Pseudo-Complex General Relativity
Οκτ 2015 · Springer
3,0star
2 κριτικέςreport
ebook
250
Σελίδες
reportΟι αξιολογήσεις και οι κριτικές δεν επαληθεύονται Μάθετε περισσότερα
Σχετικά με το ebook
This book explores the role of singularities in general relativity (GR): The theory predicts that when a sufficient large mass collapses, no known force is able to stop it until all mass is concentrated at a point. The question arises, whether an acceptable physical theory should have a singularity, not even a coordinate singularity. The appearance of a singularity shows the limitations of the theory. In GR this limitation is the strong gravitational force acting near and at a super-massive concentration of a central mass. First, a historical overview is given, on former attempts to extend GR (which includes Einstein himself), all with distinct motivations. It will be shown that the only possible algebraic extension is to introduce pseudo-complex (pc) coordinates, otherwise for weak gravitational fields non-physical ghost solutions appear. Thus, the need to use pc-variables. We will see, that the theory contains a minimal length, with important consequences. After that, the pc-GR is formulated and compared to the former attempts. A new variational principle is introduced, which requires in the Einstein equations an additional contribution. Alternatively, the standard variational principle can be applied, but one has to introduce a constraint with the same former results. The additional contribution will be associated to vacuum fluctuation, whose dependence on the radial distance can be approximately obtained, using semi-classical Quantum Mechanics. The main point is that pc-GR predicts that mass not only curves the space but also changes the vacuum structure of the space itself. In the following chapters, the minimal length will be set to zero, due to its smallness. Nevertheless, the pc-GR will keep a remnant of the pc-description, namely that the appearance of a term, which we may call "dark energy", is inevitable. The first application will be discussed in chapter 3, namely solutions of central mass distributions. For a non-rotating massive object it is the pc-Schwarzschild solution, for a rotating massive object the pc-Kerr solution and for a charged massive object it will be the Reissner-Nordström solution. This chapter serves to become familiar on how to resolve problems in pc-GR and on how to interpret the results. One of the main consequences is, that we can eliminate the event horizon and thus there will be no black holes. The huge massive objects in the center of nearly any galaxy and the so-called galactic black holes are within pc-GR still there, but with the absence of an event horizon! Chapter 4 gives another application of the theory, namely the Robertson-Walker solution, which we use to model different outcomes of the evolution of the universe. Finally the capability of this theory to predict new phenomena is illustrated.
Βαθμολογίες και αξιολογήσεις
3,0
2 αξιολογήσεις
Σχετικά με τον συγγραφέα
Prof. Dr. Peter O. Hess, Mexico
Dr. Mirko Schäfer, Frankfurt, Germany
Prof. Dr. Dr. h. c. mult. Walter Greiner, Frankfurt, Germany
Αξιολογήστε αυτό το ebook
Πείτε μας τη γνώμη σας.
Πληροφορίες ανάγνωσης
Smartphone και tablet
Εγκαταστήστε την εφαρμογή Βιβλία Google Play για Android και iPad/iPhone. Συγχρονίζεται αυτόματα με τον λογαριασμό σας και σας επιτρέπει να διαβάζετε στο διαδίκτυο ή εκτός σύνδεσης, όπου κι αν βρίσκεστε.
Φορητοί και επιτραπέζιοι υπολογιστές
Μπορείτε να ακούσετε ηχητικά βιβλία τα οποία αγοράσατε στο Google Play, χρησιμοποιώντας το πρόγραμμα περιήγησης στον ιστό του υπολογιστή σας.
eReader και άλλες συσκευές
Για να διαβάσετε περιεχόμενο σε συσκευές e-ink, όπως είναι οι συσκευές Kobo eReader, θα χρειαστεί να κατεβάσετε ένα αρχείο και να το μεταφέρετε στη συσκευή σας. Ακολουθήστε τις αναλυτικές οδηγίες του Κέντρου βοήθειας για να μεταφέρετε αρχεία σε υποστηριζόμενα eReader.
