Raising temperature reduces the extension: the entropic preference for many up/down arrangements opposes alignment by the load. For small loads, L≃Na2mg/(kBT).
For the positive-feedback entropic chain with replacement forcef(L)=f0L/a, f0>0, the conservative potential is U(L)=−∫0Lf(s)ds=−f0L2/(2a). Using −f(L)L would overcount it by a factor two. The stationary equation becomes
For T>Tc the stable extension is zero. Below Tc, nonzero minima appear, with x≃±3(Tc−T)/T close to the transition and ∣x∣→1as T→0. Restricting to downward extensions selects the positive branch. The onset is continuous in this model, with a nonanalytic mean-field change at Tc; a finite jump in L does not follow from the printed forcelaw, despite the question's discontinuity wording. A finite chain has rounded fluctuations rather than a literal thermodynamic singularity.
For charge per length λq, Gauss's law gives Er=λq/(2πϵ0r) between the conductors. Integration gives V=λqln(b/a)/(2πϵ0). Similarly Ampère's law gives Bϕ=μ0I/(2πr); integrating the magnetic energy per length and setting it equal to LI2/2 gives
Here C,L are per unit length. The displayed L is the external TEM inductance, appropriate to the ideal surface-current/high-frequencymodel. Internal magnetic energy in conductors with appreciable current penetration adds internal inductance; it cannot be determined fully from an outer conductor with unspecified wallgeometry.
A concrete test is the Casimir interaction: changing conducting boundaries changes electromagnetic ground-state modes and produces a measurable force. Ideal parallel plates have pressure
Such measurements test changes in ground-state energy, not an arbitrary absolute additive vacuum energy; real-material and thermal corrections must be included when comparing precision data.
For β≫α, they scale as V0α/β and V0(α/β)3 respectively: a narrow central perturbation couples weakly to the odd state's central node. For β≪α, both approach V0 because the perturbation is nearly constant over the wavefunctions. The leading corrections are V0[1−β2/(2α2)] and V0[1−3β2/(2α2)].
For an improved variational estimate, replace the fixed width α by an adjustable positive width s in each even/odd Gaussian. Their energyfunctionals are
Minimize each separately. At s=α they recover the unperturbed energy plus the first-order shift, so optimization cannot raise those trial estimates. For this even one-dimensional potential the lowest odd state is the first excited state, making its odd-sector minimum an upper bound on E1. Enlarging each parity-preserving trial basis can improve the estimates further.
At ω=πc/a, the radial profile is J0(πr/a): its first zero is at r≃0.765a, and the edge has opposite phase, J0(π)≃−0.304. This is an illustrative thin-disc interior profile; the exact driven high-frequencyfield also depends on the feed and edge/radiation boundary conditions. Continuing the uniform quasistatic field would be inconsistent.
Spin-zero identical particles are bosons. Both can occupy the lowest orbital, so the two-boson ground state is nondegenerate. The first excited total energy is 9E0: one particle occupies the lowest orbital and one an excited orbital. Symmetrizing the two-particle wavefunction gives one state for each of the three excited orbitals, so the first-excited degeneracy is three.
The remaining probability includes higher bound ns states and the s-waveionization continuum. In this central, instantaneous model the initial orbital has l=0,m=0, and angular orthogonality excludes states with l=0. The electronic spin is unchanged. Nuclear recoil and interactions with the emitted decay particles are outside this leading sudden-charge-change approximation.
For total relativistic energyE=γmc2, the speed is v=c1−(mc2/E)2. Both beam energies are enormously greater than the rest energy, so expanding the square root avoids obscuring the small difference:
The factor two counts polarizations; counting independent positive and negative traveling momenta in addition would double count standing modes. The thermal energy is
Replacing the mode sum by an integral requires the stated temperature to be large compared with the level-spacing scale. This is thermal energy above the vacuum contribution; a separate boundary-dependent vacuum energy is not included.
She sends two months after her twenty-ninth birthday. This compares the emission and reception events; the captains' clocks need only be synchronized at launch, not kept numerically synchronized afterward.
