cosmology notes pdf

10 0 obj << /Length 11 0 R >> stream The content is otherwise orthodox. Cosmology is an interesting course to teach, as it is not like most ofthe other subjects taught in undergraduate physics courses. Based on the recommendations of Spring 2000’s students, I replaced one of the supplemental texts (Mook and Vargish) with this compilation of notes in Spring 2001. h�bbd``b`��� �H�T�Ě���`z�P\Q@��&���i������ ��ٹ@a�.� �=� 08P�V��J�S� �qz�� �c+9�ô�f �;�`i��F7sL4��.�i�"m��m�. ��ڸ�����r�Q;��>���T�d���II^�k�ż^�O8Y���'�,�'^��\#,�Z�Xָ�þ�ߺ9�%Ҷ'Y�z.cEu?�a�$� )uͤ�������|�����$m����x�q���=-�� ���KACZ�B���–Tt:�,\���N��yz~��Х�JFc^)ZK����\�N��t��|�\����n�wN I�; 1 1 1 rg 36 36 720 540 re f BT 61.5 531.75 TD 0 0 0 rg /F1 24 Tf -0.0087 Tc 0 Tw (Cosmology) Tj ET q 246 0 0 -200.25 66 504 cm /im1 Do endstream endobj 19 0 obj 143 endobj 16 0 obj << /Type /XObject /Subtype /Image /Name /im1 /Filter /DCTDecode /Width 328 /Height 267 /BitsPerComponent 8 /ColorSpace /DeviceRGB /Length 17 0 R >> stream Adam Black and Nancy Gee, at Addison Wesley, made possible the great leap from rough lecture notes to polished book.

1 1 1 rg 36 36 720 540 re f BT 199.5 497.25 TD 0 0 0 rg /F0 44.25 Tf -0.1365 Tc 0.324 Tw (Big Bang Cosmology) Tj -138 -49.5 TD /F1 24 Tf 0.0863 Tc -0.2738 Tw (Big Bang vs. The outline of the course is as follows, 1.Review of Standard Model(SM) and … >> %PDF-1.5 %���� In GR cosmology, 3-D space itself expands. Tj 0 -60.75 TD -0.0378 Tc -0.0455 Tw (It turns out that the cosmological principle is completely ) Tj 0 -29.25 TD -0.0675 Tc 0.0675 Tw (consistent with the Hubble expansion.) xڕR�NA��W�q�����Ǜ�ń�a�1��@H ���Yf1���SW:U�U=�a.��:;�"�Z�g�ɢ��h��z
There is no perceived wisdom, built up over a century or more, which provides an unquestionable foundation, as in thermodynamics. Example: Family and Consumer Sciences (program area) courses are now located in five career clusters: • Arts, AV … These notes are intended as an introductory course for experimental particle ... Cosmology (from the Greek: kosmos, universe, world, order, and logos, word, theory) is probably the most ancient body of knowledge, dating from as far back as the predictions of seasons by early civiliza- took my undergraduate cosmology course at Ohio State University. Their feedback (including nonverbal feedback such as frowns and snores during lectures) greatly improved the lecture notes on which this book is based. By the end of the semester, a more or less complete (albeit sketchy) set of notes had been compiled. %%EOF h�b```�\VoA�� �dA#fA&q�8�A[G�����?���,�ɜi�]�3���� ��33x��~�j�)1Ob����Ь�����°D,@*��١,�5=--�"-,5-44d�vX�j�PX��kz#��5]��A0Y�� 3. endobj "(($#$% '+++,.3332-3333333333�� H �� � Lecture 14: More about the cosmological constant (ppt) (pdf) Other observational evidence: statistics of gravitational lensing, X-ray observations of galaxy clusters. 3. Cosmology 2012: Lecture Notes Andrew H. Ja e, Imperial College. %PDF-1.2 872 0 obj <>/Filter/FlateDecode/ID[<7187666F7E14BF40AABD83253B9EB920>]/Index[859 25]/Info 858 0 R/Length 76/Prev 523791/Root 860 0 R/Size 884/Type/XRef/W[1 2 1]>>stream {٫e1�I�"��'��,�����4g��4��t���Z�s^��^��.���_���ӾrO�����E�s!u��J�rC�bb���;��D#D���s��3�l]`=��}�G������ۤl~%�q\(F��jc�r ����/�Cu��åX��z��#v����.NT]��ʹ�6��s #BP������y�.���(bXOYXmv�}��0R%��r��h0�Ɨ) X�Nj7���K�_��y���%�t�O�n;+igc���a��U��B��8:�gRQ�����Z��(��靪W��x[��&';��j�o�1���0�P㢁k}�PMC/`;�&���,'�:���!��V�d>f���ֽ��XgR;�H����R_C�*���.��1�|LOr63���TC68?�,��49)D&�� ���P>3N>O$���ZM)t0�N If you have any corrections please let me know at ajd268@cornell.edu. If you have any corrections please let me know at ajd268@cornell.edu.

