Statistical Mechanics Paper I
Publishes an early paper developing the kinetic theory of thermal equilibrium using statistical methods.
Albert Einstein ยท Place
38 Einstein records associated with Bern.

Publishes an early paper developing the kinetic theory of thermal equilibrium using statistical methods.
Appointed Technical Expert, third class, at the Swiss Patent Office in Bern.
Publishes further work on the foundations of thermodynamics and statistical mechanics.
Studies fluctuations in radiation energy, an important precursor to his later quantum work.
Einstein discussed photoionization as another possible application of localized radiation quanta, connecting the frequency of light with the energy needed to remove charged particles from matter.
Einstein distinguished brightness from frequency by predicting that raising the frequency of incident light increases the energy of individual photoelectrons rather than merely increasing their number.
Einstein's quantum account implied that increasing light intensity at fixed frequency mainly increases the number of available energy quanta and therefore the number of emitted electrons.
Einstein applied the relation between quantum energy and radiation frequency to individual light quanta, giving each localized packet an energy proportional to its frequency.
Einstein proposed that under appropriate conditions electromagnetic radiation behaves as independently localized energy quanta, extending Planck's quantum relation from material oscillators to light itself.
Einstein explicitly contrasted spatially localized light quanta with a purely continuous wave description, creating a fundamental tension that later developed into wave-particle duality.
Explains photoelectric emission by proposing that light transfers energy in discrete quanta to electrons.
Einstein explained that photoelectron emission requires incident light above a material-dependent threshold frequency, regardless of how intense lower-frequency illumination becomes.
Einstein related the maximum kinetic energy of emitted electrons to the incident light frequency minus the work required to free an electron from the material.
Einstein compared the entropy of high-frequency radiation with that of a dilute gas and found a formal similarity that supported treating radiation energy as independently distributed quanta.
Einstein used the light-quantum hypothesis to interpret Stokes's rule for fluorescence, arguing that emitted light normally cannot carry a higher quantum energy than the absorbed radiation.
Sends his light-quantum paper to Annalen der Physik, using quanta to explain the photoelectric effect.
Annalen der Physik receives Einstein's paper explaining Brownian motion through molecular collisions.
Submits On the Electrodynamics of Moving Bodies, establishing the special theory of relativity.
Submits the paper deriving the relation between mass and energy from special relativity.
Publishes a relativistic analysis linking conservation of centre-of-gravity motion with the inertia carried by energy, extending the implications of mass-energy equivalence.
Publishes work extending the light-quantum hypothesis to the production and absorption of radiation.
Einstein's continuing work on radiation treated elementary exchanges between matter and electromagnetic energy as discrete processes rather than continuously divisible transfers.
Einstein re-examined Planck's radiation theory and emphasized that its success could be understood more naturally if radiation exchanged energy with matter in finite quantum amounts.
Einstein examined how material resonators exchange energy with radiation and strengthened the case that emission as well as absorption must be connected with discrete quantum transfers.
Einstein extended his quantum reasoning to resonant interactions between matter and radiation, treating absorption as an energy exchange constrained by discrete radiation quanta.
His revised dissertation on molecular dimensions is published in Annalen der Physik.
Publishes a follow-up analysis refining his theory of Brownian motion.
Promoted to Technical Expert, second class, at the Swiss Patent Office.
Using accelerated reference frames, Einstein concluded that clocks at different gravitational potentials should not run at identical rates, linking gravity directly with the measurement of time.
Extends special-relativistic reasoning to accelerated motion and concludes that gravitation must alter measurements of time, frequency and the propagation of light.
Recognises that a uniformly accelerated frame is locally equivalent to a homogeneous gravitational field, establishing the conceptual starting point for general relativity.
Einstein recognised that an observer in sufficiently small free fall can describe local physics without an apparent gravitational force, an insight that became central to his equivalence principle.
Predicts that gravity should shift the frequency of light, later called gravitational redshift.
Einstein's equivalence reasoning implied that a gravitational field must influence light propagation, opening a path from special relativity toward a relativistic theory of gravitation.
Applies quantum ideas to the specific heat of solids, an early success of quantum theory.
Begins teaching at the University of Bern as a Privatdozent.
Works with Jakob Laub on electromagnetic equations for moving bodies, reformulating electrodynamics in a way consistent with the special theory of relativity.
Publishes a broad review of the relativity principle and its consequences, clarifying how the theory changes traditional concepts of space, time and dynamics.