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<CourseUnit xmlns="http://www.manchester.ac.uk/CUICourseUnitDetails" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.manchester.ac.uk/CUICourseUnitDetails.xsd">
  <UnitCode Applicant="Y" Label="Unit code" Student="Y">
    <Code>PHYS40772</Code>
  </UnitCode>
  <UnitTitle Applicant="Y" Label="Unit title" Student="Y">
    <Title>Early Universe (M,A)</Title>
  </UnitTitle>
  <MaxUnits Applicant="Y" Label="Credit rating" Student="Y">
    <Units>10</Units>
  </MaxUnits>
  <TeachingPeriods Applicant="Y" Label="Teaching period(s)" Student="Y">
    <Period>Semester 2</Period>
  </TeachingPeriods>
  <AcademicCareer Applicant="Y" Label="Academic career" Student="Y">
    <Value>Undergraduate</Value>
  </AcademicCareer>
  <UnitLevel Applicant="Y" Label="Unit level" Student="Y">
    <Level>Level 4</Level>
  </UnitLevel>
  <StaffList Applicant="Y" Label="Teaching staff" RoleLabel="Course Unit Role" Student="Y">
    <StaffMember>
      <Name>Jens Chluba</Name>
      <Role>Unit coordinator</Role>
    </StaffMember>
  </StaffList>
  <OfferedBy Applicant="Y" Label="Offered by" Student="Y">
    <OrganisationList>
      <Organisation>
        <OrgName>Department of Physics &amp; Astronomy</OrgName>
      </Organisation>
    </OrganisationList>
    <GroupList>
      <Group>
        <GroupName></GroupName>
      </Group>
    </GroupList>
    <FheqLevels>
      <FheqLevel>
        <LevelNumber>1</LevelNumber>
        <LevelName>FHEQ level (Framework for Higher Education Qualifications) ' Masters/Integrated Masters P4 ' </LevelName>
      </FheqLevel>
    </FheqLevels>
    <Ects>
      <MaxUnits>European Credit Transfer &amp; Accumulation System Rating :   5.0</MaxUnits>
    </Ects>
  </OfferedBy>
  <MarketingOverview Applicant="Y" Label="Marketing Course unit overview" Student="">
    <Content>&lt;p&gt;Early Universe (M)&lt;/p&gt;</Content>
  </MarketingOverview>
  <UnitOverview Applicant="" Label="Course unit overview" Student="Y">
    <Content>&lt;p&gt;Early Universe (M)&lt;/p&gt;</Content>
  </UnitOverview>
  <Aims Applicant="Y" Label="Aims" Student="Y">
    <Content>&lt;p&gt;Introduction to development of the cosmological model, its problems and their possible resolution within the framework of relativistic gravity and modern particle physics.&lt;/p&gt;</Content>
  </Aims>
  <LearningOutcomes Applicant="Y" Label="Learning outcomes" Student="Y">
    <Content>&lt;p&gt;On completion successful students will be able to:&lt;/p&gt;&lt;p&gt;1. formulate the linear theory of structure formation in the CDM model, obtain solutions in simple model cases of a one component universe.&lt;br/&gt;2. explain the problems of big bang cosmology and the way to solve them in inflationary theory.&lt;br/&gt;3. calculate basic cosmological parameters in inflationary slow roll models.&lt;br/&gt;4. indicate the relations of the Cosmic Microwave Background Radiation and cosmological parameters.&lt;br/&gt;5. discuss the evidence for an accelerating universe and the possible role of dark energy.&lt;/p&gt;</Content>
  </LearningOutcomes>
  <Knowledge Applicant="Y" Label="Knowledge and understanding" Student="Y">
    <Content></Content>
  </Knowledge>
  <IntellectualSkills Applicant="Y" Label="Intellectual skills" Student="Y">
    <Content></Content>
  </IntellectualSkills>
