• EVALUATION OF THE ACCURACY AND REPRODUCIBILITY OF THE PLANNING ISOCENTRE USING AUTOMATIC AND MANUAL COUCH MOVEMENTS 

  MOGIRE, NAOMI (2023-11-01)

  The present study delves into the subject of analyzing the accuracy and reproducibility of the planned isocenter using automatic and manual couch movements, a pivotal issue within the broader context of radiotherapy. This ...
• EFFECT OF DEFECTS AND TEMPERATURE ON THE MECHANICAL AND ELECTRONIC PROPERTIES OF NbC AND NbN: A FIRST-PRINCIPLES STUDY 

  MUCHIRI, PERPETUA (2023-11-01)

  Transition metal carbides and nitrides (TMCNs) are materials that have attracted a lot of attention for both theoretical and experimental studies. This is largely attributed to their excellent physical and electronic ...
• CHARACTERISATION OF CORNISH-SOUTH ULTRA-COMPACT HII-REGIONS SAMPLE USING THE MeerKAT 

  JUMA, CALVINCE (2023-11-01)

  Ultra-compact HII (UC HII) regions are small and dense ionized regions surrounding massive protostars. They are formed when ultra-violet (UV) radiation from massive protostars ionizes the surrounding neutral hydrogen gas. ...
• PESTICIDES: OCCUPATIONAL EXPOSURE AND POTENTIAL IMPACTS ON ECOSYSTEM AND HUMAN HEALTH IN MERU COUNTY, KENYA 

  MARETE, GABRIEL MUTHEE (Technical University of Kenya, 2021-03)

  ABSTRACT This study assessed the usage of pesticides and its impacts on ecosystems and human health through occupational exposure in selected farming communities in Imenti North, Imenti South and Buuri Sub-counties in ...
• HEAD TO HEAD AND TAIL TO TAIL 180◦ DOMAIN WALLS IN PbTiO3/PbTiO3 FERROELECTRIC THIN FILMS: AN AB INITIO STUDY 

  SIFUNA, JAMES SIMIYU (2024-02-23)

  Charged domain walls (DWs) in ferroelectric materials have gained a lot of interest for a decade now. Large conductivity has been reported at the DWs of insulating ferroelectric materials, and it has lots of applications ...
• A MULTI-WAVELENGTH STUDY OF MASSIVE STAR FORMING REGION G188.95+0.89 IN PROBING THE DYNAMICS OF MASSIVE STAR FORMATION 

  MARTIN MULE MUTIE, MARTIN MULE (Technical University of Kenya, 2023-11)

  ABSTRACT Massive stars are born in regions that are opaque to optical observations. This is a challenge in understanding the processes that involve their formation. In order to investigate their formations, a multi-wavelength ...

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