We use cookies to distinguish you from other users and to provide you with a better experience on our websites. Close this message to accept cookies or find out how to manage your cookie settings.
To save content items to your account,
please confirm that you agree to abide by our usage policies.
If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account.
Find out more about saving content to .
To save content items to your Kindle, first ensure [email protected]
is added to your Approved Personal Document E-mail List under your Personal Document Settings
on the Manage Your Content and Devices page of your Amazon account. Then enter the ‘name’ part
of your Kindle email address below.
Find out more about saving to your Kindle.
Note you can select to save to either the @free.kindle.com or @kindle.com variations.
‘@free.kindle.com’ emails are free but can only be saved to your device when it is connected to wi-fi.
‘@kindle.com’ emails can be delivered even when you are not connected to wi-fi, but note that service fees apply.
Rudimentary catalogues of cosmic voids were first complied in the mid-1980s, but they were limited in scope by the lack of adequate deep galaxy survey data. Over several decades, catalogues have improved as have cosmic void identification methods. Voids in the galaxy distribution have become important objects and modern tools that are now used to investigate properties of the Universe. They have been and continue to be applied to problems in precision cosmology. The first step in utilizing this new tool is to compile massive surveys of the distant Universe that yield sufficiently large samples of cosmic voids. Then reliable void identification techniques were developed. These include sophisticated methods of 3D analysis. For some tests, “stacked voids” are created to enhance the measurement precision. Specific research results are summarized showing concrete results. Three other topics are discussed: topology of the void and supercluster structure, the LTB Universe models, and finally void galaxies.
Recommend this
Email your librarian or administrator to recommend adding this to your organisation's collection.