  <PracticalSkills Applicant="Y" Label="Practical skills" Student="Y">
    <Content></Content>
  </PracticalSkills>
  <TransferableSkills Applicant="Y" Label="Transferable skills and personal qualities" Student="Y">
    <Content></Content>
  </TransferableSkills>
  <EmployabilitySkillsList Applicant="Y" Label="Employability skills" Student="Y">
    <Skill>
      <SkillId></SkillId>
      <SkillDescription></SkillDescription>
    </Skill>
  </EmployabilitySkillsList>
  <Syllabus Applicant="Y" Label="Syllabus" Student="Y">
    <Content>&lt;ol&gt;&lt;li style="box-sizing:inherit;"&gt;Standard model of cosmology: Review&lt;ul&gt;&lt;li style="box-sizing:inherit;"&gt;Review of FRW universe&lt;/li&gt;&lt;li style="box-sizing:inherit;"&gt;Natural units&lt;/li&gt;&lt;li style="box-sizing:inherit;"&gt;Distance measures in FRW and conformal time&lt;/li&gt;&lt;li style="box-sizing:inherit;"&gt;Basic observational facts&lt;/li&gt;&lt;li style="box-sizing:inherit;"&gt;Neutrino decoupling and the radiation density&lt;/li&gt;&lt;li style="box-sizing:inherit;"&gt;A brief history of time&lt;/li&gt;&lt;/ul&gt;&lt;/li&gt;&lt;li style="box-sizing:inherit;"&gt;Cosmological perturbations and structure formation&lt;ul&gt;&lt;li style="box-sizing:inherit;"&gt;Overview of structure formation&lt;/li&gt;&lt;li style="box-sizing:inherit;"&gt;Jeans instability&lt;/li&gt;&lt;li style="box-sizing:inherit;"&gt;Relativistic perturbation theory&lt;/li&gt;&lt;li style="box-sizing:inherit;"&gt;Conformal Newtonian gauge&lt;/li&gt;&lt;li style="box-sizing:inherit;"&gt;Scalar perturbations in one component universe&lt;/li&gt;&lt;li style="box-sizing:inherit;"&gt;Multi-component universe - adiabatic and isocurvature perturbations&lt;/li&gt;&lt;li style="box-sizing:inherit;"&gt;Power spectra&lt;/li&gt;&lt;li style="box-sizing:inherit;"&gt;Suppression of power on small scales due to baryons and neutrinos&lt;/li&gt;&lt;/ul&gt;&lt;/li&gt;&lt;li style="box-sizing:inherit;"&gt;Cosmic microwave background&lt;ul&gt;&lt;li style="box-sizing:inherit;"&gt;Basic features of the angular power spectrum&lt;/li&gt;&lt;li style="box-sizing:inherit;"&gt;Recombination and photon decoupling&lt;/li&gt;&lt;li style="box-sizing:inherit;"&gt;Density and velocity fluctuations&lt;/li&gt;&lt;li style="box-sizing:inherit;"&gt;Sachs-Wolfe effects&lt;/li&gt;&lt;li style="box-sizing:inherit;"&gt;Future directions in CMB cosmology&lt;/li&gt;&lt;/ul&gt;&lt;/li&gt;&lt;li style="box-sizing:inherit;"&gt;Inflation&lt;ul&gt;&lt;li style="box-sizing:inherit;"&gt;Horizon and Flatness puzzles, primordial perturbations&lt;/li&gt;&lt;li style="box-sizing:inherit;"&gt;Definition of inflation and its solution of the horizon and flatness puzzles&lt;/li&gt;&lt;li style="box-sizing:inherit;"&gt;Potential formulation and slow roll dynamics&lt;/li&gt;&lt;li style="box-sizing:inherit;"&gt;Klein-Gordon field as a simple worked example&lt;/li&gt;&lt;li style="box-sizing:inherit;"&gt;Fluctuations generated during inflation&lt;/li&gt;&lt;li style="box-sizing:inherit;"&gt;Model zoo: large field, small field and hybrid models&lt;/li&gt;&lt;li style="box-sizing:inherit;"&gt;Connecting observations with theory&lt;/li&gt;&lt;li style="box-sizing:inherit;"&gt;Preheating and the transition to radiation domination&lt;/li&gt;&lt;/ul&gt;&lt;/li&gt;&lt;li style="box-sizing:inherit;"&gt;Dark energy&lt;ul&gt;&lt;li style="box-sizing:inherit;"&gt;Vacuum energy and timescale problems&lt;/li&gt;&lt;li style="box-sizing:inherit;"&gt;Cosmological constant&lt;/li&gt;&lt;li style="box-sizing:inherit;"&gt;Quintessence&lt;/li&gt;&lt;/ul&gt;&lt;/li&gt;&lt;/ol&gt;</Content>
