User:Carchasm/sandbox/List of unsolved problems in physics

Source: Wikipedia, the free encyclopedia.

The following is a list of notable unsolved problems grouped into broad areas of physics.[1]

Some of the major unsolved problems in physics are theoretical, meaning that existing theories seem incapable of explaining a certain observed phenomenon or experimental result. The others are experimental, meaning that there is a difficulty in creating an experiment to test a proposed theory or investigate a phenomenon in greater detail.

There are still some questions

event horizon
).

Theories of Everything

Is there a theory which explains the values of all

temporal dimension? Are "fundamental physical constants" really fundamental or do they vary over time? Are any of the fundamental particles in the standard model of particle physics actually composite particles too tightly bound to observe as such at current experimental energies? Are there elementary particles that have not yet been observed, and, if so, which ones are they and what are their properties? Are there unobserved fundamental forces
?

Supersymmetry

Quantum Loop Gravity

String Theory

Physics beyond the Standard Model

Simulated Large Hadron Collider CMS particle detector data depicting a Higgs boson produced by colliding protons decaying into hadron jets and electrons

The Standard Model of

experimental predictions
, it leaves some phenomena unexplained. Some of the most notable issues with the standard model include:

Quantum gravity

The standard model does not explain gravity. The approach of simply adding a graviton to the Standard Model does not recreate what is observed experimentally without other modifications, as yet undiscovered, to the Standard Model. Moreover, the Standard Model is widely considered to be incompatible with the most successful theory of gravity to date, general relativity.[6]

Dark matter

Cosmological observations tell us the standard model explains about 5% of the energy present in the universe. About 26% should be dark matter,[citation needed] which would behave just like other matter, but which only interacts weakly (if at all) with the Standard Model fields. Yet, the Standard Model does not supply any fundamental particles that are good dark matter candidates.

Dark energy

The remaining 69% of universe's energy should consist of the so-called dark energy, a constant energy density for the vacuum. Attempts to explain dark energy in terms of vacuum energy of the standard model lead to a mismatch of 120 orders of magnitude.[7]

Neutrino masses

According to the standard model, neutrinos are massless particles. However, neutrino oscillation experiments have shown that neutrinos do have mass. Mass terms for the neutrinos can be added to the standard model by hand, but these lead to new theoretical problems. For example, the mass terms need to be extraordinarily small and it is not clear if the neutrino masses would arise in the same way that the masses of other fundamental particles do in the Standard Model.

Matter–antimatter asymmetry

The universe is made out of mostly matter. However, the standard model predicts that matter and antimatter should have been created in (almost) equal amounts if the initial conditions of the universe did not involve disproportionate matter relative to antimatter. Yet, there is no mechanism in the Standard Model to sufficiently explain this asymmetry.[citation needed]

Anomalous magnetic dipole moment of the muon

The experimentally measured value of muon's anomalous magnetic dipole moment (muon "g − 2") is significantly different from the Standard Model prediction.[8]

Hierarchy problem

The standard model introduces particle masses through a process known as spontaneous symmetry breaking caused by the Higgs field. Within the standard model, the mass of the Higgs gets some very large quantum corrections due to the presence of virtual particles (mostly virtual top quarks). These corrections are much larger than the actual mass of the Higgs. This means that the bare mass parameter of the Higgs in the standard model must be fine tuned in such a way that almost completely cancels the quantum corrections.[9] This level of fine-tuning is deemed unnatural by many theorists.[who?]

Strong CP Problem

Theoretically it can be argued that the standard model should contain a term that breaks

CP symmetry—relating matter to antimatter—in the strong interaction sector. Experimentally, however, no such violation has been found, implying that the coefficient of this term is very close to zero.[10]

Cosmology and Astrophysics

Black Holes

Origin of the Universe

Structure of the Universe

  • Problem of time: In quantum mechanics time is a classical background parameter and the flow of time is universal and absolute. In general relativity time is one component of four-dimensional spacetime, and the flow of time changes depending on the curvature of spacetime and the spacetime trajectory of the observer. How can these two concepts of time be reconciled?[13]
  • self-sustaining through inflation of quantum-mechanical fluctuations, and thus ongoing in some extremely distant place?[14]
  • Dark flow: Is a non-spherically symmetric gravitational pull from outside the observable universe responsible for some of the observed motion of large objects such as galactic clusters in the universe?
  • Axis of evil: Some large features of the microwave sky at distances of over 13 billion light years appear to be aligned with both the motion and orientation of the solar system. Is this due to systematic errors in processing, contamination of results by local effects, or an unexplained violation of the Copernican principle?

