress vs. shear strain curve: Plot the calculated shear stress against the applied shear strain for each increment. The slope of the stress-strain curve in its linear region provides the shear modulus, G=τ/γ, where τ is the shear stress and γ is the applied shear strain.
  3. Bulk modulus (K)
    1. Initial structure: Start with a relaxed structure of the material. It's crucial that the material is fully optimized, ensuring that any changes in volume are purely due to applied pressure.
    2. Volume changes: Incrementally change the volume of the crystal cell, either compressing or expanding it. This is typically done by uniformly scaling the lattice parameters.
    3. Calculate pressure: For each altered volume, perform a DFT calculation to determine the pressure required to maintain that volume. DFT allows for the calculation of stress tensors which provide a direct measure of the internal pressure.
    4. Pressure-volume curve: Plot the applied pressure against the resulting volume change. The bulk modulus can be calculated from the slope of this curve in the linear elastic region. The bulk modulus is defined as K=−VdV/dP, where V is the original volume, dP is the change in pressure, and dV is the change in volume.[7]

See also

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References

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Further reading

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Revisions and contributorsEdit on WikipediaRead on Wikipedia
from Grokipedia
The elastic modulus is a fundamental mechanical property that quantifies a material's , defined as the ratio of applied stress to the resulting strain within the elastic deformation range, where the material returns to its original shape upon removal of the load. This property arises from the atomic and molecular of materials and is crucial for understanding how substances respond to forces without undergoing permanent damage. There are three primary types of elastic moduli, each corresponding to different deformation modes: (E), which measures resistance to linear extension or compression under uniaxial stress and is calculated as E = stress / axial strain; (G), which quantifies resistance to angular distortion under and is given by G = / shear strain; and (K), which describes resistance to uniform volumetric compression and is defined as K = - (pressure change) / (relative volume change). is the most commonly referenced elastic modulus in contexts, often simply called the modulus of elasticity, and its value indicates how much a material will elongate or shorten per unit stress. For example, has a Young's modulus around 200 GPa, making it significantly stiffer than rubber, which is about 0.01–0.1 GPa. These moduli are essential in fields like , , and for predicting structural behavior, designing load-bearing components, and selecting materials that balance strength and flexibility. Values are typically expressed in pascals (Pa) or gigapascals (GPa) in the , reflecting the material's inherent resistance to deformation rather than its size or shape. Experimental determination involves applying controlled loads and measuring deformations, often using machines to generate stress-strain curves from which the moduli are derived.

Basic Concepts

Stress and Strain

In solid mechanics, is defined as the internal force per unit area acting within a , quantifying the intensity of forces distributed over a surface. The , introduced by in the 1820s, provides a complete mathematical description of this force distribution in the deformed configuration, relating the traction vector on any surface to its normal vector through the second-order tensor σ, where the normal stress component σ_n = t · n and arises from the tangential component. For a simple case, normal stress σ is given by σ = F / A, where F is the applied force perpendicular to the cross-sectional area A. Stress manifests in different types depending on the direction and nature of the force: tensile stress occurs when forces pull the material apart, elongating it along the force direction; compressive stress arises from forces pushing the material together, shortening it; and shear stress results from forces acting parallel to the surface, causing layers to slide relative to one another. These types are fundamental to analyzing material behavior under load, with tensile and compressive stresses being normal to the surface and shear stresses tangential. Strain, conversely, measures the relative deformation or distortion of a from its original configuration, serving as the kinematic counterpart to stress. Normal strain ε quantifies linear deformation as ε = ΔL / L_0, where ΔL is the change in length and L_0 is the original length, positive for extension (tensile) and negative for contraction (compressive). Shear strain γ describes angular distortion as γ = Δx / L, where Δx is the transverse displacement and L is the over which the shear acts, often approximated as the of the shear angle for small deformations. A key distinction exists between engineering strain and true strain: engineering strain uses the original undeformed length L_0 in the denominator, suitable for small deformations, while true (or logarithmic) strain employs the instantaneous length, defined as ε_true = ∫ (dL / L) = ln(L / L_0), providing a more accurate measure for large deformations where cross-sectional area changes significantly. For small deformations in , the infinitesimal strain tensor ε_ij = (1/2)(∂u_i/∂x_j + ∂u_j/∂x_i) captures the symmetric part of the displacement gradient, neglecting higher-order terms and assuming rotations do not contribute to strain. The foundational concepts of stress and strain trace back to early continuum mechanics, with Leonhard Euler and developing initial ideas on deformation and internal forces in the , while Cauchy's work in the 1820s formalized the stress tensor and clarified strain as a deformation measure independent of rigid-body motions.

