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    Standard Model

    192 курсов
    Cosmology and Particle Physics - Class 3
    ICTP-SAIFR

    Cosmology and Particle Physics - Class 3

    Open Problems in Particle Physics - Class 3
    ICTP-SAIFR

    Open Problems in Particle Physics - Class 3

    Constraints on the Parameters of the Neutrino Extension of the Standard Model
    Bogolyubov Institute for Theoretical Physics

    Constraints on the Parameters of the Neutrino Extension of the Standard Model

    Simple and Efficient Public-Key Encryption from Computational Diffie-Hellman in the Standard Model
    TheIACR

    Simple and Efficient Public-Key Encryption from Computational Diffie-Hellman in the Standard Model

    Weak Decays as a Window to New Physics
    APS Physics

    Weak Decays as a Window to New Physics

    The Discovery and Characterization of a Higgs Boson
    APS Physics

    The Discovery and Characterization of a Higgs Boson

    Smoothing the Gap Between NP and ER
    IEEE

    Smoothing the Gap Between NP and ER

    Accelerate, Collide, Detect
    World Science Festival

    Accelerate, Collide, Detect

    Nature's Constituents
    World Science Festival

    Nature's Constituents

    The Elusive Neutrino and the Nature of the Cosmos
    World Science Festival

    The Elusive Neutrino and the Nature of the Cosmos

    Formal Abstractions for Attested Execution Secure Processors
    TheIACR

    Formal Abstractions for Attested Execution Secure Processors

    Mysteries of Matter at the LHC
    The Royal Institution

    Mysteries of Matter at the LHC

    Detecting Ultralight Axions with Black Holes and Gravitational Waves
    BIMSA

    Detecting Ultralight Axions with Black Holes and Gravitational Waves

    How Bright is the Proton? A Precise Determination of the Photon Parton Distribution Function
    BIMSA

    How Bright is the Proton? A Precise Determination of the Photon Parton Distribution Function

    Cosmological Relaxation of the Electroweak Scale
    BIMSA

    Cosmological Relaxation of the Electroweak Scale

    Magnetic Field Effect on Higgs Boson Production Rate Through Gluon Fusion
    ICTP-SAIFR

    Magnetic Field Effect on Higgs Boson Production Rate Through Gluon Fusion

    Searching for Surprises at the Highest Energies
    Imperial College London

    Searching for Surprises at the Highest Energies

    Standard Model and Beyond - Class 3
    ICTP-SAIFR

    Standard Model and Beyond - Class 3

    Standard Model and Beyond - Class 2
    ICTP-SAIFR

    Standard Model and Beyond - Class 2

    Neutrino Physics - Class 4
    ICTP-SAIFR

    Neutrino Physics - Class 4

    Neutrinos Beyond the Standard Model - Class 1
    ICTP-SAIFR

    Neutrinos Beyond the Standard Model - Class 1