Quantum Mechanics

  • Locality: Are there non-local phenomena in quantum physics?[18][19] If they exist, are non-local phenomena limited to the entanglement revealed in the violations of the Bell inequalities, or can information and conserved quantities also move in a non-local way? Under what circumstances are non-local phenomena observed? What does the existence or absence of non-local phenomena imply about the fundamental structure of spacetime? How does this elucidate the proper interpretation of the fundamental nature of quantum physics?

Quantum Field Theory

  • Color confinement: The quantum chromodynamics (QCD) color confinement conjecture is that color charged particles (such as quarks and gluons) cannot be separated from their parent hadron without producing new hadrons.[21] Is it possible to provide an analytic proof of color confinement in any non-abelian gauge theory?
  • quantum vacuum have little effect on the expansion of the universe?[24]
  • Quantum gravity: Can quantum mechanics and general relativity be realized as a fully consistent theory (perhaps as a quantum field theory)?[25] Is spacetime fundamentally continuous or discrete? Would a consistent theory involve a force mediated by a hypothetical graviton, or be a product of a discrete structure of spacetime itself (as in loop quantum gravity)? Are there deviations from the predictions of general relativity at very small or very large scales or in other extreme circumstances that flow from a quantum gravity mechanism?

Nuclear and particle physics

  • charge quantization.)[26]
  • Neutron lifetime puzzle: While the neutron lifetime has been studied for decades, there currently exists a lack of consilience on its exact value, due to different results from two experimental methods ("bottle" versus "beam").[27]
  • Yukawa couplings)?[28]
  • Proton radius puzzle: What is the electric charge radius of the proton? How does it differ from gluonic charge?
  • Pentaquarks and other exotic hadrons: What combinations of quarks are possible? Why were pentaquarks so difficult to discover?[29] Are they a tightly-bound system of five elementary particles, or a more weakly-bound pairing of a baryon and a meson?[30]
The "island of stability" in the proton vs. neutron number plot for heavy nuclei

Fluid dynamics

Turbulence in the tip vortex from an airplane wing passing through coloured smoke

Condensed matter physics

BSCCO
). The mechanism for superconductivity of these materials is unknown.
  • High-temperature superconductors: What is the mechanism that causes certain materials to exhibit superconductivity at temperatures much higher than around 25 kelvins? Is it possible to make a material that is a superconductor at room temperature and atmospheric pressure?[4]
  • Amorphous solids: What is the nature of the glass transition between a fluid or regular solid and a glassy phase? What are the physical processes giving rise to the general properties of glasses and the glass transition?[31][32]
  • Fractional Hall effect
    : What mechanism explains the existence of the state in the fractional
    non-Abelian fractional statistics?[33]
Magnetoresistance in a fractional quantum Hall state.
  • Metal whiskering: In electrical devices, some metallic surfaces may spontaneously grow fine metallic whiskers, which can lead to equipment failures. While compressive mechanical stress is known to encourage whisker formation, the growth mechanism has yet to be determined.
  • Superfluid transition in helium-4: Explain the discrepancy between the experimental[34] and theoretical[35][36][37] determinations of the heat capacity critical exponent α.[38]
  • Bose–Einstein condensation: How do we rigorously prove the existence of Bose–Einstein condensates for general interacting systems?[39]