Hooke's Law

Hooke's law describes the fundamental linear relationship between stress and strain in elastic materials. In the simplest uniaxial case, it states that the normal stress σ\sigma is directly proportional to the corresponding normal strain ϵ\epsilon, expressed as σ=Eϵ,\sigma = E \epsilon, where EE is a material constant known as the elastic modulus. This relation implies that the deformation produced by a force is recoverable upon removal of the load, provided the material remains within its elastic limit. For more complex loading in three dimensions, Hooke's law generalizes to a tensor form, σij=Cijklϵkl,\sigma_{ij} = C_{ijkl} \epsilon_{kl}, where σij\sigma_{ij} is the stress tensor, ϵkl\epsilon_{kl} is the strain tensor, and CijklC_{ijkl} is the fourth-rank stiffness tensor that encapsulates the material's elastic properties; summation over repeated indices kk and ll is implied. The law originated with , a 17th-century English , who first hinted at the proportionality in 1676 through a Latin ("ceiiinosssttuv") in a letter to the Royal Society, and fully published it in 1678 in his work De potentia restitutiva, or of Spring. Hooke's empirical observation stemmed from experiments with springs and wires, capturing the restorative force in elastic bodies. In the early 1820s, French mathematicians and advanced this into a rigorous continuum framework, deriving the general equations of by incorporating stress-strain relations into the balance of linear momentum, thus enabling analysis of deformable solids beyond simple one-dimensional cases. Hooke's law relies on key assumptions to ensure its linearity: deformations must be small (typically strains less than 0.1–1%, depending on the material) to maintain geometric linearity and avoid nonlinear effects; the stress-strain response must be linear, meaning no higher-order terms in the constitutive relation; and the behavior is time-independent, neglecting rate-dependent phenomena like or creep. These conditions align the law with reversible, elastic deformations in homogeneous materials. However, the law has limitations in its applicability. It holds only up to the proportional limit or yield point, beyond which the stress-strain curve deviates from , leading to permanent deformation rather than full recovery. Additionally, the simple forms often assume material , where elastic properties are direction-independent; anisotropic materials require the full tensorial description without such simplification. A practical example illustrates the uniaxial application: consider a cylindrical wire of original length LL, cross-sectional area AA, subjected to a tensile FF. The axial stress is σ=F/A\sigma = F / A, and by , the axial strain is ϵ=σ/E=F/(AE)\epsilon = \sigma / E = F / (A E). The resulting elongation (displacement) is then ΔL=ϵL=FL/(AE)\Delta L = \epsilon L = F L / (A E), showing how the load induces a proportional extension that vanishes when the is removed, assuming operation within the elastic regime. This derivation directly ties the applied load to measurable displacement, forming the basis for calculations in tension members.

Definition and Properties

Definition of Elastic Modulus

The elastic modulus is a fundamental material property that quantifies the relationship between stress and strain within the linear elastic regime, serving as the constant of proportionality in . This law posits that, for small deformations, the applied stress σ\sigma is directly proportional to the resulting strain ϵ\epsilon, expressed mathematically as: E=σϵE = \frac{\sigma}{\epsilon} where EE denotes the elastic modulus. The SI unit of elastic modulus is the pascal (Pa), equivalent to newtons per square meter (N/m²), though values are commonly reported in gigapascals (GPa) for practical engineering contexts due to their typical magnitude. Physically, the elastic modulus represents a material's stiffness, or its resistance to deformation under an applied load, indicating how much stress is required to produce a unit strain. This measure applies specifically to elastic deformation, which is reversible and occurs when atomic bonds stretch temporarily without permanent rearrangement; in contrast, exceeding the elastic limit leads to plastic deformation, where the material undergoes irreversible changes in shape. For more complex loading scenarios beyond simple uniaxial tension, the elastic modulus concept generalizes to a collection of elastic constants that fully describe the material's response, relating the full stress tensor to the strain tensor in multidimensional space. To illustrate the range of across materials, exhibits an elastic modulus of approximately 200 GPa, enabling it to withstand significant loads with minimal deformation, whereas rubber has a much lower value of about 0.01 GPa, allowing substantial elastic stretching.

Distinction Between Elastic Constants and Moduli

In materials science, elastic constants denote the components of the fourth-rank stiffness tensor CijklC_{ijkl}, which linearly relates the stress tensor σij\sigma_{ij} to the strain tensor ϵkl\epsilon_{kl} via the generalized form of Hooke's law: σij=Cijklϵkl\sigma_{ij} = C_{ijkl} \epsilon_{kl}. For a fully anisotropic material with triclinic symmetry, symmetries inherent to the stress and strain tensors (such as Cijkl=Cjikl=Cijlk=CklijC_{ijkl} = C_{jikl} = C_{ijlk} = C_{klij}) reduce the potential 81 components to 21 independent elastic constants, fully characterizing the material's stiffness in all directions. Elastic moduli, on the other hand, are specific scalar measures derived from these constants that quantify a material's resistance to particular deformation modes under controlled stress conditions. Examples include EE, which describes uniaxial extension or compression; the GG, which governs resistance to shear deformation; and the KK, which measures volumetric response to hydrostatic pressure. These moduli simplify analysis for engineering applications but apply directly only to scenarios matching their defined deformation type. In isotropic materials, where properties are uniform in all directions, the distinction blurs into equivalence, as the tensor reduces to just two independent constants—such as the λ\lambda (relating to volumetric changes) and μ\mu (the )—from which all scalar moduli can be expressed through algebraic relations. This reduction stems from the material's , eliminating directional dependence and allowing a complete description with minimal parameters. Historically, the concept originated with Thomas Young's 1807 introduction of the "modulus of elasticity" as a scalar quantity for longitudinal stiffness in beams and wires, reflecting early focus on simple deformations in isotropic contexts. Over time, as understanding of crystal anisotropy advanced in the 19th and 20th centuries, the terminology expanded to encompass the full tensorial framework of elastic constants, accommodating complex directional behaviors in crystalline solids. For example, isotropic materials like polycrystalline metals require only two constants to predict all elastic responses, whereas triclinic crystals, lacking higher symmetry, demand the full 21 independent constants to accurately model deformations in arbitrary directions.

