Welcome to ler's documentation! =============================== .. image:: ../lerlogo.png :align: center :width: 30% :alt: ler logo ================== ler ================== ``ler`` (/ˈɛlɚ/): :red_first:`LVK` (LIGO-Virgo-KAGRA collaboration) :red_first:`Event` (compact-binary mergers) :red_first:`Rate` calculator and simulator. ``ler`` is a statistical based python package whose core function is to calculate detectable rates of gravitational waves events (both lensed and un-lensed events). Description available in the `Summary `_ section. | The code is available at `github.ler `_. | For reaching out to the developer, please raise issue in `github.ler.issue `_. ``ler`` is closely integarted with a gravitational waves SNR calculator package `gwsnr `_. | ``ler`` main developer: `Hemanta Ph. `_ | ``ler`` developer and analyst: Anupreeta More, Harsh Narola, Ng Chung Yin (Leo), Justin Janquart, Chris Van Den Broeck, Otto Akseli Hannuksela, Neha Singh, David Keitel .. Yiwei Li (Lisa). Glossary ================== .. glossary:: Gravitational waves .. image:: _static/gw.gif :align: left :width: 480px :alt: ler logo *Animation showing the propagation of gravitational waves from inspiraling binary black holes.* `Source `_ : Jeffrey Bryant, Wolfram|Alpha, LLC. | Ripples in the fabric of space-time caused by some of the most violent and energetic processes in the Universe, such as merger of compact binaries (e.g., black holes and neutron stars) and supernovae explosions. Albert Einstein predicted the existence of gravitational waves in 1916 in his general theory of relativity, but it took a century to detect them directly. The first detection was made in 2015 by the LIGO and Virgo collaborations, which won the 2017 Nobel Prize in Physics. Gravitational waves are invisible, yet incredibly fast; they travel at the speed of light, squeezing and stretching anything in their path. | Lensing of gravitational waves .. raw:: html
*Interactive animation showing the lensing of gravitational waves by a massive object.* | A process similar to the gravitational lensing of light, where gravitational waves emitted from distant astrophysical events are bent and splitted (strong-lensing case) into multiple images by the gravity of intervening massive objects, such as galaxy and galaxy cluster. This can magnify and change the arrival time of the gravitational waves. | .. image:: _static/Light_Bending.gif :align: right :width: 480px :alt: ler logo *Animation showing the bending of light by a massive object.* `Source `_ : NASA, ESA, and Goddard Space Flight Center/K. Jackson. | | | | | | Rate calculation and statistics .. image:: _static/BBH_Merger_rate_density_and_PDF_of_redshift.png :align: left :width: 480px :alt: ler logo *Figure showing the merger rate density of binary black hole (BBH) mergers as a function of redshift.* `Source `_ : generated by the LeR package. | In the context of astrophysics and gravitational wave science, rate calculation involves predicting the frequency of events such as compact-binary mergers based on observed data and theoretical models. Statistical methods are used to analyze and interpret the data, estimate parameters, and test hypotheses. .. toctree:: :maxdepth: 2 :caption: Contents: Installation2 Summary code_overview GW_events GW_equations Lensed_events Lensed_equations .. toctree:: :maxdepth: 1 :caption: API: autoapi/ler/rates/index.rst autoapi/ler/gw_source_population/index.rst autoapi/ler/lens_galaxy_population/index.rst autoapi/ler/image_properties/index.rst autoapi/ler/utils/index.rst .. toctree:: :maxdepth: 2 :caption: Examples: examples/rates/LeR complete examples examples/rates/GWRATES complete exmaples examples/rates/grb detection rate examples/rates/ler bns example examples/rates/rates_with_3G_detectors examples/source population/merger rate density evolution with redshift examples/source population/merger rate density model comparision examples/source population/sample compact binary parameters examples/source population/sample compact binary parameters with redshift examples/source population/statistical study of changing mass model params examples/source population/statistical study of cosmological friction examples/lens_parameters/sample lens parameters examples/optical_depth/validation_SIE examples/optical_depth/validation_SIS examples/image_properties/dt_vs_dmu Indices and tables ================== * :ref:`genindex` * :ref:`modindex` * :ref:`search`