  </Syllabus>
  <TeachingMethods Applicant="Y" Label="Teaching and learning methods" Student="Y">
    <Content></Content>
  </TeachingMethods>
  <AssessmentMethods Applicant="Y" Label="Assessment methods" Student="Y">
    <IntroText> </IntroText>
    <Method>
      <MethodId>1</MethodId>
      <MethodName>Written exam</MethodName>
      <MethodWeight>100%</MethodWeight>
    </Method>
  </AssessmentMethods>
  <FeedbackMethods Applicant="Y" Label="Feedback methods" Student="Y">
    <Content>&lt;p&gt;Will be available on students&amp;rsquo; individual written solutions to examples sheets, model answers will be issued. Several review sessions will be suggested during the semester.&lt;/p&gt;</Content>
  </FeedbackMethods>
  <RequirementsList Applicant="Y" Label="Pre/co-requisites" Student="Y">
    <Requirement>
      <UnitCode>PHYS30392</UnitCode>
      <UnitTitle>Cosmology</UnitTitle>
      <RequirementType>Pre-Requisite</RequirementType>
      <Description>Compulsory</Description>
    </Requirement>
    <Requirement>
      <UnitCode>PHYS40771</UnitCode>
      <UnitTitle>Gravitation (M,A)</UnitTitle>
      <RequirementType>Pre-Requisite</RequirementType>
      <Description>Compulsory</Description>
    </Requirement>
    <AdditionalRequirement></AdditionalRequirement>
  </RequirementsList>
  <AcademicPrograms Applicant="Y" Label="Academic programmes" Student="Y">
    <AcademicProgram>
      <Program></Program>
      <Plan></Plan>
      <Level></Level>
      <Requirement></Requirement>
    </AcademicProgram>
  </AcademicPrograms>
  <FreeChoice Applicant="Y" Label="Available as a free choice unit?" Student="Y">
    <Content>N</Content>
  </FreeChoice>
  <Accreditation Applicant="Y" Label="Accreditation" Student="Y">
    <Content></Content>
  </Accreditation>
  <RecommendedReading Applicant="Y" Label="Recommended reading" Student="Y">
    <Content>&lt;p&gt;Gorbunov D.S. &amp;amp; Rubakov V.A. Introduction to the Theory of the Early Universe: Cosmological Perturbations and Inflationary Theory, (World Scientific, 2011)&lt;br/&gt;Mukhanov, V.F. Physical Foundations of Cosmology, (CUP, 2005)&lt;br/&gt;Weinberg, S. Cosmology (OUP)&lt;/p&gt;</Content>
  </RecommendedReading>
  <StudyHours Applicant="Y" Label="Study hours" Student="Y">
    <IntroText> </IntroText>
    <ScheduledHours Applicant="Y" Label="Scheduled activity hours" Student="Y">
      <ActivityHours>
        <ActivityType>Assessment written exam</ActivityType>
        <Hours>2</Hours>
      </ActivityHours>
      <ActivityHours>
        <ActivityType>Lectures</ActivityType>
        <Hours>23</Hours>
      </ActivityHours>
    </ScheduledHours>
    <PlacementHours Applicant="Y" Label="Placement hours" Student="Y">
      <ActivityHours>
        <ActivityType></ActivityType>
        <Hours>0</Hours>
      </ActivityHours>
    </PlacementHours>
    <TotalHours Applicant="Y" Label="Independent study hours" Student="Y">
      <Hours>75</Hours>
    </TotalHours>
  </StudyHours>
  <Notes Applicant="Y" Label="Additional notes" Student="Y">
    <Content></Content>
  </Notes>
</CourseUnit>
