Particle Astrophysics — MCQs August 20, 2025 by u930973931_answers 50 Score: 0 Attempted: 0/50 Subscribe 1. What are neutrinos primarily produced by in astrophysical sources? (A) Nuclear reactors (B) Cosmic rays interactions (C) Black holes (D) Pulsars 2. Which type of neutrino was first detected experimentally? (A) Electron neutrino (B) Muon neutrino (C) Tau neutrino (D) Sterile neutrino 3. The first detection of solar neutrinos was made by: (A) Homestake experiment (B) IceCube (C) Super-Kamiokande (D) SNO 4. The Super-Kamiokande detector is located in: (A) USA (B) Japan (C) Canada (D) Switzerland 5. Which particle is the primary candidate for dark matter? (A) Proton (B) Neutrino (C) WIMP (D) Photon 6. Axions are hypothetical particles proposed to solve: (A) Dark matter problem (B) Strong CP problem (C) Inflation theory (D) Neutrino oscillations 7. Neutrino oscillations provide evidence that neutrinos: (A) Are massless (B) Have mass (C) Travel faster than light (D) Are photons 8. Which detector is located at the South Pole to detect high-energy neutrinos? (A) SNO (B) LUX (C) IceCube (D) XENON1T 9. Cosmic rays are primarily composed of: (A) Electrons (B) Protons (C) Neutrons (D) Photons 10. The highest-energy cosmic rays are called: (A) Gamma rays (B) Ultra-high-energy cosmic rays (C) X-rays (D) Neutrino showers 11. The Greisen–Zatsepin–Kuzmin (GZK) limit applies to: (A) Neutrinos (B) Cosmic rays (C) Photons (D) Axions 12. What is the approximate GZK cutoff energy? (A) 10^15 eV (B) 10^18 eV (C) 5 × 10^19 eV (D) 10^22 eV 13. Which particle was discovered first at CERN in 2012? (A) Higgs boson (B) Graviton (C) Tau neutrino (D) Axion 14. Which interaction is responsible for neutrino detection? (A) Gravitational (B) Weak nuclear (C) Strong nuclear (D) Electromagnetic 15. What is the mean free path of a neutrino through matter? (A) Very short (B) Moderate (C) Extremely long (D) Zero 16. Cosmic rays were first discovered by: (A) Victor Hess (B) Albert Einstein (C) Enrico Fermi (D) Carl Anderson 17. The first antiparticle discovered was: (A) Antiproton (B) Positron (C) Antineutron (D) Anti-neutrino 18. Which experiment first detected atmospheric neutrino oscillations? (A) Super-Kamiokande (B) IceCube (C) LHC (D) SNO 19. Dark matter detectors like XENON1T use: (A) Liquid Argon (B) Liquid Xenon (C) Water Cherenkov (D) Scintillators 20. Which experiment confirmed solar neutrino oscillations? (A) SNO (Sudbury Neutrino Observatory) (B) IceCube (C) LHC (D) Kamiokande 21. Which cosmic particles produce extensive air showers? (A) Neutrinos (B) Protons in cosmic rays (C) Photons (D) Electrons 22. Which detector studies cosmic-ray induced air showers? (A) Pierre Auger Observatory (B) Super-Kamiokande (C) IceCube (D) XENONnT 23. Neutrino masses are measured in: (A) GeV (B) MeV (C) eV (D) TeV 24. Sterile neutrinos interact only via: (A) Weak force (B) Electromagnetism (C) Gravity (D) Strong force 25. Which particle is its own antiparticle? (A) Photon (B) Electron (C) Proton (D) Neutrino (Majorana type) 26. Which process produces high-energy gamma rays in space? (A) Synchrotron radiation (B) Nuclear decay (C) Pair annihilation (D) All of the above 27. The detection of neutrinos from SN1987A confirmed: (A) Existence of black holes (B) Core-collapse supernova theory (C) Higgs boson (D) Inflation theory 28. Cosmic rays deflect in space due to: (A) Gravity (B) Magnetic fields (C) Neutrino interactions (D) Dark energy 29. The flux of solar neutrinos observed was lower than predicted. This is called: (A) Neutrino deficit problem (B) Dark matter problem (C) Solar wind problem (D) Proton decay problem 30. Which particle has not yet been directly detected? (A) WIMPs (B) Neutrinos (C) Protons (D) Electrons 31. High-energy astrophysical neutrinos are detected using: (A) Cherenkov radiation (B) X-rays (C) Gamma rays (D) Synchrotron light 32. The Cherenkov light in neutrino detectors is produced when: (A) Neutrinos emit photons (B) Charged particles move faster than light in a medium (C) Neutrinos collide with protons (D) Dark matter decays 33. Cosmic rays interacting with Earth’s atmosphere produce: (A) Neutrinos (B) Muons (C) Pions (D) All of the above 34. Which of the following is a lepton? (A) Proton (B) Neutron (C) Muon (D) Pion 35. Which particle explains CP violation in particle physics? (A) Neutrino (B) Kaon (C) Proton (D) Photon 36. Which astrophysical object is a potential accelerator of cosmic rays? (A) Supernova remnants (B) Neutron stars (C) Active galactic nuclei (D) All of the above 37. The highest-energy neutrinos detected by IceCube are nicknamed: (A) GZK neutrinos (B) Cosmogenic neutrinos (C) PeV neutrinos (D) Solar neutrinos 38. Which neutrino detector is based in Canada? (A) Super-Kamiokande (B) SNO (C) IceCube (D) Borexino 39. Which element is often used as a target in neutrino experiments? (A) Lead (B) Water (C) Chlorine (D) All of the above 40. Who proposed that cosmic rays are accelerated by shock waves in supernova remnants? (A) Fermi (B) Einstein (C) Zwicky (D) Gamow 41. Which symmetry predicts the existence of supersymmetric particles? (A) CP symmetry (B) Lorentz symmetry (C) Supersymmetry (SUSY) (D) Gauge symmetry 42. Which particle could be a candidate for hot dark matter? (A) Photon (B) Neutrino (C) WIMP (D) Axion 43. The term “cosmic ray shower” refers to: (A) Neutrinos from the Sun (B) Cascade of secondary particles in the atmosphere (C) Radiation from black holes (D) X-rays from quasars 44. Which experiment looks for neutrinoless double-beta decay? (A) GERDA (B) IceCube (C) SNO (D) Super-Kamiokande 45. Which cosmic messenger can escape dense astrophysical regions? (A) Protons (B) Neutrinos (C) Photons (D) Heavy ions 46. What is the rest mass of a photon? (A) Zero (B) Very small (C) 1 eV (D) 10 eV 47. Cosmic rays were originally called: (A) Cosmic photons (B) Cosmic electrons (C) Cosmic radiation (D) Solar winds 48. Which experiment studies gamma-ray bursts in relation to neutrinos? (A) IceCube (B) Super-Kamiokande (C) Auger Observatory (D) XENON1T 49. Which particle might explain both dark matter and CP violation? (A) Axion (B) Photon (C) Higgs boson (D) Tau neutrino 50. The detection of gravitational waves combined with neutrino signals is called: (A) Multimessenger astrophysics (B) Neutrino astronomy (C) Gamma-ray astronomy (D) Cosmic ray physics