91探花

Skip to main content
Department Of Physics text logo
  • Research
    • Our research
    • Our research groups
    • Our research in action
    • Research funding 91探花
    • Summer internships for undergraduates
  • Study
    • Undergraduates
    • Postgraduates
  • Engage
    • For alumni
    • For business
    • For schools
    • For the public
  • Support
91探花
Theoretical physicists working at a blackboard collaboration pod in the Beecroft building.
Credit: Jack Hobhouse

Professor Joseph Conlon

Professor of Theoretical Physics

Research theme

  • Particle astrophysics & cosmology
  • Fundamental particles and interactions
  • Fields, strings, and quantum dynamics

Sub department

  • Rudolf Peierls Centre for Theoretical Physics

Research groups

  • Particle theory
Joseph.Conlon@physics.ox.ac.uk
Telephone: 01865 (2)73608
Rudolf Peierls Centre for Theoretical Physics, room 60.10
  • About
  • Publications

Searching for a 0.1-1 keV Cosmic Axion Background

ArXiv 1305.3603 (2013)

Authors:

Joseph P Conlon, MC David Marsh

Abstract:

Primordial decays of string theory moduli at z \sim 10^{12} naturally generate a dark radiation Cosmic Axion Background (CAB) with 0.1 - 1 keV energies. This CAB can be detected through axion-photon conversion in astrophysical magnetic fields to give quasi-thermal excesses in the extreme ultraviolet and soft X-ray bands. Substantial and observable luminosities may be generated even for axion-photon couplings \ll 10^{-11} GeV^{-1}. We propose that axion-photon conversion may explain the observed excess emission of soft X-rays from galaxy clusters, and may also contribute to the diffuse unresolved cosmic X-ray background. We list a number of correlated predictions of the scenario.

Searching for a 0.1-1 keV Cosmic Axion Background

(2013)

Authors:

Joseph P Conlon, MC David Marsh

The Cosmophenomenology of Axionic Dark Radiation

ArXiv 1304.1804 (2013)

Authors:

Joseph P Conlon, MC David Marsh

Abstract:

Relativistic axions are good candidates for the dark radiation for which there are mounting observational hints. The primordial decays of heavy fields produce axions which are ultra-energetic compared to thermalised matter and inelastic axion-matter scattering can occur with $E_{CoM} \gg T_{\gamma}$, thus accessing many interesting processes which are otherwise kinematically forbidden in standard cosmology. Axion-photon scattering into quarks and leptons during BBN affects the light element abundances, and bounds on overproduction of $^4$He constrain a combination of the axion decay constant and the reheating temperature. For supersymmetric models, axion scattering into visible sector superpartners can give direct non-thermal production of dark matter at $T_{\gamma} \ll T_{freezeout}$. Most axions --- or any other dark radiation candidate from modulus decay --- still linger today as a Cosmic Axion Background with $E_{axion} \sim \mathcal{O}(100) eV$, and a flux of $\sim 10^6 cm^{-2} s^{-1}$.

The Cosmophenomenology of Axionic Dark Radiation

(2013)

Authors:

Joseph P Conlon, MC David Marsh

Cosmological natural selection and the purpose of the universe

Complexity 18:5 (2013) 48-56

Authors:

A Gardner, JP Conlon

Abstract:

The cosmological natural selection (CNS) hypothesis holds that the fundamental constants of nature have been fine-tuned by an evolutionary process in which universes produce daughter universes via the formation of black holes. Here, we formulate the CNS hypothesis using standard mathematical tools of evolutionary biology. Specifically, we capture the dynamics of CNS using Price's equation, and we capture the adaptive purpose of the universe using an optimization program. We establish mathematical correspondences between the dynamics and optimization formalisms, confirming that CNS acts according to a formal design objective, with successive generations of universes appearing designed to produce black holes. 漏 2013 Wiley Periodicals, Inc.

Pagination

  • First page First
  • Previous page Prev
  • …
  • Page 14
  • Page 15
  • Page 16
  • Page 17
  • Current page 18
  • Page 19
  • Page 20
  • Page 21
  • Page 22
  • …
  • Next page Next
  • Last page Last

Footer 91探花

  • Contact us
  • Giving to the Dept of Physics
  • Work with us
  • Media

User account menu

  • Log in

Follow us

FIND US

Clarendon Laboratory,

Parks Road,

91探花,

OX1 3PU

CONTACT US

Tel: +44(0)1865272200

Department Of Physics text logo

漏 91探花 - Department of Physics

Cookies | Privacy policy | Accessibility statement

  • Home
  • Research
  • Study
  • Engage
  • Our people
  • News & Comment
  • Events
  • Our facilities & services
  • About us
  • Giving to Physics