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.
After a short description of the historical discovery of pulsars, the different possible interpretations for pulsars are discussed. The different observational classes of pulsars are summarized. The dipole model for pulsars is introduced to motivate the definition of the characteristic age and the magnetic field of pulsars. The notion of the braking index of pulsars is confronted with the dipole model and the emission of gravitational waves from pulsars. The pulsar diagram is discussed in terms of the evolution of pulsars and the recycling mechanism for binary pulsars. The model of the aligned rotator introduces the magnetosphere of pulsars and a more sophisticated approach for the pulsar emission mechanism. The details of extracting the neutron star masses from pulsar timing is outlined. Observational data from the Hulse–Taylor pulsar and the double pulsar are confronted with predictions from general relativity in strong fields.
Recommend this
Email your librarian or administrator to recommend adding this to your organisation's collection.