From b0f7fd4e368c2d2cf8f098692591a8b7f8218569 Mon Sep 17 00:00:00 2001 From: yurilevincolumbia <136669906+yurilevincolumbia@users.noreply.github.com> Date: Mon, 21 Aug 2023 20:45:40 +1000 Subject: [PATCH] Update NSseismology.html --- NSseismology.html | 35 +++++++++++++++++++++++++++++------ 1 file changed, 29 insertions(+), 6 deletions(-) diff --git a/NSseismology.html b/NSseismology.html index 94063b4..2c93e98 100644 --- a/NSseismology.html +++ b/NSseismology.html @@ -4,14 +4,37 @@ Neutron star seismology -

Thermal nois

-

Astrophysics is a huge field. It studies the smallest and the largest objects in the Universe and everything in between. Like many theoretical - astrophysicists, I work on a number of different, sometimes overlapping topics. This website is an attempt to give an overview of my research and - my scientific trajetory

+

Neutron star seismology

+

Vibrational modes of the Eatch and the Sun are routinely measured and provide a wealth of information about their + internal structure. Observing a vibrational mode of a neutron star woud provide a wealth of information about their internal structure, and + this is one of the holy grails of neutron star astrophysics. I have worked on the theory of two types of vibrational modes: the r-modes of + rapidly rotating neutron stars, and torsional magneto-elastic modes of magnetars.

+ Runaway Heating + by R-Modes of Neutron Stars in Low-Mass X-Ray Binaries

- List of - my papers not published as part of the LIGO Scientific Collaboration

+

+ Crust-core + coupling and r-mode damping in neutron stars: a toy model

+ +

+ QPOs during + magnetar flares are not driven by mechanical normal modes of the crust

+ +

+ On the theory of magnetar QPOs

+ +

+ Magnetar oscillations - I. + Strongly coupled dynamics of the crust and the core

+ +

+ + Magnetar oscillations - II. Spectral method

+ +

+ + On the excitation of f modes and torsional modes by magnetar giant flares