endstream Chapter 2 Introduction Cosmology has recently become a very popular research topic. Tj ET endstream endobj 14 0 obj 1035 endobj 12 0 obj << /CropBox [ 36 36 756 576 ] /Type /Page /Parent 5 0 R /Resources << /Font << /F0 6 0 R /F1 8 0 R >> /ProcSet 2 0 R >> /Contents 13 0 R >> endobj 18 0 obj << /Length 19 0 R >> stream The outline of the course is as follows, 1.Review of Standard Model(SM) and … I have tried to avoid the other extreme, practised by some of my particle physics colleagues, of writing books on cosmology with the obvious intent of making particle physicists out of every theoretical astronomer. �;@�B I�^in �E�2?�o7�� ��?�m��(iա ��d�{�4��&H=� ���)�D� ��� 0 �F' 5 0 obj <> x����[���yۙ��ݸ��{�H)�*�����(�G5"��K�#��{��t�Hv�R2h��������q0��'�^o��_������З���z���b��������h�/7w���B�1�N{�?&�{��99輦�S4��2�j?1eR;� of��.�#�`�R�@5���~0.8�{�?������G\*�J;o�Ϗ��?/� stream endstream endobj 860 0 obj <>/Metadata 107 0 R/PageLayout/OneColumn/Pages 851 0 R/StructTreeRoot 127 0 R/Type/Catalog>> endobj 861 0 obj <>/ExtGState<>/Font<>/XObject<>>>/Rotate 0/StructParents 0/Type/Page>> endobj 862 0 obj <>stream >> Ҧꯪ��{m�Ƈ1� ��"Ar �^���f֯5ilQ�K�-a �hhmش�*����页ϝ������0������bzNU�B1��p*��L��N��PY����t���?�X�j�+�U?R���ĩS�������2n��>J�\m&��[�I��|��@��wA�=7��Ԫ�O���?i��AIY%����U�VF� %PDF-1.2 %���� 883 0 obj <>stream /Length 380 =O�]��qfO���{�eR��=`�Im�Wj��`�N��� 9�s����o��7�u(;k�u�߉ǩ�UѽoT���b�?��n��+W�%_9Q�+ �t{���l��?�O��~�C�i��+QP^�Y����4��ʶ�r�iəܢ stream Therefore, expansion of space itself is the real explanation for cosmological redshifts z, not the Doppler effect. the main ideas in cosmology without too much hand-waving. �� @�2�HĀ"�,[GCCH�"�U&Xa ��+CWF��o��F��o��F��o��F��o��F��o��K�S����9�����/�0�Tا,J�6�3}��xz�x�S�}��}ӱ1U�y������i6�K���� 1 1 1 rg 36 36 720 540 re f BT 61.5 537.75 TD 0 0 0 rg /F1 24 Tf -0.0087 Tc 0 Tw (Cosmology) Tj 6 -54 TD /F0 24 Tf -0.048 Tc 0.048 Tw (Cosmological Principle) Tj ET 67.5 480 225 1.5 re f BT 292.5 483.75 TD -0.075 Tc 0.1687 Tw (: At any instant in time, universe is ) Tj -225 -29.25 TD -0.0284 Tc 0.0284 Tw (homogeneous \(same at all locations\) and isotropic \(same in all ) Tj 0 -28.5 TD -0.0711 Tc 0.2378 Tw (directions\), i.e., the universe looks the same to all observers.) notes will likely be expanded until I lose interest in neutrinos. endstream endobj 864 0 obj <>stream

