Open main menu
Home
Random
Recent changes
Special pages
Community portal
Preferences
About Wikipedia
Disclaimers
Incubator escapee wiki
Search
User menu
Talk
Dark mode
Contributions
Create account
Log in
Editing
Cosmic inflation
(section)
Warning:
You are not logged in. Your IP address will be publicly visible if you make any edits. If you
log in
or
create an account
, your edits will be attributed to your username, along with other benefits.
Anti-spam check. Do
not
fill this in!
===Magnetic-monopole problem=== {{main| Big Bang#Magnetic monopoles}} Stable magnetic monopoles are a problem for [[Grand Unified Theory|Grand Unified Theories]], which propose that at high temperatures (such as in the early universe), the [[electromagnetic force]], [[strong nuclear force|strong]], and [[weak nuclear force|weak]] [[nuclear force]]s are not actually fundamental forces but arise due to [[spontaneous symmetry breaking]] from a single [[gauge theory]]. These theories predict a number of heavy, stable particles that have not been observed in nature. The most notorious is the magnetic monopole, a kind of stable, heavy "charge" of magnetic field.<ref> {{cite journal |last='t Hooft |first=Gerard |author-link=Gerard 't Hooft |year=1974 |title=Magnetic monopoles in unified gauge theories |journal=[[Nuclear Physics B]] |volume=79 |issue=2 |pages=276β84 |bibcode=1974NuPhB..79..276T |hdl=1874/4686 |doi=10.1016/0550-3213(74)90486-6 |url=http://dspace.library.uu.nl:8080/handle/1874/4686 |archive-url=https://web.archive.org/web/20241204020241/http://dspace.library.uu.nl:8080/handle/1874/4686 |url-status=dead |archive-date=4 December 2024 }} </ref><ref> {{Cite journal |first=Alexander M. |last=Polyakov |year=1974 |title=Particle spectrum in quantum field theory |journal=[[JETP Letters]] |volume=20 |pages=194β195 |bibcode=1974JETPL..20..194P }} </ref> Monopoles are predicted to be copiously produced following Grand Unified Theories at high temperature,<ref> {{Cite journal |first1=Alan |last1=Guth |author-link=Alan Guth |first2=S. |last2=Tye |year=1980 |title= Phase transitions and magnetic monopole production in the very early universe |journal=[[Physical Review Letters]] |volume=44 |issue=10 |pages=631β635; Erratum ''ibid.'' (1980) '''44''' p 963 |doi=10.1103/PhysRevLett.44.631 |bibcode=1980PhRvL..44..631G |osti=1447535 |url=http://repository.ust.hk/ir/bitstream/1783.1-49322/1/PhysRevLett.44.631.pdf |url-status=live |archive-url=https://ghostarchive.org/archive/20221009/http://repository.ust.hk/ir/bitstream/1783.1-49322/1/PhysRevLett.44.631.pdf |archive-date=2022-10-09 }} </ref><ref> {{Cite journal |first1=Martin B. |last1=Einhorn |last2=Stein |first2=D.L. |last3=Toussaint |first3=Doug |year=1980 |title=Are grand unified theories compatible with standard cosmology? |journal=[[Physical Review D]] |volume=21 |issue=12 |pages=3295β3298 |bibcode=1980PhRvD..21.3295E |doi=10.1103/PhysRevD.21.3295 }} </ref> and they should have persisted to the present day, to such an extent that they would become the primary constituent of the Universe.<ref> {{Cite journal |first1=Ya. |last1=Zel'dovich |first2=M. Yu. |last2=Khlopov |year=1978 |title=On the concentration of relic monopoles in the universe |journal=[[Physics Letters B]] |volume=79 |issue=3 |pages=239β41 |bibcode=1978PhLB...79..239Z |doi=10.1016/0370-2693(78)90232-0 }} </ref><ref> {{cite journal |first=John |last=Preskill |year=1979 |title=Cosmological production of superheavy magnetic monopoles |doi=10.1103/PhysRevLett.43.1365 |journal=[[Physical Review Letters]] |volume=43 |issue=19 |pages=1365β1368 |bibcode=1979PhRvL..43.1365P |url=https://authors.library.caltech.edu/6133/1/PREprl79.pdf |url-status=live |archive-url=https://ghostarchive.org/archive/20221009/https://authors.library.caltech.edu/6133/1/PREprl79.pdf |archive-date=2022-10-09 }} </ref> Not only is that not the case, but all searches for them have failed, placing stringent limits on the density of relic magnetic monopoles in the Universe.<ref> {{Cite journal |last1=Yao |first1=W.-M. |display-authors=etal |collaboration=Particle Data Group |year=2006 |title=Review of Particle Physics |journal=[[Journal of Physics G]] |volume=33 |issue=1 |pages=1β1232 |arxiv=astro-ph/0601168 |bibcode=2006JPhG...33....1Y |doi=10.1088/0954-3899/33/1/001 |s2cid=262936640 |url=http://pdg.lbl.gov/ }} </ref> A period of inflation that occurs below the temperature where magnetic monopoles can be produced would offer a possible resolution of this problem: Monopoles would be separated from each other as the Universe around them expands, potentially lowering their observed density by many orders of magnitude. Though, as cosmologist [[Martin Rees]] has written, : "Skeptics about exotic physics might not be hugely impressed by a theoretical argument to explain the absence of particles that are themselves only hypothetical. Preventive medicine can readily seem 100 percent effective against a disease that doesn't exist!"<ref> {{cite book |last=Rees |first=Martin |author-link=Martin Rees |year=1998 |title=Before the Beginning |place=New York, NY |publisher=Basic Books |page=185 |isbn=0-201-15142-1 }} </ref>
Edit summary
(Briefly describe your changes)
By publishing changes, you agree to the
Terms of Use
, and you irrevocably agree to release your contribution under the
CC BY-SA 4.0 License
and the
GFDL
. You agree that a hyperlink or URL is sufficient attribution under the Creative Commons license.
Cancel
Editing help
(opens in new window)