Skip to main content

Introduction to High Energy Physics

  • Chapter
  • First Online:
Inclusive b Jet Production in Proton-Proton Collisions

Part of the book series: Springer Theses ((Springer Theses))

  • 278 Accesses

Abstract

The object of High Energy Physics is the study the constituents of matter and their interactions at quantic and relativistic scales, conditions only reachable with very high energies. At these scales, matter and interactions are both described in terms of particles.

This is a preview of subscription content, log in via an institution to check access.

Access this chapter

Chapter
USD 29.95
Price excludes VAT (USA)
  • Available as PDF
  • Read on any device
  • Instant download
  • Own it forever
eBook
USD 84.99
Price excludes VAT (USA)
  • Available as EPUB and PDF
  • Read on any device
  • Instant download
  • Own it forever
Softcover Book
USD 109.99
Price excludes VAT (USA)
  • Compact, lightweight edition
  • Dispatched in 3 to 5 business days
  • Free shipping worldwide - see info
Hardcover Book
USD 109.99
Price excludes VAT (USA)
  • Durable hardcover edition
  • Dispatched in 3 to 5 business days
  • Free shipping worldwide - see info

Tax calculation will be finalised at checkout

Purchases are for personal use only

Institutional subscriptions

Notes

  1. 1.

    \(h = 6.626~070~040(81) \times 10^{-34}\,\mathrm{Js}\).

  2. 2.

    The symbol c stands for celerity, an outmoded synonymous of velocity.

  3. 3.

    \(h = 938.272 046(21)\,\mathrm{MeV}/c^2\).

References

  1. Tanabashi M et al (2018) Review of particle physics. Phys Rev D 98(3):030001

    Google Scholar 

  2. The decay of a lambda particle in the 32 cm hydrogen bubble chamber (1960). https://cds.cern.ch/record/39474

  3. Perrin J (1930) Les atomes. Librairie Félix Alcan, Paris

    Google Scholar 

  4. Rutherford E (1914) LVII The structure of the atom. Philos Mag 27(159):488–498. https://doi.org/10.1080/14786440308635117. http://dx.doi.org/10.1080/14786440308635117. http://dx.doi.org/10.1080/14786440308635117

  5. Kurzon (2017) Geiger–Marsden experiment expectation and result. Accessed: 2017-09-10. https://upload.wikimedia.org/wikipedia/commons/f/f9/Geiger-Marsden_experiment_expectation_and_result.svg

  6. DESY A picture of the proton. http://www.desy.de

  7. Abramowicz H et al (2015) Combination of measurements of inclusivedeep inelastic \(e\pm p\) scattering cross sections and QCD analysis of HERA data. Eur. Phys. J. C75(12):580. https://doi.org/10.1140/epjc/s10052-015-3710-4. arXiv:1506.06042 [hep-ex]

  8. Barone V, Predazzi E (2002) High-energy particle diffraction, vol. 565. Texts and monographs in physics. Springer, Berlin. isbn: 3540421076. http://www-spires.fnal.gov/spires/find/books/www?cl=QC794.6.C6B37::2002

  9. Kapteyn JC (1922) First attempt at a theory of the arrangement and motion of the sidereal system. Astrophys J 55:302–328. https://doi.org/10.1086/142670

    Article  ADS  Google Scholar 

  10. Zwicky F (1933) Die Rotverschiebung von extragalaktischen Nebeln. Helv Phys Acta 6:110–127 [Gen Relativ Gravit 41(207) (2009)]. https://doi.org/10.1007/s10714-008-0707-4

  11. Rubin VC, Ford Jr WK (1970) Rotation of the Andromeda nebula from a spectroscopic survey of emission regions. Astrophys J 159:379–403. https://doi.org/10.1086/150317

  12. Natarajan P et al (2017) Mapping substructure in the HST frontier fields cluster lenses and in cosmological simulations. In: Mon Not R Astron Soc 468(2):1962–1980. https://doi.org/10.1093/mnras/stw3385. arXiv:1702.04348 [astro-ph.GA]

  13. Ade PAR et al (2016) Planck 2015 results. XIII. Cosmological parameters. In: Astron. Astrophys. 594:A13. https://doi.org/10.1051/0004-6361/201525830. arXiv:1502.01589 [astro-ph.CO]

  14. Hu W (2017) Intermediate guide to the acoustic peaks and polarization. http://background.uchicago.edu/~whu/intermediate/intermediate.html. Accessed: 2017-10-21

  15. Huterer D, Turner MS (1999) Prospects for probing the dark energy via supernova distance measurements. Phys Rev D60:081301. https://doi.org/10.1103/PhysRevD.60.081301. arXiv:astro-ph/9808133 [astro-ph]

  16. Frieman J, Turner M, Huterer D (2008) Dark energy and the accelerating universe. Ann Rev Astron Astrophys 46:385–432. https://doi.org/10.1146/annurev.astro.46.060407.145243. arXiv:0803.0982 [astro-ph]

Download references

Author information

Authors and Affiliations

Authors

Corresponding author

Correspondence to Patrick L. S. Connor .

1.A Dark Matter and Dark Energy

1.A Dark Matter and Dark Energy

As we already stressed, gravitation is too weak to compete with other interactions, and is therefore not described in HEP. But the existence of dark matter and dark energy is a strong motivation for BSM.

1.1 1.A.1 Dark Matter

Several observations suggest more matter to be in the universe than the radiated light may let it believe, i.e. some type of matter that does not interact electromagnetically and that cannot be found on earth; this unknown matter is called dark matter.

Historically, the main technique to detect dark matter has been to compute the difference between the luminous mass and the dynamical mass. This can be done at different scales:

  • star clusters [9],

  • galaxy clusters [10]

  • and galaxy dynamics [11].

More recently, gravitational lenses even allowed to map dark matter in the universe [12]; in addition, anisotropies in the Cosmic Microwave Background may be partly explained by the presence of dark matter [13, 14]. This list is not exhaustive, but these observations are pointing to an important missing piece of modern HEP.

1.2 1.A.2 Dark Energy

The cosmological constant is necessary to explain the observed expansion of the universe with the theory of general relativity [15]. Since it can be understood as a contribution to the energy, it is called dark energy. It would account for around two thirds of the content of the universe [16]; on the other hand, unlike baryonic and dark matter, it would fill the entire universe quite uniformly. Its nature is totally unknown; and its density is too low to be detected in experiments as of today.

Rights and permissions

Reprints and permissions

Copyright information

© 2019 Springer Nature Switzerland AG

About this chapter

Check for updates. Verify currency and authenticity via CrossMark

Cite this chapter

Connor, P.L.S. (2019). Introduction to High Energy Physics. In: Inclusive b Jet Production in Proton-Proton Collisions. Springer Theses. Springer, Cham. https://doi.org/10.1007/978-3-030-34383-5_1

Download citation

Publish with us

Policies and ethics