Chapter 2 Introduction Cosmology has recently become a very popular research topic. ���]� Je1UNRry�R�^��C��(��f�i������#�ߏDo�+��k��̤���,�,M^�Q�lv�A�\��1��KR"�4J3�� ���Lq���\��7�pWdR| 5�BY߇��. Bantu Cosmology & the Origins of Egyptian Civilization Notes by Asar Imhotep . All lengths, e.g., distance between galaxies, wavelength of light, etc. expand with the universe. An introduction to cosmology M.H.G. �x�PX5"��AZ���J� Tytgat∗ Service de Physique The´orique CP225 Universite´ Libre de Bruxelles, 1050 Brussels, Belgium Abstract These lecture notes give an introduction to cosmology for high-energy physi-cists. a !1AQa"q�2���B#$Rb34�r�C%�S��cs5��&D�TdE£t6�U�e���u��F'���������������Vfv��������7GWgw��������(8HXhx�������� )9IYiy��������

On occasion I refer back to that book (cited here as “G&C”) for material that does not seem worth repeating here. There is no perceived wisdom, built up over a century or more, which provides an unquestionable foundation, as in thermodynamics.

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endstream endobj startxref I introduce the cosmological princi- �L.s�2��ʐ2�5�#���K��P���j:�60,yw3],�i�ljx�nt9�d8�(�mAlgu2,KʻDk��W�:�rȜGcP��T��DI�,�. *:JZjz���������� �� ? Example: Family and Consumer Sciences (program area) courses are now located in five career clusters: • Arts, AV … students found the notes quite valuable. �������+�U|�������&�oP�=W��>N��_P����דV7�a���w'U_/�`azkɫ�0�Uỏ���vg��c+fEO{��Zׂ]�àO��t�����V̊�������a�@��:�ٟ�e���=�/ k^ v��?�t>��������+�RI$�s];H;L�S5�t� �0c�L�5Ӵ�����:t�����+�RI$�I$�_����+�RI$�I$�_����+�RI$�I$�_����+�RI$�I$�_����+�RI$�I$�_����+�RI$�I$�_����+�RI$�I$�_����+�W���t�߬�#��.�oXh�����m��� k��\tt��24�E��q� ]=7�'H�}���1�1�1�kkn�Z� ��4�q\�OM���:�B����l�l�f��۰����GH#M4A���x��J��OSɮӒ̜v(sl�������g�j�����q���B���]�%�8� P��c�@3-�+۴ ����U���+��=O&�NK2q�@,�Ͳdž�f[�W�h A����hȣ��p����$� 4�`ёF3k��{�w��I�8 h>���"�f�}����sX � 4p �|���s����#�v?�� H���Ӗ�:��. Ҧꯪ��{m�Ƈ1� ��"Ar No!) GW%�m��K�Ua�e�uD� 6���� �#C��G�G9��Y��� ]�x �&{�I�#�����Q���w�}���������j��>ɚ�^�y��B�3��udP7^S�uԅӂ�#�v6'��Q�I�r��� ��T9�]E�:��U�[�/j8��6:�B�n����I��D����Ǔ�|~����n(8�n�7�ܹ���.�G�_��L��Pc�x(Q��Pb�%� O?-A^�nl����ջ�SL�V�!h��|.I�x \8�P�$;�j?�&�0|��@���DW'�ǯ u�҉[Н�a���'=^g����` �~� Historical Side Notes: In the past, Career and Technical Education (CTE) was organized by program areas, but is now organized by career clusters. 32 0 obj << Steady State) Tj 0 -36 TD /F0 24 Tf -0.0546 Tc 0.0546 Tw (Perfect cosmological principle) Tj ET 61.5 408 291.75 1.5 re f BT 353.25 411.75 TD -0.0786 Tc 0.4536 Tw (: universe is unchanging in space ) Tj -291.75 -29.25 TD 0.0348 Tc -0.0348 Tw (and time => Steady) Tj 186.75 0 TD 0.258 Tc 0 Tw (-) Tj 7.5 0 TD -0.024 Tc 0.399 Tw (State universe ) Tj 141.75 0 TD 0.258 Tc 0 Tw (-) Tj 14.25 0 TD -0.036 Tc (Bondi) Tj 58.5 0 TD -0.013 Tc 0.013 Tw (, Hoyle, Gold.) %PDF-1.5