Equivalently, the left-going photon has Earth frequencyf0/[γA(1+3/5)]=f0/2, and Bob's frame supplies another factor γB(1−4/5)=1/3. Both methods give the same redshift.
The positive-z expression in the question takes ω=ωz^. “Clockwise” needs a viewing direction: this rotation looks clockwise when viewed looking along +z from below, and counterclockwise when viewed from the positive-z side. Looking from the other end reverses the verbal label, not the vector relation.
Since the positive charge and the loop current circulate in the same stated sense, their dipolemoments are parallel when judged from a common viewpoint. At h≫R, the loop's axial field magnitude is B≃μ0IR2/(2h3). With the sphere small compared with that variation scale,
The magnetic force is attractive, pulling the sphere toward the loop. Reversing only one circulation would reverse that magnetic force. The calculation treats the rotating charge asa prescribed moment and uses the stated separated length scales; it does not add unrelated induction or electric interactions to the dipolemodel.
Let R(θ) be the real rotation matrix with columns along the plate's fast and slow axes. Expressing the input in those axes, applying the principal retardance, then rotating back gives the rotated half-wave platematrix
The magnitude is the stated 2Ω shift. Its sign follows the explicit time and rotation conventions above; reversing the physical rotation or using the orthogonal linear input reverses the shift. Atime-phasor convention must be changed consistently with the plate matrices, rather than used alone to change a physical redshift into ablueshift.
Write the vertical complex amplitudeas Ψ(z)=a(z)eiϕ(z). A constant streamfunction phase has kx−kcrt+ϕ(z)=const, hence dx/dz=−ϕz/k. For k>0, westward tilt with height implies ϕz>0. With v′=ψx′ and b′=f0ψz′, a zonal average over the wave gives
A numerical scale estimate requires areferenceocean density and latitude not specified exactly. Taking ρ0≃1025kgm−3, g≃9.81ms−2 and a representative midlatitude ∣f∣≃10−4s−1 gives
For L=100km≫LR, rotational adjustment produces a largely retained interface displacement with a geostrophic current. Wave emission and inertial oscillations accompany the adjustment, but the balanced structure is much more important. To quantify that distinction under an initially resting, linear single-Fourier-component assumption, potential-vorticity conservation gives
This is about 0.002 for the kilometre scale and 0.95 for the hundred-kilometre scale. These fractions use Las an inverse wavenumber scale, not a full wavelength, and are illustrative rather than unique predictions for an unspecified disturbance or bounded basin.
Apply the intended, corrected dispersion relation in c. A uniform mean zonal wind gives ωground=ω+kU. Stationarity with U=−20ms−1 therefore requires eastward intrinsic phase speedω/k=−U=20ms−1. With k=1/a,
Astorm within roughly 12∘ of the equator has substantial projection on the Gaussian mode. There is no sharp latitude cutoff: ∣y∣=LD gives amplitude e−1/2 and the 1/eamplitude latitude is about 16.4∘. Forcing outside that core has progressively weaker overlap.
The intrinsic wave is eastward even though its observed ground pattern is stationary; westward advection cancels its phase propagation. Its intrinsic period is about 12.4Earthdays. The inferred ∣m∣≫1/(2H) puts it in the short-vertical-wavelength branch, well below the long-wavespeed 2NH=200ms−1. For upward energyradiation, ∂ω/∂m must be positive, which selects m<0 for positive k,ω: vertical phase propagation is then downward. Dust absorption supplies thermal forcing with a zonally asymmetric component; the response does not imply that dust itself moves eastward at the intrinsic phase speed.
For an ideal gas of fixed molecular composition, translational energy is supplemented by rotational, vibrational and eventually electronic excitationsas their level spacings become thermally accessible. Activating more internal degrees of freedom generally increases the heat capacity. In aharmonic vibrational mode the contribution rises from nearly zero when kBT≪ℏω to its classical limit when kBT≫ℏω; summing modes with different frequencies gives a smooth increase over an intermediate temperature range.