Optics

See also

References

  1. .
  2. ^ Hammond, Richard (1 May 2008). "The Unknown Universe: The Origin of the Universe, Quantum Gravity, Wormholes, and Other Things Science Still Can't Explain". Proceedings of the Royal Society of London, Series A. 456 (1999): 1685.
  3. ^ Womersley, J. (February 2005). "Beyond the Standard Model" (PDF). Symmetry Magazine. Archived from the original (PDF) on 17 October 2007. Retrieved 23 November 2010.
  4. ^ a b c d e Baez, John C. (March 2006). "Open Questions in Physics". Usenet Physics FAQ. University of California, Riverside: Department of Mathematics. Retrieved 7 March 2011.
  5. ^ R. Oerter (2006). The Theory of Almost Everything: The Standard Model, the Unsung Triumph of Modern Physics (Kindle ed.). Penguin Group. p. 2. .
  6. . One can find thousands of statements in the literature to the effect that "general relativity and quantum mechanics are incompatible". These are completely outdated and no longer relevant. Effective field theory shows that general relativity and quantum mechanics work together perfectly normally over a range of scales and curvatures, including those relevant for the world that we see around us. However, effective field theories are only valid over some range of scales. General relativity certainly does have problematic issues at extreme scales. There are important problems which the effective field theory does not solve because they are beyond its range of validity. However, this means that the issue of quantum gravity is not what we thought it to be. Rather than a fundamental incompatibility of quantum mechanics and gravity, we are in the more familiar situation of needing a more complete theory beyond the range of their combined applicability. The usual marriage of general relativity and quantum mechanics is fine at ordinary energies, but we now seek to uncover the modifications that must be present in more extreme conditions. This is the modern view of the problem of quantum gravity, and it represents progress over the outdated view of the past."
  7. ^ Krauss, L. (2009). A Universe from Nothing. AAI Conference.
  8. ].
  9. ^ "The Hierarchy Problem". Of Particular Significance. 14 August 2011. Retrieved 13 December 2015.
  10. . Retrieved 15 August 2015.
  11. .
  12. ^ Joshi, Pankaj S. (January 2009). "Do Naked Singularities Break the Rules of Physics?". Scientific American. Archived from the original on 25 May 2012.
  13. S2CID 116947742
    .
  14. ^ Podolsky, Dmitry. "Top ten open problems in physics". NEQNET. Archived from the original on 22 October 2012. Retrieved 24 January 2013.
  15. ^ Cite error: The named reference newscientist was invoked but never defined (see the help page).
  16. ^ Stephen Battersby (21 June 2011). "Largest cosmic structures 'too big' for theories". New Scientist. Retrieved 5 July 2019
  17. S2CID 118419619
    .
  18. .
  19. .
  20. ^ "Yang–Mills and Mass Gap". Clay Mathematics Institute. Retrieved 31 January 2018.
  21. ^ Wu, T.-Y.; Pauchy Hwang, W.-Y. (1991). Relativistic quantum mechanics and quantum fields. .
  22. .
  23. ].
  24. ^ Cite error: The named reference :3 was invoked but never defined (see the help page).
  25. ^ Alan Sokal (22 July 1996). "Don't Pull the String Yet on Superstring Theory". New York Times.
  26. ^ Dirac, Paul, "Quantised Singularities in the Electromagnetic Field". Proceedings of the Royal Society A 133, 60 (1931).
  27. ^ Wolchover, Natalie (13 February 2018). "Neutron Lifetime Puzzle Deepens, but No Dark Matter Seen". Quanta Magazine. Retrieved 31 July 2018. When physicists strip neutrons from atomic nuclei, put them in a bottle, then count how many remain there after some time, they infer that neutrons radioactively decay in 14 minutes and 39 seconds, on average. But when other physicists generate beams of neutrons and tally the emerging protons—the particles that free neutrons decay into—they peg the average neutron lifetime at around 14 minutes and 48 seconds. The discrepancy between the "bottle" and "beam" measurements has persisted since both methods of gauging the neutron's longevity began yielding results in the 1990s. At first, all the measurements were so imprecise that nobody worried. Gradually, though, both methods have improved, and still they disagree.
  28. .
  29. ^ H. Muir (2 July 2003). "Pentaquark discovery confounds sceptics". New Scientist. Retrieved 8 January 2010.
  30. ^ G. Amit (14 July 2015). "Pentaquark discovery at LHC shows long-sought new form of matter". New Scientist. Retrieved 14 July 2015.
  31. ^ Kenneth Chang (29 July 2008). "The Nature of Glass Remains Anything but Clear". The New York Times.
  32. S2CID 28052338
    . The deepest and most interesting unsolved problem in solid state theory is probably the theory of the nature of glass and the glass transition.
  33. .
  34. .
  35. .
  36. .
  37. .
  38. .
  39. ^ Schlein, Benjamin. "Graduate Seminar on Partial Differential Equations in the Sciences – Energy and Dynamics of Boson Systems". Hausdorff Center for Mathematics. Retrieved 23 April 2012.
  40. ^ Barton, G.; Scharnhorst, K. (1993). "QED between parallel mirrors: light signals faster than c, or amplified by the vacuum".
    S2CID 120489943
    .

External links