Tj 6 -36 TD -0.15 Tc 0 Tw (\225) Tj 14.25 0 TD -0.1128 Tc 0.6378 Tw (Hubble\222s Law => expansion means no steady state, unless matter ) Tj -14.25 -29.25 TD -0.0024 Tc 0.0024 Tw (continually created to preserve density) Tj 0 -42.75 TD -0.15 Tc 0 Tw (\225) Tj 14.25 0 TD -0.0729 Tc 0.1801 Tw (preference of AGN/quasars for large distances \(early times\)) Tj -14.25 -43.5 TD -0.15 Tc 0 Tw (\225) Tj 14.25 0 TD -0.0871 Tc 0.3371 Tw (cosmic microwave background ) Tj 305.25 0 TD 0.258 Tc 0 Tw (-) Tj 13.5 0 TD -0.0206 Tc 0.0206 Tw (consistent with Big Bang \(BB\)) Tj -333 -42.75 TD -0.15 Tc 0 Tw (\225) Tj 14.25 0 TD -0.0227 Tc 0.106 Tw (predominance of light elements \(e.g., H, He\) consistent with ea) Tj 606 0 TD -0.138 Tc -0.612 Tw (rly ) Tj -620.25 -28.5 TD -0.2258 Tc 0.9758 Tw (hot universe) Tj 0 -43.5 TD -0.15 Tc 0 Tw (\225) Tj 14.25 0 TD -0.1037 Tc 0.1037 Tw (Olbers\222 ) Tj 77.25 0 TD -0.0513 Tc 0.3013 Tw (paradox \(why is night sky dark?\) resolved with BB model) Tj ET endstream endobj 11 0 obj 1754 endobj 4 0 obj << /CropBox [ 36 36 756 576 ] /Type /Page /Parent 5 0 R /Resources << /Font << /F0 6 0 R /F1 8 0 R >> /ProcSet 2 0 R >> /Contents 10 0 R >> endobj 13 0 obj << /Length 14 0 R >> stream notes will likely be expanded until I lose interest in neutrinos. Lecture Notes in Cosmology OliverF.Piattella1 Nucleo´ Cosmo-UFESandPhysicsDepartment, FederalUniversityofEsp´ıritoSanto ... the universe, relativistic cosmology and Friedmann equations (Chapter 2); ther-mal history, Big Bang Nucleosynthesis, recombination and cold relic abundance Tj 0 -44.25 TD -0.1058 Tc 0.1058 Tw (This despite ) Tj 122.25 0 TD -0.026 Tc -0.724 Tw (superclustering ) Tj 152.25 0 TD -0.123 Tc 0.373 Tw (on scales up to ~ 100 ) Tj 209.25 0 TD -0.164 Tc 0 Tw (Mpc) Tj 43.5 0 TD 0.078 Tc -0.078 Tw (; ) Tj -527.25 -29.25 TD -0.0633 Tc 0.3633 Tw (distribution apparently smoother on larger scales.) stream Cosmology. ��+�RI$�I$�_����+�RI$�I$�_����+�RI$�I$�_����+�RI$�I$�_����+�RI$�I$�_����+�RI$�I$�_����+�RI$�I$�_����+�RI$�I$�_����+�RI$�I1 �b�T�Ϋ����+�RI$�IE��X�40L4F�E��X�40L4F�E��X�40L4F����۱��V�Y�O�{m���ǫS,���'⽶�|{�թ�D����DDDI$�I%����+�RI$�I$�_����+�RI$�I$�_����+�RI$�I$�_����+�VS>��W~-�m�'��m�"���}�0 �+)�Z���ܶ���Ih�ё^�˾�q����ϭUߋn[z� Ǥ�[hȯee�D8�{JҦꯪ��{m�Ƈ1� ��"Ar 47 0 obj <<

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