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In supersymmetric axion models, if the gravitino or axino is the lightest SUSY particle (LSP), the other is often the next-to-LSP (NLSP).
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E. J. Chun, J. E. Kim, and H. P. Nilles, Axino mass
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1995
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R. Bradley, J. Clarke, D. Kinion, L. J. Rosenberg, K. van Bibber, S. Matsuki, M. Muck, and P. Sikivie, Microwave cavity searches for dark-matter axions
2003
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2004
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M. Kawasaki, K. Kohri, and T. Moroi, Big-Bang nucleosynthesis and hadronic decay of long-lived massive particles
2005
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K. Ichikawa, M. Kawasaki, K. Nakayama, M. Senami, and F. Takahashi, Increasing effective number of neutrinos by decaying particles
2007
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J. Pradler and F. D. Steffen, Thermal Gravitino Production and Collider Tests of Leptogenesis
2007
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V. S. Rychkov and A. Strumia, Thermal production of gravitinos
2007
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M. Bolz, A. Brandenburg, and W. Buchmuller, Thermal Production of Gravitinos
2008
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M. Kawasaki, K. Nakayama, and M. Senami, Cosmological implications of supersymmetric axion models
2013
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2013
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2014
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2015
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2008
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M. Kawasaki, K. Kohri, T. Moroi, and A. Yotsuyanagi, Big-Bang Nucleosynthesis and Gravitino
2008
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A. Strumia, Thermal Production of Axino Dark Matter
2010
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M. Kawasaki, N. Kitajima, and K. Nakayama, Inflation from a Supersymmetric Axion Model
2010
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2010
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E. J. Chun, Dark matter in the Kim-Nilles mechanism
2011
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2011
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2015
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2015
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2015
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2016
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2016
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2016
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2016
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2016
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2016
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2016
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2016
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E. Di Valentino and F. R. Bouchet, A comment on power-law inflation with a dark radiation component
2016
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2016
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2016
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2016
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P. Ko and Y. Tang, Residual Non-Abelian Dark Matter and Dark Radiation
2017
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