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

Moduli Stabilisation and the Holographic Swampland

(2020)

Authors:

Joseph P Conlon, Filippo Revello

Moduli stabilisation and the holographic swampland

Letters in High Energy Physics Andromeda Publishing and Education Services 171:2020 (2020)

Authors:

Jp Conlon, F Revello

Abstract:

We investigate whether Swampland constraints on the low-energy dynamics of weakly coupled, moduli- stabilised string vacua in AdS can be related to inconsistencies of their putative holographic duals or, more generally, recast in terms of CFT data. We find that various swampland consistency constraints are equivalent to a negativity condition on the sign of certain mixed anomalous dimensions. This condition is similar to well-established CFT positivity bounds arising from causality and unitarity, but not known to hold in general. The studied scenarios include LVS, KKLT, and both perturbative and racetrack stabilisation. Interestingly, the LVS vacuum (with 螖蠁=8.038) also appears to live very close to a critical value (螖蠁=8) where the anomalous dimensions change sign. We finally point out an intriguing connection to the Swampland Distance Conjecture, both in its original and refined versions.

A Note on Brane Inflation

Acta Physica Polonica B Proceedings Supplement Jagiellonian University 13:2 (2020) 231

Physics potential of the International Axion Observatory (IAXO)

Journal of Cosmology and Astroparticle Physics IOP Publishing 2019:6 (2019) 47

Authors:

E Armengaud, D Attie, S Basso, P Brun, N Bykovskiy, JM Carmona, JF Castel, S Cebrian, M Cicoli, M Civitani, C Cogollos, Joseph Conlon, D Costa, T Dafni, R Daido, AV Derbin, MA Descalle, K Desch, IS Dratchnev, B Doebrich, A Dudarev, E Ferrer-Ribas, I Fleck, J Galan, G Galanti, L Garrido, D Gascon, L Gastaldo, C Germani, G Ghisellini, M Giannotti, I Giomataris, S Gninenko, N Golubev, R Graciani, IG Irastorza, K Jakovcic, J Kaminski, M Krcmar, C Krieger, B Lakic, T Lasserre, P Laurent, O Limousin, A Lindner, I Lomskaya, B Lubsandorzhiev, G Luzon, MCD Marsh, C Mergalejo

Abstract:

We review the physics potential of a next generation search for solar axions: the International Axion Observatory (IAXO). Endowed with a sensitivity to discover axion-like particles (ALPs) with a coupling to photons as small as ga纬 鈭 10鈭12 GeV鈭1 , or to electrons gae 鈭10鈭13, IAXO has the potential to find the QCD axion in the 1 meV鈭1 eV mass range where it solves the strong CP problem, can account for the cold dark matter of the Universe and be responsible for the anomalous cooling observed in a number of stellar systems. At the same time, IAXO will have enough sensitivity to detect lower mass axions invoked to explain: 1) the origin of the anomalous 鈥渢ransparency鈥 of the Universe to gamma-rays, 2) the observed soft X-ray excess from galaxy clusters or 3) some inflationary models. In addition, we review string theory axions with parameters accessible by IAXO and discuss their potential role in cosmology as Dark Matter and Dark Radiation as well as their connections to the above mentioned conundrums.

Physics potential of the International Axion Observatory (IAXO)

(2019)

Authors:

E Armengaud, D Attie, S Basso, P Brun, N Bykovskiy, JM Carmona, JF Castel, S Cebri谩n, M Cicoli, M Civitani, C Cogollos, JP Conlon, D Costa, T Dafni, R Daido, AV Derbin, MA Descalle, K Desch, IS Dratchnev, B D枚brich, A Dudarev, E Ferrer-Ribas, I Fleck, J Gal谩n, G Galanti, L Garrido, D Gascon, L Gastaldo, C Germani, G Ghisellini, M Giannotti, I Giomataris, S Gninenko, N Golubev, R Graciani, IG Irastorza, K Jakovcic, J Kaminski, M Krcmar, C Krieger, B Laki膰, T Lasserre, P Laurent, O Limousin, A Lindner, I Lomskaya, B Lubsandorzhiev, G Luz贸n, MCD Marsh, C Mergalejo, F Mescia, M Meyer, J Miralda-Escud茅, H Mirallas, VN Muratova, XF Navick, C Nones, A Notari, A Nozik, A Ortiz de Sol贸rzano, V Pantuev, T Papaevangelou, G Pareschi, K Perez, E Picatoste, MJ Pivovaroff, J Redondo, A Ringwald, M Roncadelli, E Ruiz-Ch贸liz, J Ruz, K Saikawa, J Salvad贸, MP Samperiz, T Schiffer, S Schmidt, U Schneekloth, M Schott, H Silva, G Tagliaferri, F Takahashi, F Tavecchio, H ten Kate, I Tkachev, S Troitsky, E Unzhakov, P Vedrine, JK Vogel, C Weinsheimer, A Weltman, W Yin

Pagination

  • First page First
  • Previous page Prev
  • …
  • Page 2
  • Page 3
  • Page 4
  • Page 5
  • Current page 6
  • Page 7
  • Page 8
  • Page 9
  • Page 10
  • …
  • 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