Dark Matter and Dark Energy | 24 Dec 2024

Source: TH 

Why in News?  

Recently, physicists revised the minimum mass of dark matter and pushed it up to 2.3 × 10-30 proton masses.  

• For decades scientists thought this minimum mass was about 10-31 times the mass of a proton.

What is Dark Matter? 

• About: Dark matter is a form of matter that is entirely invisible, emitting no light or energy, making it undetectable by conventional sensors and detectors. 
  • Dark matter doesn't interact with electromagnetic forces, so it neither absorbs, reflects, nor emits light, making it hard to detect. 
  • Dark matter makes up about 27% of the universe, outweighing visible matter six to one, while visible matter accounts for only 5%. 
  • Visible matter (Baryonic matter) consists of subatomic particles like protons, neutrons, and electrons. 

• Composition of Dark Matter: Dark matter is thought to consist of non-baryonic WIMPs (weakly interacting massive particles), 10-100 times the mass of a proton, but weakly interacts with normal matter, making detection difficult. Among WIMPs are: 
  • Neutralinos: They are hypothetical particles (not yet been observed) that are heavier and slower than neutrinos. 
  • Sterile Neutrinos: Sterile neutrino is proposed as a dark matter candidate as it only interacts with regular matter through gravity. Also, neutrinos are particles that don't form regular matter. 
• Origin of Dark Matter:  
  • Big Bang Theory: Dark matter may have formed during the Big Bang and concentrated into black holes, where their gravitational forces trap dark matter particles. 
  • Stellar Remnants: Stellar remnants such as white dwarfs and neutron stars are also thought to contain high amounts of dark matter.  
    • Brown dwarfs (failed stars) that didn't accumulate enough material to kick-start nuclear fusion in their cores can also be a source of dark matters.  
• Evidence of Dark Matter:  
  • Galaxy Rotation Curves: According to Newtonian gravity, objects at the edge of galaxies should be moving slower than those near the center.  
    • Observations show stars on galaxy edges move faster than expected, suggesting unseen mass—attributed to dark matter—provides extra gravitational pull. 
  • Gravitational Lensing: Gravitational lensing occurs when light is bent by a massive object's gravity, revealing more mass than visible, suggesting the presence of dark matter. 
  • Galaxy Formation: Galaxies' distribution and motion over time suggest dark matter, as it enables galaxies to clump together and form current structures. 
• Projects to Study Dark Matter: There are some key projects designed to shed light on dark matter. 
  • Alpha Magnetic Spectrometer (AMS): The AMS is an experiment mounted on the International Space Station which has detected an excess of positrons (the antimatter counterpart to electrons), which may be a signature of dark matter. 
  • XENON1T: The XENON1T experiment in the Italian Gran Sasso Laboratory aims to detect dark matter by observing the interactions of WIMPs with xenon atoms. 
  • IceCube Neutrino Observatory, Antarctica: The IceCube Neutrino Observatory is investigating the possibility of sterile neutrinos—hypothetical particles that only interact with regular matter via gravity and could be a form of dark matter. 
  • Particle Colliders at CERN, Switzerland: CERN's Large Hadron Collider (LHC) conducts high-energy particle collisions to probe the fundamental particles of the universe. The LHC also looks for potential signs of dark matter by analyzing the aftermath of particle collisions. 
  • James Webb Space Telescope (JWST): JWST is expected to provide valuable insights into how galaxies and cosmic structures developed, which could help us understand the role of dark matter in their formation. 

What is Dark Energy? 

• Dark energy is a mysterious form of energy that makes up about 68% of the universe. It is thought to be responsible for the accelerated expansion of the universe.  
• It is distributed evenly throughout the universe, not only in space but also in time i.e., its effect is not diluted as the universe expands.  
• The even distribution means that dark energy does not have any local gravitational effects, but rather a global effect on the universe as a whole.  
  • This leads to a repulsive force, which tends to accelerate the expansion of the universe.  
• The rate of expansion and its acceleration can be measured by observations based on the Hubble law. 
  • Hubble's Law states that galaxies move faster away from Earth as they are farther, implying the universe is expanding. 

Conclusion 

Dark matter, making up a significant portion of the universe, remains elusive yet crucial for understanding cosmic structures and evolution. Ongoing experiments and astronomical observations continue to explore its properties, origin, and impact, promising advancements in fundamental physics.