Now showing items 1-4 of 4

    • Implementing mechanisms to improve the performance of LTE-WLAN Aggregation 

      Coscollola Coletes, Magí (Universitat Politècnica de Catalunya, 2017-09)
      Master thesis
      Open Access
      Covenantee:   University of Surrey
      As the release of 5G gets closer, different technologies appear aiming to make a difference in this next generation of mobile communications. A proposed way to achieve more capacity for end-users in 5G is aggregating Long ...
    • Prototyping FBMC/OQAM for 5G mobile communications proof of concept 

      Arteaga Martinez, Xavier (Universitat Politècnica de Catalunya, 2015-05-15)
      Master thesis
      Open Access
      Covenantee:   University of Surrey
      [ANGLÈS] Nowadays, the number of wireless devices connected to the internet is rowing quite fast. However, the available spectrum will remain the same. Consequently, the next generation of mobile communications (5G) is ...
    • Search for nova presolar grains: gamma-ray Spectroscopy of Ar-34 and its relevance for the astrophysical Cl-33(p,gamma) reaction 

      José Pont, Jordi (American Institute of Physics (AIP), 2020-06-26)
      Article
      Open Access
      Covenantee:   University of Surrey / Argonne National Laboratory / Simon Fraser University
      The discovery of presolar grains in primitive meteorites has initiated a new era of research in the study of stellar nucleosynthesis. However, the accurate classification of presolar grains as being of specific stellar ...
    • Spectroscopy of P 30 and the abundance of Si 29 in presolar grains 

      Lotay, G.; Doherty, D.T.; Seweryniak, D.; Janssens, R.V.F.; José Pont, Jordi; Woods, Phil J. (American Physical Society, 2020-09-22)
      Article
      Open Access
      Covenantee:   University of Surrey / Argonne National Laboratory / University of North Carolina at Chapel Hill / Duke University / Institut d'Estudis Espacials de Catalunya / University of Massachusetts Lowell / University of Edinburgh
      The astrophysical 29Si(p,¿) reaction is expected to play a key role in determining the final 29Si yields ejected in nova explosions. Such yields are used to accurately identify the stellar origins of meteoritic stardust ...