Moduli for Isotropic Materials

Young's Modulus

Young's modulus, often denoted as EE, quantifies a material's stiffness under uniaxial loading and is defined as the ratio of applied stress σ\sigma to the resulting axial strain ϵ\epsilon within the linear elastic regime for both tensile and compressive conditions. This measure arises from Hooke's law applied to one-dimensional deformation, where E=σϵE = \frac{\sigma}{\epsilon}, and it remains constant up to the material's proportional limit. The units of Young's modulus are typically gigapascals (GPa) in engineering contexts, reflecting its role in predicting how materials resist elongation or shortening without permanent deformation. Young's modulus is commonly determined through , following standards such as ASTM E111, which outlines procedures for measuring the modulus in structural materials by applying controlled loads and recording load-displacement to compute the of the stress-strain in the elastic region. For a simple cylindrical specimen or rod of LL and cross-sectional area AA subjected to an axial FF, the resulting change in ΔL\Delta L is given by ΔL=FLAE.\Delta L = \frac{F L}{A E}. This equation enables direct calculation of EE from experimental measurements of ΔL\Delta L. In practice, extensometers or strain gauges ensure precise strain assessment during testing to avoid errors from machine compliance. The value of Young's modulus exhibits temperature dependence, with examples in metallic alloys showing variations that influence material performance in thermal environments. Such behavior underscores the need to consider operating conditions in design, particularly for components exposed to temperature fluctuations. In engineering applications, Young's modulus is essential for analyzing beam deflection and structural integrity, where higher values indicate greater resistance to bending under load. For example, the used in the has a Young's modulus of approximately 190 GPa, enabling the structure to withstand wind and gravitational forces while minimizing deflection and ensuring stability. Young's modulus also connects to ν\nu, defined as the negative ratio of lateral strain to axial strain under uniaxial stress, which describes the material's transverse contraction during axial extension. This relation aids in predicting volumetric changes but is considered alongside EE for complete elastic characterization.

Shear Modulus and Bulk Modulus

The , also known as the modulus of rigidity and denoted by GG, quantifies a material's resistance to shear deformation, which involves angular distortion without significant volume change. It is defined as the ratio of τ\tau (the force per unit area acting parallel to a surface) to shear strain γ\gamma (the angular displacement or tangent of the shear angle), expressed as G=τγG = \frac{\tau}{\gamma}. This modulus is particularly relevant for analyzing torsional loading in structural components like shafts and beams, where materials undergo ./20%3A_Miscellaneous/20.03%3A_Shear_Modulus_and_Torsion_Constant) In torsion tests, the shear modulus governs the relationship between applied torque and resulting twist. For a circular shaft of length LL subjected to torque TT, the angle of twist θ\theta (in radians) is given by θ=TLGJ,\theta = \frac{T L}{G J}, where JJ is the polar moment of inertia of the cross-section. This equation allows determination of GG by measuring θ\theta, TT, LL, and calculating JJ. Torsion tests, often conducted using specialized machines that apply controlled torque while recording angular deflection, provide direct measurement of GG for metals and polymers, ensuring the material remains in the elastic regime. The bulk modulus, denoted KK, measures a material's resistance to uniform volumetric compression or expansion under hydrostatic pressure, focusing on changes in volume rather than shape. It is defined as K=VΔPΔVK = -V \frac{\Delta P}{\Delta V}, where VV is the initial volume, ΔP\Delta P is the infinitesimal change in hydrostatic pressure applied equally from all directions, and ΔV\Delta V is the resulting volume change; the negative sign accounts for volume decrease under increased pressure. The reciprocal of the bulk modulus, 1K\frac{1}{K}, is the compressibility, indicating how readily a material's volume alters under pressure. Hydrostatic conditions ensure no shear components, isolating pure volumetric response, as in pressurized fluids or confined solids. The concept of bulk modulus emerged in the mid-19th century amid advancements in continuum mechanics and thermodynamics. Bulk modulus is commonly measured using ultrasonic techniques, which exploit the relationship between wave speed and elastic properties. The speed of longitudinal waves cLc_L in a material relates to KK via cL=K+43Gρc_L = \sqrt{\frac{K + \frac{4}{3}G}{\rho}}
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