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Euler Buckling Stress⚠ unverified

Mechanical / Columns · Critical buckling stress of a column

Parameters

InputSymbolUnitDefaultDescription
EEPa200000000000.0Young's modulus
IIm^41e-05Second moment of area
AAm^20.01Cross-sectional area
LLm3.0Length
KK1.0Effective-length factor
OutputSymbolUnitDescription
sigma_crσcrPaCritical stress

The science & history

Understanding the Parameters

Derivation (Approaching a Proof)

Begin with the Euler critical load (Euler Buckling Load column):

$$P_{cr} = \frac{\pi^2 E I}{(KL)^2}.$$

The buckling stress is the load divided by the area:

$$\sigma_{cr} = \frac{P_{cr}}{A} = \frac{\pi^2 E I}{(KL)^2 A}.$$

Substitute $I = A r^2$ (definition of radius of gyration) to eliminate the absolute section size:

$$\sigma_{cr} = \frac{\pi^2 E (A r^2)}{(KL)^2 A} = \frac{\pi^2 E}{(KL/r)^2} = \frac{\pi^2 E}{\lambda^2}.$$

The area cancels, leaving buckling stress as a function of material stiffness and slenderness only. This is the key insight: for a slender column, allowable stress is set by geometry (slenderness), not by material strength. The curve $\sigma_{cr}(\lambda) = \pi^2 E/\lambda^2$ is truncated at $\sigma_{cr}=\sigma_y$, defining the transition slenderness (Critical Slenderness).

Dimensional check. $[\sigma_{cr}] = \dfrac{\text{Pa}}{(\text{dimensionless})^2} = \text{Pa}$. ✓

History and Development

Recasting Euler's 1744 load as a stress-vs-slenderness curve was the 19th-century engineering contribution that made buckling usable in design. Plotting $\sigma_{cr}$ against $\lambda$ exposed the gap at low slenderness where real columns failed early, motivating the Rankine–Gordon, Johnson parabola (Intermediate Column Load), and tangent-modulus theories, and ultimately the smooth column curves of AISC and Eurocode 3.

Related Concepts: Euler Buckling Load column, Slenderness Ratio, Critical Slenderness, Intermediate Column Load, Factor of Safety, Radius of Gyration

Notes: Valid only where $\sigma_{cr} \le \sigma_y$ (slender columns). For short/intermediate columns use $\min(\sigma_y, \sigma_{cr})$ or the Johnson parabola. Real columns with initial crookedness and eccentricity buckle below the ideal $\sigma_{cr}$ — see Secant Formula Stress.

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