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  2. Supernova neutrinos - Wikipedia

    en.wikipedia.org/wiki/Supernova_Neutrinos

    Supernova neutrinos are weakly interactive elementary particles produced during a core-collapse supernova explosion. [1] A massive star collapses at the end of its life, emitting on the order of 10 58 neutrinos and antineutrinos in all lepton flavors. [2] The luminosity of different neutrino and antineutrino species are roughly the same. [3]

  3. Two-photon physics - Wikipedia

    en.wikipedia.org/wiki/Two-photon_physics

    A Feynman diagram (box diagram) for photon–photon scattering: one photon scatters from the transient vacuum charge fluctuations of the other. Two-photon physics, also called gamma–gamma physics, is a branch of particle physics that describes the interactions between two photons.

  4. Strongly interacting massive particle - Wikipedia

    en.wikipedia.org/wiki/Strongly_interacting...

    Strongly interacting massive particles have been proposed as a solution for the ultra-high-energy cosmic-ray problem [4] [5] and the absence of cooling flows in galactic clusters. [ 6 ] [ 7 ] Various experiments and observations have set constraints on SIMP dark matter from 1990 onward.

  5. Weakly interacting massive particle - Wikipedia

    en.wikipedia.org/wiki/Weakly_interacting_massive...

    Weakly interacting massive particles (WIMPs) are hypothetical particles that are one of the proposed candidates for dark matter.. There exists no formal definition of a WIMP, but broadly, it is an elementary particle which interacts via gravity and any other force (or forces) which is as weak as or weaker than the weak nuclear force, but also non-vanishing in strength.

  6. Fluidized bed reactor - Wikipedia

    en.wikipedia.org/wiki/Fluidized_bed_reactor

    A fluidized bed reactor (FBR) is a type of reactor device that can be used to carry out a variety of multiphase chemical reactions. In this type of reactor, a fluid (gas or liquid) is passed through a solid granular material (usually a catalyst) at high enough speeds to suspend the solid and cause it to behave as though it were a fluid.

  7. Neutrino astronomy - Wikipedia

    en.wikipedia.org/wiki/Neutrino_astronomy

    Neutrinos are very hard to detect due to their non-interactive nature. In order to detect neutrinos, scientists have to shield the detectors from cosmic rays, which can penetrate hundreds of meters of rock. Neutrinos, on the other hand, can go through the entire planet without being absorbed, like "ghost particles".

  8. Cloud chamber - Wikipedia

    en.wikipedia.org/wiki/Cloud_chamber

    The bubble chamber similarly reveals the tracks of subatomic particles, but inverts the principle of the cloud chamber to detect them as trails of bubbles in a superheated liquid, usually liquid hydrogen, rather than as trails of drops in a supercritical vapor. Bubble chambers can be made physically larger than cloud chambers, and since they ...

  9. Collision theory - Wikipedia

    en.wikipedia.org/wiki/Collision_theory

    For particles in a solution, an example model to calculate the collision frequency and associated coagulation rate is the Smoluchowski coagulation equation proposed by Marian Smoluchowski in a seminal 1916 publication. [4] In this model, Fick's flux at the infinite time limit is used to mimic the particle speed of the collision theory.